613:. At low frequencies these are actually expected to be so numerous that they form a source of (foreground) noise for LISA data analysis. At higher frequencies LISA is expected to detect and resolve around 25,000 galactic compact binaries. Studying the distribution of the masses, periods, and locations of this population, will teach us about the formation and evolution of binary systems in the galaxy. Furthermore, LISA will be able to resolve 10 binaries currently known from electromagnetic observations (and find ≈500 more with electromagnetic counterparts within one square degree). Joint study of these systems will allow inference on other dissipation mechanisms in these systems, e.g. through tidal interactions. One of the currently known binaries that LISA will be able to resolve is the white dwarf binary
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368:, each centred on one of the spacecraft, with the test masses defining the ends of the arms. The entire arrangement, which is ten times larger than the orbit of the Moon, will be placed in solar orbit at the same distance from the Sun as the Earth, but trailing the Earth by 20 degrees, and with the orbital planes of the three spacecraft inclined relative to the ecliptic by about 0.33 degree, which results in the plane of the triangular spacecraft formation being tilted 60 degrees from the plane of the ecliptic. The mean linear distance between the formation and the Earth will be 50 million kilometres.
830:
730:, GW150914, it was realized that a similar event would be detectable by LISA well before the merger. Based on the LIGO estimated event rates, it is expected that LISA will detect and resolve about 100 binaries that would merge a few weeks to months later in the LIGO detection band. LISA will be able to accurately predict the time of merger ahead of time and locate the event with 1 square degree on the sky. This will greatly aid the possibilities for searches for electromagnetic counterpart events.
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399:) and the stability of the constellation orbit (larger constellations are more sensitive to the gravitational effects of other planets, limiting the mission lifetime). Another length-dependent factor which must be compensated for is the "point-ahead angle" between the incoming and outgoing laser beams; the telescope must receive its incoming beam from where its partner was a few seconds ago, but
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detection of gravitational waves by the LIGO, ground-based detectors in
September 2015, NASA expressed interest in rejoining the mission as a junior partner. In response to an ESA call for mission proposals for the `Gravitational Universe' themed L3 mission, a mission proposal for a detector with three 2.5-million-kilometre arms again called LISA was submitted in January 2017.
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482:(LPF) was launched in 2015 to test the technology necessary to put a test mass in (almost) perfect free fall conditions. LPF consists of a single spacecraft with one of the LISA interferometer arms shortened to about 38 cm (15 in), so that it fits inside a single spacecraft. The spacecraft reached its operational location in heliocentric orbit at the
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program forward, and instructed the L1 candidate missions to present reduced cost versions that could be flown within ESA's budget. A reduced version of LISA was designed with only two 1-million-kilometre arms under the name NGO (New/Next
Gravitational wave Observatory). Despite NGO being ranked highest in terms of scientific potential, ESA decided to fly
356:
697:=4. EMRIs are interesting because they are slowly evolving, spending around 10 orbits and between a few months and a few years in the LISA sensitivity band before merging. This allows very accurate (up to an error of 1 in 10) measurements of the properties of the system, including the mass and spin of the central object and the mass and orbital elements (
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40:
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Littenberg, Tyson; McWilliams, Sean T.; Nelemans, Gijs; Petiteau, Antoine; Porter, Edward K.; Schutz, Bernard F.; Sesana, Alberto; Stebbins, Robin; Sumner, Tim; Vallisneri, Michele; Vitale, Stefano; Volonteri, Marta; Ward, Henry (17 Jan 2012). "ELISA: Astrophysics and cosmology in the millihertz regime".
1575:
Littenberg, Tyson; McWilliams, Sean T.; Nelemans, Gijs; Petiteau, Antoine; Porter, Edward K.; Schutz, Bernard F.; Sesana, Alberto; Stebbins, Robin; Sumner, Tim; Vallisneri, Michele; Vitale, Stefano; Volonteri, Marta; Ward, Henry (17 Jan 2012). "ELISA: Astrophysics and cosmology in the millihertz regime".
1492:
Littenberg, Tyson; McWilliams, Sean T.; Nelemans, Gijs; Petiteau, Antoine; Porter, Edward K.; Schutz, Bernard F.; Sesana, Alberto; Stebbins, Robin; Sumner, Tim; Vallisneri, Michele; Vitale, Stefano; Volonteri, Marta; Ward, Henry (17 Jan 2012). "ELISA: Astrophysics and cosmology in the millihertz regime".
1453:
Littenberg, Tyson; McWilliams, Sean T.; Nelemans, Gijs; Petiteau, Antoine; Porter, Edward K.; Schutz, Bernard F.; Sesana, Alberto; Stebbins, Robin; Sumner, Tim; Vallisneri, Michele; Vitale, Stefano; Volonteri, Marta; Ward, Henry (17 Jan 2012). "ELISA: Astrophysics and cosmology in the millihertz regime".
1414:
Littenberg, Tyson; McWilliams, Sean T.; Nelemans, Gijs; Petiteau, Antoine; Porter, Edward K.; Schutz, Bernard F.; Sesana, Alberto; Stebbins, Robin; Sumner, Tim; Vallisneri, Michele; Vitale, Stefano; Volonteri, Marta; Ward, Henry (17 Jan 2012). "ELISA: Astrophysics and cosmology in the millihertz regime".
838:: A beamsplitter (green line) splits coherent light (from the white box) into two beams which reflect off the mirrors (cyan oblongs); only one outgoing and reflected beam in each arm is shown, and separated for clarity. The reflected beams recombine and an interference pattern is detected (purple circle).
916:
L2 and L3 mission slots. A theme called "the
Gravitational Universe" was formulated with the reduced NGO rechristened eLISA as a straw-man mission. In November 2013, ESA announced that it selected "the Gravitational Universe" for its L3 mission slot (expected launch in 2034). Following the successful
2318:
Littenberg, Tyson; McWilliams, Sean T; Nelemans, Gijs; Petiteau, Antoine; Porter, Edward K; Schutz, Bernard F; Sesana, Alberto; Stebbins, Robin; Sumner, Tim; Vallisneri, Michele; Vitale, Stefano; Volonteri, Marta; Ward, Henry (21 June 2012). "Low-frequency gravitational-wave science with eLISA/NGO".
1162:
Littenberg, Tyson; McWilliams, Sean T; Nelemans, Gijs; Petiteau, Antoine; Porter, Edward K; Schutz, Bernard F; Sesana, Alberto; Stebbins, Robin; Sumner, Tim; Vallisneri, Michele; Vitale, Stefano; Volonteri, Marta; Ward, Henry (21 June 2012). "Low-frequency gravitational-wave science with eLISA/NGO".
896:
The first design studies for a gravitational-wave detector to be flown in space were performed in the 1980s under the name LAGOS (Laser Antena for
Gravitational radiation Observation in Space). LISA was first proposed as a mission to ESA in the early 1990s. First as a candidate for the M3-cycle, and
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LISA will also be able to detect the gravitational waves emanating from black hole binary mergers where the lighter black hole is in the intermediate black hole range (between 10 and 10 solar masses). In the case of both components being intermediate black holes between 600 and 10 solar masses, LISA
363:
The LISA mission's primary objective is to detect and measure gravitational waves produced by compact binary systems and mergers of supermassive black holes. LISA will observe gravitational waves by measuring differential changes in the length of its arms, as sensed by laser interferometry. Each of
900:
In the 2000s the joint ESA/NASA LISA mission was identified as a candidate for the 'L1' slot in ESA's Cosmic Vision 2015–2025 programme. However, due to budget cuts, NASA announced in early 2011 that it would not be contributing to any of ESA's L-class missions. ESA nonetheless decided to push the
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Gravitational wave signals from black holes could provide hints at a more fundamental theory of gravity. LISA will be able to test possible modifications of
Einstein's general theory of relativity, motivated by dark energy or dark matter. These could manifest, for example, through modifications of
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Extreme mass ratio inspirals (EMRIs) consist of a stellar compact object (<60 solar masses) on a slowly decaying orbit around a massive black hole of around 10 solar masses. For the ideal case of a prograde orbit around a (nearly) maximally spinning black hole, LISA will be able to detect these
451:
Unlike terrestrial gravitational-wave observatories, LISA cannot keep its arms "locked" in position at a fixed length. Instead, the distances between satellites vary significantly over each year's orbit, and the detector must keep track of the constantly changing distance, counting the millions of
808:
LISA will also search for currently unknown (and unmodelled) sources of gravitational waves. The history of astrophysics has shown that whenever a new frequency range/medium of detection is available new unexpected sources show up. This could for example include kinks and cusps in cosmic strings.
444:. Comparison between the observed laser beam frequency (in return beam) and the local laser beam frequency (sent beam) encodes the wave parameters. The principle of laser-interferometric inter-satellite ranging measurements was successfully implemented in the Laser Ranging Interferometer onboard
1613:
Amaro-Seoane, Pau; Aoudia, Sofiane; Babak, Stanislav; Binétruy, Pierre; Berti, Emanuele; Bohé, Alejandro; Caprini, Chiara; Colpi, Monica; Cornish, Neil J.; Danzmann, Karsten; Dufaux, Jean-François; Gair, Jonathan; Jennrich, Oliver; Jetzer, Philippe; Klein, Antoine; Lang, Ryan N.; Lobo, Alberto;
1574:
Amaro-Seoane, Pau; Aoudia, Sofiane; Babak, Stanislav; Binétruy, Pierre; Berti, Emanuele; Bohé, Alejandro; Caprini, Chiara; Colpi, Monica; Cornish, Neil J.; Danzmann, Karsten; Dufaux, Jean-François; Gair, Jonathan; Jennrich, Oliver; Jetzer, Philippe; Klein, Antoine; Lang, Ryan N.; Lobo, Alberto;
1491:
Amaro-Seoane, Pau; Aoudia, Sofiane; Babak, Stanislav; Binétruy, Pierre; Berti, Emanuele; Bohé, Alejandro; Caprini, Chiara; Colpi, Monica; Cornish, Neil J.; Danzmann, Karsten; Dufaux, Jean-François; Gair, Jonathan; Jennrich, Oliver; Jetzer, Philippe; Klein, Antoine; Lang, Ryan N.; Lobo, Alberto;
1452:
Amaro-Seoane, Pau; Aoudia, Sofiane; Babak, Stanislav; Binétruy, Pierre; Berti, Emanuele; Bohé, Alejandro; Caprini, Chiara; Colpi, Monica; Cornish, Neil J.; Danzmann, Karsten; Dufaux, Jean-François; Gair, Jonathan; Jennrich, Oliver; Jetzer, Philippe; Klein, Antoine; Lang, Ryan N.; Lobo, Alberto;
1413:
Amaro-Seoane, Pau; Aoudia, Sofiane; Babak, Stanislav; Binétruy, Pierre; Berti, Emanuele; Bohé, Alejandro; Caprini, Chiara; Colpi, Monica; Cornish, Neil J.; Danzmann, Karsten; Dufaux, Jean-François; Gair, Jonathan; Jennrich, Oliver; Jetzer, Philippe; Klein, Antoine; Lang, Ryan N.; Lobo, Alberto;
435:
in which two "transponder" satellites play the role of reflectors and one "master" satellite the roles of source and observer. When a gravitational wave passes the interferometer, the lengths of the two LISA arms vary due to spacetime distortions caused by the wave. Practically, LISA measures a
486:
L1 on 22 January 2016, where it underwent payload commissioning. Scientific research started on March 8, 2016. The goal of LPF was to demonstrate a noise level 10 times worse than needed for LISA. However, LPF exceeded this goal by a large margin, approaching the LISA requirement noise levels.
2317:
Amaro-Seoane, Pau; Aoudia, Sofiane; Babak, Stanislav; Binétruy, Pierre; Berti, Emanuele; Bohé, Alejandro; Caprini, Chiara; Colpi, Monica; Cornish, Neil J; Danzmann, Karsten; Dufaux, Jean-François; Gair, Jonathan; Jennrich, Oliver; Jetzer, Philippe; Klein, Antoine; Lang, Ryan N; Lobo, Alberto;
1161:
Amaro-Seoane, Pau; Aoudia, Sofiane; Babak, Stanislav; Binétruy, Pierre; Berti, Emanuele; Bohé, Alejandro; Caprini, Chiara; Colpi, Monica; Cornish, Neil J; Danzmann, Karsten; Dufaux, Jean-François; Gair, Jonathan; Jennrich, Oliver; Jetzer, Philippe; Klein, Antoine; Lang, Ryan N; Lobo, Alberto;
897:
later as 'cornerstone mission' for the 'Horizon 2000 plus' program. As the decade progressed, the design was refined to a triangular configuration of three spacecraft with three 5-million-kilometre arms. This mission was pitched as a joint mission between ESA and NASA in 1997.
879:
measures frequencies too low for LISA. The different types of gravitational wave measurement systems — LISA, NANOGrav and ground-based detectors — are complementary rather than competitive, much like astronomical observatories in different electromagnetic bands (e.g.,
395:, or 0.12 Hz ). As the satellites are free-flying, the spacing is easily adjusted before launch, with upper bounds being imposed by the sizes of the telescopes required at each end of the interferometer (which are constrained by the size of the launch vehicle's
2530:
Amaro-Seoane, Pau; Gair, Jonathan R; Freitag, Marc; Miller, M Coleman; Mandel, Ilya; Cutler, Curt J; Babak, Stanislav (7 September 2007). "Intermediate and extreme mass-ratio inspirals—astrophysics, science applications and detection using LISA".
674:≈ 2) LISA will be able to locate mergers within 100 square degrees on the night sky at least 24 hours before the actual merger, allowing electromagnetic telescopes to search for counterparts, with the potential of witnessing the formation of a
406:
The original 2008 LISA proposal had arms 5 million kilometres (5 Gm) long. When downscoped to eLISA in 2013, arms of 1 million kilometres were proposed. The approved 2017 LISA proposal has arms 2.5 million kilometres (2.5 Gm) long.
364:
the three LISA spacecraft contains two telescopes, two lasers and two test masses (each a 46 mm, roughly 2 kg, gold-coated cube of gold/platinum), arranged in two optical assemblies pointed at the other two spacecraft. These form
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A LISA-like detector is sensitive to the low-frequency band of the gravitational-wave spectrum, which contains many astrophysically interesting sources. Such a detector would observe signals from binary stars within our galaxy (the
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resonant arm cavities and signal recycling systems like terrestrial detectors, limiting its length-measurement accuracy. But with arms almost a million times longer, the motions to be detected are correspondingly larger.
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orbiting white dwarf binaries. The number of such detections in the Milky Way is estimated to range from 17 in a pessimistic scenario to more than 2000 in an optimistic scenario, and even extragalactic detections in the
7932:
714:
will be able to detect events up to redshifts around 1. In the case of an intermediate mass black hole spiralling into a massive black hole (between 10 and 10 solar masses) events will be detectable up to at least
705:) of the smaller object. EMRIs are expected to occur regularly in the centers of most galaxies and in dense star clusters. Conservative population estimates predict at least one detectable event per year for LISA.
281:
On 25 January 2024, the LISA Mission was formally adopted by ESA. This adoption recognises that the mission concept and technology are advanced enough that building the spacecraft and its instruments can commence.
5056:
2643:
Binétruy, Pierre; Bohé, Alejandro; Caprini, Chiara; Dufaux, Jean-François (13 June 2012). "Cosmological backgrounds of gravitational waves and eLISA/NGO: phase transitions, cosmic strings and other sources".
875:, are already in operation on Earth, but their sensitivity at low frequencies is limited by the largest practical arm lengths, by seismic noise, and by interference from nearby moving masses. Conversely,
277:
In
January 2017, LISA was proposed as a candidate mission. On June 20, 2017, the suggested mission received its clearance goal for the 2030s, and was approved as one of the main research missions of ESA.
3002:
Just as light comes in a spectrum, or a variety of wavelengths, so do gravitational waves. Different wavelengths point to different types of cosmic origins and require different flavors of detectors.
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with an absolute error of 0.01 (km/s)/Mpc. At larger ranges LISA events can (stochastically) be linked to electromagnetic counterparts, to further constrain the expansion curve of the universe.
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8023:
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301:, can pass unhindered by intervening mass. Launching LISA will add a new sense to scientists' perception of the universe and enable them to study phenomena that are invisible in normal light.
274:. In 2013, ESA selected 'The Gravitational Universe' as the theme for one of its three large projects in the 2030s whereby it committed to launch a space-based gravitational-wave observatory.
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The longer the arms, the more sensitive the detector is to long-period gravitational waves, but its sensitivity to wavelengths shorter than the arms is reduced (2,500,000 km is 8.3
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553:—less than the diameter of a helium atom—over a distance of a million kilometres, yielding a strain sensitivity of better than 1 part in 10 in the low-frequency band about a millihertz.
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258:(ESA). However, in 2011, NASA announced that it would be unable to continue its LISA partnership with the European Space Agency due to funding limitations. The project is a recognized
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666:< 3), it will be able to determine the spins of the components, which carry information about the past evolution of the components (e.g. whether they have grown primarily through
297:. Passing gravitational waves alternately squeeze and stretch space itself by a tiny amount. Gravitational waves are caused by energetic events in the universe and, unlike any other
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to monitor fluctuations in the Earth–spacecraft distance. By contrast, LISA is a dedicated mission that will use laser interferometry to achieve a much higher sensitivity. Other
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769:. The accuracy of such a determination is limited by the sample size and therefore the mission duration. With a mission lifetime of 4 years one expects to be able to determine
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511:(EPTA). The characteristic strain of potential astrophysical sources are also shown. To be detectable the characteristic strain of a signal must be above the noise curve.
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to determine the spacecraft's position relative to the mass, very precise thrusters adjust the spacecraft so that it follows, keeping itself centered around the mass.
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Previous searches for gravitational waves in space were conducted for short periods by planetary missions that had other primary science objectives (such as
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379:. The test mass floats free inside, effectively in free-fall, while the spacecraft around it absorbs all these local non-gravitational forces. Then, using
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Flanagan, Éanna É. (1998). "Measuring gravitational waves from binary black hole coalescences. I. Signal to noise for inspiral, merger, and ringdown".
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243:. The LISA concept features three spacecraft arranged in an equilateral triangle with each side 2.5 million kilometers long, flying in an Earth-like
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2007:
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718:=3. Since little is known about the population of intermediate mass black holes, there is no good estimate of the event rates for these events.
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LISA will be able to detect the nearly monochromatic gravitational waves emanating of close binaries consisting of two compact stellar objects (
549:—and extremely high detection sensitivity. A LISA-like instrument should be able to measure relative displacements with a resolution of 20
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mission had been experiencing technical delays, making it uncertain if the technology would be ready for the projected L1 launch date.
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755:< 0.1) through the detection of massive black hole mergers and EMRIs. Consequently, it can make an independent measurement of the
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Detector noise curves for LISA and eLISA as a function of frequency. They lie in between the bands for ground-based detectors like
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456:: changes with periods of less than a day are signals of interest, while changes with periods of a month or more are irrelevant.
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662:≈ 10. The most conservative population models expect at least a few such events to happen each year. For mergers closer by (
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526:. Indirect evidence of gravitational waves was derived from observations of the decreasing orbital periods of several
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Observing gravitational waves requires two things: a strong source of gravitational waves—such as the merger of two
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844:: A gravitational wave passing over the left arm (yellow) changes its length and thus the interference pattern.
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Tamanini, Nicola; Danielski, Camilla. "Listening to the gravitational wave sound of circumbinary exoplanets".
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LISA will be sensitive to the permanent displacement induced on probe masses by gravitational waves, known as
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LISA will be able to independently measure the redshift and distance of events occurring relatively close by (
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Wang, Gang; Ni, Wei-Tou (February 2013). "Numerical simulation of time delay interferometry for eLISA/NGO".
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LISA will be able to detect the gravitational waves from the merger of a pair of massive black holes with a
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View of amplified effects of a + polarized gravitational wave (stylized) on LISA laser beams / arms paths.
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2294:"Gravitational waves detected 100 years after Einstein's prediction | NSF – National Science Foundation"
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B. P. Abbott; et al. (2016). "Observation of
Gravitational Waves from a Binary Black Hole Merger".
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2015:
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with a period of 6.91 minutes, the second shortest period binary white dwarf pair discovered to date.
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247:. The distance between the satellites is precisely monitored to detect a passing gravitational wave.
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Cornish, Neil; Robson, Travis (29 March 2017). "Galactic binary science with the new LISA design".
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seeks to use direct measurements of gravitational waves to study astrophysical systems and to test
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LISA spacecraft orbitography and interferometer – yearly-periodic revolution in heliocentric orbit.
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3118:"CALL FOR MISSION CONCEPTS FOR THE LARGE-SIZE 'L3' MISSION OPPORTUNITY IN ESA'S SCIENCE PROGRAMME"
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2038:"Sub-Femto-g Free Fall for Space-Based Gravitational Wave Observatories: LISA Pathfinder Results"
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1623:
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orbiting a supermassive black hole. There are also more speculative signals such as signals from
445:
344:
286:
244:
228:
158:
3573:
2803:
Sesana, Alberto (2016). "Prospects for
Multiband Gravitational-Wave Astronomy after GW150914".
8139:
7886:
7822:
7732:
7553:
6783:
6681:
6664:
6642:
5811:
5396:
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wavelengths by which the distance changes each second. Then, the signals are separated in the
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328:
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7955:
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4009:
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5564:
4513:
4132:
4117:
1221:
906:
740:
614:
519:
479:
473:
396:
165:
2753:"The gravitational-wave detection of exoplanets orbiting white dwarf binaries using LISA"
2349:
1866:
1193:
2955:
2947:
2890:
2826:
2675:
2667:
2611:
2554:
2500:
2447:
2402:
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2149:
2053:
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1813:
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1185:
8423:
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6493:
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4986:
4549:
3958:
3631:
3141:
2168:
2123:
574:
483:
316:
294:
175:
2562:
2455:
1534:"Circumbinary exoplanets and brown dwarfs with the Laser Interferometer Space Antenna"
8433:
8305:
8287:
8117:
6636:
6577:
6444:
6267:
4881:
4770:
4484:
4148:
4068:
3889:
3743:
3117:
3078:
Danzmann, Karsten; The eLISA Consortium (24 May 2013). "The
Gravitational Universe".
2906:
2867:
Enrico, Barausse; et al. (2020). "Prospects for fundamental physics with LISA".
2850:
2683:
2279:
2212:
1939:
1874:
1821:
945:
913:
856:
582:
535:
527:
500:
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340:
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orbiting such binaries, and possibly other sources of cosmological origin, such as a
271:
2971:
2752:
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2570:
2516:
2410:
2357:
1201:
8418:
8351:
8293:
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6620:
6439:
5041:
4865:
4029:
2834:
2463:
2263:
2062:
2037:
1923:
602:
7960:
7848:
4140:
1559:
1532:
Danielski, Camilla; Korol, Valeriya; Tamanini, Nicola; Rossi, Elena Maria (2019).
3100:"Selected: The Gravitational Universe ESA decides on next Large Mission Concepts"
2987:"Scientists have two ways to spot gravitational waves. Here are some other ideas"
1889:
1113:
8299:
8048:
7901:
7843:
7838:
7789:
7749:
7726:
7674:
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7662:
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6651:
6488:
5340:
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4375:
4217:
881:
702:
626:
598:
415:
392:
324:
135:
3240:
2898:
1215:
Selected: The
Gravitational Universe ESA decides on next Large Mission Concepts
7921:
7679:
7630:
7392:
7043:
7035:
7011:
6982:
6962:
6944:
6930:
6753:
5819:
5131:
4976:
4685:
3995:
3967:
3753:
2768:
2204:
1083:
651:
647:
606:
546:
372:
308:
2963:
2508:
8178:
8151:
8123:
7926:
7808:
7685:
7433:
7407:
7332:
7155:
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6918:
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6226:
5484:
4897:
4597:
4412:
4303:
4052:
3947:
3517:
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3414:
3343:
2620:
2585:
610:
558:
550:
298:
290:
232:
2842:
2424:
Stroeer, A; Vecchio, A (7 October 2006). "The LISA verification binaries".
2371:
Nelemans, Gijs (7 May 2009). "The Galactic gravitational wave foreground".
2271:
2177:
2100:
2081:
1931:
1325:"Gravitational wave mission selected, planet-hunting mission moves forward"
3194:
1890:"In-Orbit Performance of the GRACE Follow-on Laser Ranging Interferometer"
401:
send its outgoing beam to where its partner will be a few seconds from now
8208:
8190:
8184:
8157:
8000:
7875:
7869:
7813:
7754:
6882:
6864:
6824:
6759:
6689:
6498:
6262:
6257:
5771:
5707:
5548:
5260:
5021:
4921:
4913:
4817:
4754:
4565:
4428:
4254:
4246:
3952:
3926:
3828:
3822:
3817:
3807:
3802:
3797:
3792:
3787:
3568:
3563:
2545:
2438:
2140:
921:
885:
655:
336:
235:—from astronomical sources. LISA will be the first dedicated space-based
112:
6183:
2158:
1982:
355:
8202:
8166:
8084:
8028:
7990:
7911:
7783:
7759:
7397:
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7265:
7247:
7241:
7179:
7173:
7167:
6888:
6614:
6414:
6394:
6334:
6239:
5994:
5925:
5763:
5412:
5372:
5268:
5179:
5171:
5163:
5155:
5147:
5139:
4857:
4841:
4809:
3686:
2072:
954:(DECIGO) – proposed Japanese space based gravitational-wave observatory
523:
39:
7516:
2491:
739:
the propagation of gravitational waves, or through the possibility of
8172:
8111:
7951:
7906:
7891:
7863:
7853:
7636:
7387:
7019:
6789:
6723:
6553:
6098:
5835:
5691:
5404:
5348:
5316:
5308:
5231:
5211:
4801:
4778:
4677:
4653:
4492:
4319:
4279:
4156:
3974:
3522:
3333:
2586:"Expectations for extreme-mass-ratio bursts from the Galactic Centre"
2095:
Moore, Christopher; Cole, Robert; Berry, Christopher (19 July 2013).
872:
675:
566:
312:
912:
Soon afterwards, ESA announced it would be selecting themes for its
788:
generated in the early universe through various channels, including
8346:
4086:
2881:
2817:
2788:
2246:
1906:
1849:
1550:
1399:"Gravitational-Wave Detetectors Get Ready to Hunt for the Big Bang"
625:
LISA will also be able to detect the presence of large planets and
8135:
7576:
7229:
6900:
6816:
6765:
6711:
6068:
6063:
5866:
5803:
5723:
5660:
5655:
5650:
5645:
5640:
5635:
5625:
5556:
5420:
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5332:
5324:
5292:
5284:
4889:
4262:
3748:
3537:
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3384:
3084:
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2658:
2602:
2385:
2332:
1796:
1628:
1589:
1506:
1467:
1428:
1176:
828:
494:
414:
354:
125:
905:(JUICE) as its L1 mission. One of the main concerns was that the
371:
To eliminate non-gravitational forces such as light pressure and
7858:
7818:
7362:
7337:
7317:
6108:
6058:
6016:
5989:
5909:
5500:
4905:
4589:
3578:
3527:
3512:
3502:
3180:
3102:. Max Planck Institute for Gravitational Physics. Archived from
2699:"Discovering the shortest orbital period eclipsing binary known"
1768:
969:
967:
864:
634:
might be possible, far beyond the current capabilities of other
259:
251:
7520:
6530:
6187:
4090:
3244:
76:
8231:
3166:
3136:
979:
262:
experiment (RE8). A scaled-down design initially known as the
920:
As of January 2024, LISA is expected to launch in 2035 on an
2723:"ZTF found Dead Stars Whipping Around Each Other in Minutes"
670:
or mergers). For mergers around the peak of star formation (
227:) is a planned space probe to detect and accurately measure
239:. It aims to measure gravitational waves directly by using
3212:
1006:"eLISA, The First Gravitational Wave Observatory in Space"
3227:
833:
Simplified operation of a gravitational wave observatory
2191:
Castelvecchi, Davide; Witze, Witze (February 11, 2016).
1767:. Stanford 2008 Position Navigation and Time Symposium.
1761:
LISA: Drag-free Formation Flying at 5 million kilometers
1347:"Capturing the ripples of spacetime: LISA gets go-ahead"
1057:
975:"Capturing the ripples of spacetime: LISA gets go-ahead"
952:
Deci-hertz Interferometer Gravitational wave Observatory
459:
This difference means that LISA cannot use high-finesse
375:
on the test masses, each spacecraft is constructed as a
285:
The LISA mission is designed for direct observation of
270:) was proposed as one of three large projects in ESA's
250:
The LISA project started out as a joint effort between
8335:
27:
European space mission to measure gravitational waves
585:
and primordial gravitational waves generated during
8278:
8230:
8057:
8014:
7942:
7799:
7712:
7705:
7655:
7586:
7561:
7552:
7421:
7283:
7212:
7142:
7074:
6851:
6700:
6595:
6546:
6539:
6481:
6460:
6348:
6327:
6276:
6248:
6225:
6122:
5977:
5878:
5847:
5100:
4957:
4794:
4697:
4512:
4403:
4237:
4192:
4131:
4124:
3988:
3935:
3904:
3844:
3770:
3763:
3736:
3703:
3669:
3653:
3644:
3624:
3603:
3587:
3556:
3495:
3484:
3439:
3423:
3357:
3316:
3305:
3296:
2697:Community, Nature Research Astronomy (2019-07-24).
1983:"First locks released from LISA Pathfinder's cubes"
184:
174:
164:
154:
149:
131:
118:
108:
100:
95:
71:
61:
53:
2862:
2860:
2584:Berry, C. P. L.; Gair, J. R. (12 September 2013).
2014:. eLISA Science.org. March 8, 2016. Archived from
1235:"ESA's new vision to study the invisible universe"
1136:"RE8/LISA: The Laser Interferometer Space Antenna"
2590:Monthly Notices of the Royal Astronomical Society
1527:
1525:
440:between one local laser and one distant laser by
6309:Space Applications and Telecommunications Centre
3012:
3010:
1276:
1274:
1272:
654:all the way back to their earliest formation at
2124:"Testing General Relativity with Pulsar Timing"
1649:
1647:
1270:
1268:
1266:
1264:
1262:
1260:
1258:
1256:
1254:
1252:
924:, two years earlier than previously announced.
8460:Interferometric gravitational-wave instruments
6319:Space Telescope European Coordinating Facility
2646:Journal of Cosmology and Astroparticle Physics
2193:"Einstein's gravitational waves found at last"
2012:Max Planck Institute for Gravitational Physics
1000:
998:
7532:
6199:
4102:
3825:(first-ever possible light from bh-bh merger)
3256:
2751:Tamanini, Nicola; Danielski, Camilla (2019).
339:, and speculative astrophysical objects like
8:
3018:"The Gravitational Universe (science theme)"
2008:"LISA Pathfinder begins its science mission"
1082:. NASA/US Federal Government. Archived from
32:
7709:
7558:
7539:
7525:
7517:
6543:
6527:
6468:European Launcher Development Organisation
6222:
6206:
6192:
6184:
4128:
4109:
4095:
4087:
3767:
3650:
3492:
3313:
3302:
3263:
3249:
3241:
3044:
3042:
2097:"Gravitational Wave Detectors and Sources"
1888:Abich, Klaus; et al. (19 July 2019).
1282:"LISA: Laser Interferometer Space Antenna"
304:Potential sources for signals are merging
38:
31:
3209:"LISA International Science Team website"
3083:
2937:
2880:
2816:
2787:
2657:
2619:
2601:
2544:
2490:
2437:
2384:
2331:
2245:
2167:
2157:
2139:
2071:
2061:
1905:
1848:
1795:
1627:
1588:
1549:
1505:
1466:
1427:
1401:. Scientific American. 17 September 2013.
1175:
784:LISA will be sensitive to the stochastic
3837:(first black hole - neutron star merger)
3027:. University of Bicocca. 4 February 2014
8342:
963:
765:that does not depend on the use of the
722:Multi-band gravitational wave astronomy
571:extreme-mass-ratio inspirals and bursts
538:project announced that it had directly
315:, massive black holes orbited by small
2922:"The gravitational-wave memory effect"
1758:Byer, Robert L. (November 5–6, 2008).
1307:"Europe selects grand gravity mission"
44:Artist's conception of LISA spacecraft
8320:List of proposed missions to the Moon
6430:Space Situational Awareness Programme
1989:. ESA Press Release. February 3, 2016
1837:Journal of Physics: Conference Series
709:Intermediate mass black hole binaries
7:
8325:List of proposed space observatories
7692:Chinese Crewed Lunar Landing Mission
7477:
6473:European Space Research Organisation
6289:Space Research and Technology Centre
3395:Stanford gravitational wave detector
3059:. Rabould University Nijimegen. 2012
2985:Conover, Emily (15 September 2023).
825:Other gravitational-wave experiments
431:. Its three satellites form a giant
7501:
2703:Nature Research Astronomy Community
8450:European Space Agency space probes
3547:European Gravitational Observatory
1735:. eLISA Consortium. Archived from
1709:. eLISA Consortium. Archived from
1683:. eLISA Consortium. Archived from
1657:. eLISA Consortium. Archived from
1375:. eLISA Consortium. Archived from
1287:. LISA Consortium. 20 January 2017
1034:. eLISA Consortium. Archived from
1008:. eLISA Consortium. Archived from
728:first gravitational wave detection
726:Following the announcement of the
264:New Gravitational-wave Observatory
221:Laser Interferometer Space Antenna
33:Laser Interferometer Space Antenna
25:
18:New Gravitational wave Observatory
7985:Nancy Grace Roman Space Telescope
6140:List of proposed space telescopes
4826:Nancy Grace Roman Space Telescope
3831:(first-ever "mass gap" collision)
3140:. 8 November 2021. Archived from
1080:"President's FY12 Budget Request"
8417:
8405:
8393:
8381:
8369:
8357:
8345:
7500:
7488:
7476:
7465:
7464:
6294:ESA Centre for Earth Observation
6168:
6167:
2036:Armano, M.; et al. (2016).
1106:"Recognized Experiments at CERN"
636:detection methods for exoplanets
425:gravitational wave-observatories
5047:Nautilus Deep Space Observatory
1961:"ESA: Lisa Pathfinder overview"
1140:The CERN Experimental Programme
747:Probe expansion of the universe
231:—tiny ripples in the fabric of
57:Gravitational waves observation
7313:Columbus Man-Tended Free Flyer
3288:Gravitational-wave observatory
3050:"eLISA (or NGO): the New LISA"
2835:10.1103/PhysRevLett.116.231102
2350:10.1088/0264-9381/29/12/124016
2264:10.1103/PhysRevLett.116.061102
2063:10.1103/PhysRevLett.116.231101
1924:10.1103/PhysRevLett.123.031101
1867:10.1088/1742-6596/840/1/012024
1194:10.1088/0264-9381/29/12/124016
1110:The CERN Scientific Committees
1032:"eLISA, Partners and Contacts"
794:cosmological phase transitions
734:Fundamental black hole physics
579:cosmological phase transitions
366:Michelson-like interferometers
237:gravitational-wave observatory
1:
6150:List of heliophysics missions
3980:Gravitational wave background
3532:LIGO Scientific Collaboration
2956:10.1088/0264-9381/27/8/084036
2926:Classical and Quantum Gravity
2676:10.1088/1475-7516/2012/06/027
2533:Classical and Quantum Gravity
2426:Classical and Quantum Gravity
2403:10.1088/0264-9381/26/9/094030
2373:Classical and Quantum Gravity
2320:Classical and Quantum Gravity
1814:10.1088/0264-9381/30/6/065011
1784:Classical and Quantum Gravity
1681:"eLISA: distance measurement"
1373:"eLISA: Science Context 2028"
1164:Classical and Quantum Gravity
798:spontaneous symmetry breaking
786:gravitational wave background
780:Gravitational wave background
333:cosmological phase transition
3783:First observation (GW150914)
3569:TAMA 20, later known as LISM
3272:Gravitational-wave astronomy
2128:Living Reviews in Relativity
1655:"eLISA: the mission concept"
1538:Astronomy & Astrophysics
682:Extreme mass ratio inspirals
540:detected gravitational waves
516:Gravitational-wave astronomy
509:European Pulsar Timing Array
321:extreme mass ratio inspirals
6130:Great Observatories program
3917:Tests of general relativity
2920:Favata, Marc (2010-04-21).
2563:10.1088/0264-9381/24/17/R01
2456:10.1088/0264-9381/23/19/S19
1733:"eLISA: dragfree operation"
1560:10.1051/0004-6361/201936729
861:gravitational wave antennas
819:gravitational memory effect
688:Extreme mass ratio inspiral
621:Planets of compact binaries
573:produced by a stellar-mass
478:An ESA test mission called
289:, which are distortions of
8496:
8163:ISS Deorbit Vehicle (2030)
7383:Mars sample return mission
7203:European Data Relay System
6883:Meteosat Second Generation
6796:James Webb Space Telescope
6658:Jupiter Icy Moons Explorer
6340:European Data Relay System
6314:Concurrent Design Facility
5621:Orbiting Solar Observatory
3579:Caltech 40m interferometer
2899:10.1007/s10714-020-02691-1
2122:Stairs, Ingrid H. (2003).
1058:"LISA on the NASA website"
903:Jupiter Icy Moons Explorer
857:microwave Doppler tracking
685:
642:Massive black hole mergers
542:from a black hole merger.
471:
8315:
7456:
7006:Meteosat Third Generation
6865:Meteosat First Generation
6526:
6514:Planetary Science Archive
6299:European Astronaut Centre
6221:
6173:Category:Space telescopes
6163:
3278:
3195:"LISA Pathfinder mission"
3167:"eLISA Consortium portal"
2769:10.1038/s41550-019-0807-y
2727:Zwicky Transient Facility
2205:10.1038/nature.2016.19361
942:– proposed LISA successor
593:Galactic compact binaries
198:
194:
145:
141:
91:
87:
49:
37:
8266:Uranus Orbiter and Probe
6135:List of space telescopes
4020:Supermassive black holes
3132:"LISA | Mission Summary"
2509:10.1103/PhysRevD.57.4535
563:supermassive black holes
534:. In February 2016, the
433:Michelson interferometer
6425:Living Planet Programme
6284:Space Operations Centre
3859:Resonant mass detectors
2234:Physical Review Letters
1963:. European Space Agency
1894:Physical Review Letters
1353:. European Space Agency
934:Beyond Einstein program
561:); signals from binary
6736:Hubble Space Telescope
6304:Space Astronomy Centre
5461:HEAO-2 (Einstein Obs.)
1112:. CERN. Archived from
846:
800:, and cosmic strings.
767:cosmic distance ladder
587:cosmological inflation
512:
420:
360:
8465:Proposed space probes
8130:Venus Orbiter Mission
6533:Projects and missions
6215:European Space Agency
5082:Space Solar Telescope
4044:Rotating neutron star
3855:Laser interferometers
2621:10.1093/mnras/stt1543
1707:"eLISA: key features"
832:
498:
418:
358:
256:European Space Agency
155:Reference system
7133:European Robotic Arm
6977:Sentinel-5 Precursor
6155:List of planetariums
5057:NRO donation to NASA
3936:Effects / properties
3865:Atom interferometers
3778:List of observations
3705:Pulsar timing arrays
3228:"NASA LISA homepage"
505:pulsar timing arrays
429:laser interferometry
241:laser interferometry
8455:Future spaceflights
7547:Future spaceflights
7458:Future missions in
6504:European Space Camp
6235:Guiana Space Centre
5851:(Mission completed)
4133:Radio and Microwave
4025:Stellar black holes
4005:quantum fluctuation
3885:Pulsar timing array
3872:Indirect detection
3812:neutron star merger
3595:INDIGO (LIGO-India)
3181:"ESA LISA homepage"
3144:on 10 November 2021
2948:2010CQGra..27h4036F
2891:2020GReGr..52...81B
2827:2016PhRvL.116w1102S
2668:2012JCAP...06..027B
2612:2013MNRAS.435.3521B
2555:2007CQGra..24R.113A
2501:1998PhRvD..57.4535F
2448:2006CQGra..23S.809S
2395:2009CQGra..26i4030N
2342:2012CQGra..29l4016A
2256:2016PhRvL.116f1102A
2159:10.12942/lrr-2003-5
2150:2003LRR.....6....5S
2054:2016PhRvL.116w1101A
1916:2019PhRvL.123c1101A
1859:2017JPhCS.840a2024C
1806:2013CQGra..30f5011W
1638:2013GWN.....6....4A
1599:2013GWN.....6....4A
1516:2013GWN.....6....4A
1477:2013GWN.....6....4A
1438:2013GWN.....6....4A
1186:2012CQGra..29l4016A
532:Hulse–Taylor pulsar
427:, LISA is based on
411:Detection principle
377:zero-drag satellite
351:Mission description
287:gravitational waves
229:gravitational waves
34:
7619:Boeing Starliner-1
7308:Ceres Polar Lander
7143:Telecommunications
5788:Suzaku (Astro-EII)
5613:OAO-3 (Copernicus)
5597:Mikhailo Lomonosov
5445:Hinotori (Astro-A)
5052:New Worlds Mission
3912:General relativity
3616:Einstein Telescope
3518:Fermilab holometer
3283:Gravitational wave
1739:on 5 December 2013
1713:on 5 December 2013
1687:on 5 December 2013
1661:on 5 December 2013
1379:on 21 October 2014
1220:2016-10-03 at the
1038:on 5 December 2013
1012:on 5 December 2013
847:
650:between 10 and 10
513:
442:light interference
421:
381:capacitive sensing
361:
335:shortly after the
329:substellar objects
327:of compact stars,
293:travelling at the
245:heliocentric orbit
150:Orbital parameters
8475:Space-based laser
8333:
8332:
8274:
8273:
8140:Comet Interceptor
8104:Rosalind Franklin
7823:Lunar Trailblazer
7701:
7700:
7514:
7513:
7452:
7451:
7070:
7069:
6852:Earth observation
6682:Comet Interceptor
6673:Rosalind Franklin
6645:Trace Gas Orbiter
6596:Planetary science
6522:
6521:
6435:Science Programme
6181:
6180:
6079:SIM & SIMlite
5453:Hisaki (SPRINT-A)
5413:Hakucho (CORSA-b)
4972:Astro-1 Telescope
4790:
4789:
4084:
4083:
3900:
3899:
3851:Direct detection
3699:
3698:
3695:
3694:
3677:Big Bang Observer
3640:
3639:
3480:
3479:
2539:(17): R113–R169.
2479:Physical Review D
2432:(19): S809–S817.
2018:on April 19, 2016
1611:See sect. 1.1 in
1572:See sect. 7.2 in
1489:See sect. 3.3 in
1450:See sect. 4.3 in
1411:See sect. 5.2 in
983:. 25 January 2024
940:Big Bang Observer
741:hairy black holes
632:Magellanic Clouds
423:Like most modern
345:domain boundaries
311:at the centre of
217:
216:
16:(Redirected from
8487:
8470:Space telescopes
8440:CERN experiments
8422:
8421:
8410:
8409:
8408:
8398:
8397:
8396:
8386:
8385:
8384:
8374:
8373:
8362:
8361:
8360:
8350:
8349:
8341:
7710:
7559:
7541:
7534:
7527:
7518:
7504:
7503:
7492:
7480:
7479:
7468:
7467:
7444:Schiaparelli EDM
7303:Calathus Mission
7127:Georges Lemaître
7085:ISS contribution
6544:
6528:
6223:
6208:
6201:
6194:
6185:
6171:
6170:
5970:
5966:Hitomi (Astro-H)
5962:
5954:
5946:
5938:
5930:
5922:
5914:
5906:
5898:
5890:
5871:
5863:
5852:
5840:
5832:
5824:
5816:
5808:
5800:
5792:
5784:
5776:
5768:
5760:
5752:
5744:
5736:
5728:
5720:
5712:
5704:
5696:
5688:
5680:
5672:
5617:
5609:
5601:
5593:
5585:
5577:
5569:
5561:
5553:
5545:
5537:
5529:
5521:
5513:
5505:
5497:
5489:
5481:
5473:
5465:
5457:
5449:
5441:
5433:
5425:
5417:
5409:
5401:
5393:
5385:
5377:
5369:
5361:
5353:
5345:
5337:
5329:
5321:
5313:
5305:
5297:
5289:
5281:
5273:
5265:
5257:
5249:
5241:
5216:
5208:
5200:
5192:
5184:
5176:
5168:
5160:
5152:
5144:
5136:
5128:
5120:
5112:
4950:
4942:
4934:
4926:
4918:
4910:
4902:
4894:
4886:
4878:
4870:
4862:
4854:
4846:
4838:
4830:
4822:
4814:
4806:
4783:
4775:
4767:
4759:
4751:
4743:
4735:
4727:
4719:
4711:
4700:or unclassified)
4690:
4682:
4674:
4666:
4658:
4650:
4642:
4634:
4626:
4618:
4610:
4602:
4594:
4586:
4578:
4570:
4562:
4554:
4546:
4538:
4530:
4505:
4497:
4489:
4481:
4473:
4465:
4457:
4449:
4445:Hinode (Solar-B)
4441:
4433:
4425:
4417:
4396:
4388:
4380:
4372:
4364:
4356:
4348:
4340:
4336:Hinode (Solar-B)
4332:
4324:
4316:
4308:
4300:
4292:
4284:
4276:
4268:
4259:
4251:
4230:
4222:
4214:
4206:
4185:
4177:
4169:
4161:
4153:
4145:
4129:
4118:Space telescopes
4111:
4104:
4097:
4088:
4016:Binary inspiral
4010:Phase transition
4001:Cosmic inflation
3768:
3651:
3493:
3314:
3303:
3265:
3258:
3251:
3242:
3237:
3235:
3234:
3223:
3221:
3220:
3211:. Archived from
3204:
3202:
3201:
3190:
3188:
3187:
3176:
3174:
3173:
3154:
3153:
3151:
3149:
3128:
3122:
3121:
3114:
3108:
3107:
3096:
3090:
3089:
3087:
3075:
3069:
3068:
3066:
3064:
3054:
3046:
3037:
3036:
3034:
3032:
3022:
3014:
3005:
3004:
2999:
2997:
2982:
2976:
2975:
2941:
2917:
2911:
2910:
2884:
2864:
2855:
2854:
2820:
2800:
2794:
2793:
2791:
2779:
2773:
2772:
2757:Nature Astronomy
2748:
2742:
2741:
2739:
2738:
2729:. Archived from
2719:
2713:
2712:
2710:
2709:
2694:
2688:
2687:
2661:
2640:
2634:
2633:
2623:
2605:
2596:(4): 3521–3540.
2581:
2575:
2574:
2548:
2546:astro-ph/0703495
2527:
2521:
2520:
2494:
2485:(8): 4535–4565.
2474:
2468:
2467:
2441:
2439:astro-ph/0605227
2421:
2415:
2414:
2388:
2368:
2362:
2361:
2335:
2314:
2308:
2307:
2305:
2304:
2290:
2284:
2283:
2249:
2229:
2223:
2222:
2220:
2219:
2188:
2182:
2181:
2171:
2161:
2143:
2141:astro-ph/0307536
2119:
2113:
2112:
2110:
2108:
2103:on 16 April 2014
2099:. Archived from
2092:
2086:
2085:
2075:
2065:
2033:
2027:
2026:
2024:
2023:
2004:
1998:
1997:
1995:
1994:
1979:
1973:
1972:
1970:
1968:
1957:
1951:
1950:
1948:
1946:
1909:
1885:
1879:
1878:
1852:
1832:
1826:
1825:
1799:
1779:
1773:
1772:
1766:
1755:
1749:
1748:
1746:
1744:
1729:
1723:
1722:
1720:
1718:
1703:
1697:
1696:
1694:
1692:
1677:
1671:
1670:
1668:
1666:
1651:
1642:
1641:
1631:
1609:
1603:
1602:
1592:
1570:
1564:
1563:
1553:
1529:
1520:
1519:
1509:
1487:
1481:
1480:
1470:
1448:
1442:
1441:
1431:
1409:
1403:
1402:
1395:
1389:
1388:
1386:
1384:
1369:
1363:
1362:
1360:
1358:
1343:
1337:
1336:
1334:
1332:
1321:
1315:
1314:
1303:
1297:
1296:
1294:
1292:
1286:
1278:
1247:
1246:
1244:
1242:
1231:
1225:
1212:
1206:
1205:
1179:
1158:
1152:
1151:
1149:
1147:
1132:
1126:
1125:
1123:
1121:
1102:
1096:
1095:
1093:
1091:
1076:
1070:
1069:
1067:
1065:
1054:
1048:
1047:
1045:
1043:
1028:
1022:
1021:
1019:
1017:
1002:
993:
992:
990:
988:
971:
757:Hubble parameter
678:after a merger.
454:frequency domain
96:Start of mission
83:
80:
78:
42:
35:
21:
8495:
8494:
8490:
8489:
8488:
8486:
8485:
8484:
8480:2035 in science
8430:
8429:
8428:
8416:
8406:
8404:
8394:
8392:
8382:
8380:
8368:
8358:
8356:
8344:
8336:
8334:
8329:
8311:
8280:
8270:
8226:
8053:
8010:
7938:
7795:
7697:
7651:
7613:Axiom Mission 4
7582:
7548:
7545:
7515:
7510:
7448:
7417:
7285:
7279:
7260:LISA Pathfinder
7217:
7215:
7208:
7138:
7121:Albert Einstein
7109:Johannes Kepler
7066:
6847:
6705:
6703:
6696:
6591:
6535:
6518:
6477:
6456:
6344:
6323:
6272:
6250:Launch vehicles
6244:
6217:
6212:
6182:
6177:
6159:
6145:X-ray telescope
6118:
6000:Constellation-X
5973:
5968:
5960:
5952:
5944:
5936:
5928:
5920:
5912:
5904:
5896:
5888:
5874:
5869:
5861:
5850:
5849:
5843:
5838:
5836:Yokoh (Solar-A)
5830:
5822:
5814:
5806:
5804:Tenma (Astro-B)
5798:
5790:
5782:
5774:
5766:
5758:
5750:
5742:
5734:
5726:
5718:
5710:
5702:
5694:
5686:
5678:
5670:
5615:
5607:
5599:
5591:
5583:
5575:
5567:
5565:LISA Pathfinder
5559:
5551:
5543:
5535:
5527:
5519:
5511:
5503:
5495:
5487:
5479:
5471:
5463:
5455:
5447:
5439:
5431:
5423:
5421:HALCA (MUSES-B)
5415:
5407:
5399:
5397:Ginga (Astro-C)
5391:
5383:
5375:
5367:
5359:
5351:
5343:
5335:
5327:
5319:
5311:
5303:
5295:
5287:
5279:
5271:
5263:
5255:
5247:
5239:
5214:
5206:
5198:
5190:
5182:
5174:
5166:
5158:
5150:
5142:
5134:
5126:
5118:
5116:Akari (Astro-F)
5110:
5096:
4953:
4948:
4940:
4932:
4924:
4916:
4908:
4900:
4892:
4884:
4876:
4868:
4860:
4852:
4844:
4836:
4828:
4820:
4812:
4804:
4786:
4781:
4773:
4765:
4757:
4749:
4741:
4733:
4725:
4717:
4709:
4699:
4698:Other (particle
4693:
4688:
4680:
4672:
4664:
4656:
4648:
4640:
4632:
4624:
4616:
4608:
4600:
4592:
4584:
4576:
4568:
4560:
4552:
4544:
4536:
4528:
4508:
4503:
4495:
4487:
4479:
4471:
4463:
4455:
4447:
4439:
4431:
4423:
4415:
4399:
4394:
4386:
4378:
4370:
4362:
4354:
4346:
4338:
4330:
4322:
4314:
4306:
4298:
4290:
4282:
4274:
4266:
4257:
4249:
4233:
4228:
4220:
4212:
4204:
4188:
4183:
4175:
4167:
4159:
4151:
4143:
4120:
4115:
4085:
4080:
3989:Types / sources
3984:
3931:
3922:Metric theories
3896:
3840:
3759:
3732:
3691:
3665:
3647:interferometers
3646:
3636:
3620:
3611:Cosmic Explorer
3599:
3583:
3552:
3488:interferometers
3487:
3476:
3471:Mario Schenberg
3435:
3419:
3353:
3349:Mario Schenberg
3308:
3292:
3274:
3269:
3232:
3230:
3226:
3218:
3216:
3207:
3199:
3197:
3193:
3185:
3183:
3179:
3171:
3169:
3165:
3162:
3157:
3147:
3145:
3130:
3129:
3125:
3116:
3115:
3111:
3098:
3097:
3093:
3077:
3076:
3072:
3062:
3060:
3052:
3048:
3047:
3040:
3030:
3028:
3020:
3016:
3015:
3008:
2995:
2993:
2991:sciencenews.org
2984:
2983:
2979:
2919:
2918:
2914:
2866:
2865:
2858:
2805:Phys. Rev. Lett
2802:
2801:
2797:
2781:
2780:
2776:
2750:
2749:
2745:
2736:
2734:
2721:
2720:
2716:
2707:
2705:
2696:
2695:
2691:
2642:
2641:
2637:
2583:
2582:
2578:
2529:
2528:
2524:
2476:
2475:
2471:
2423:
2422:
2418:
2370:
2369:
2365:
2316:
2315:
2311:
2302:
2300:
2292:
2291:
2287:
2231:
2230:
2226:
2217:
2215:
2190:
2189:
2185:
2121:
2120:
2116:
2106:
2104:
2094:
2093:
2089:
2042:Phys. Rev. Lett
2035:
2034:
2030:
2021:
2019:
2006:
2005:
2001:
1992:
1990:
1981:
1980:
1976:
1966:
1964:
1959:
1958:
1954:
1944:
1942:
1887:
1886:
1882:
1834:
1833:
1829:
1781:
1780:
1776:
1764:
1757:
1756:
1752:
1742:
1740:
1731:
1730:
1726:
1716:
1714:
1705:
1704:
1700:
1690:
1688:
1679:
1678:
1674:
1664:
1662:
1653:
1652:
1645:
1612:
1610:
1606:
1573:
1571:
1567:
1531:
1530:
1523:
1490:
1488:
1484:
1451:
1449:
1445:
1412:
1410:
1406:
1397:
1396:
1392:
1382:
1380:
1371:
1370:
1366:
1356:
1354:
1345:
1344:
1340:
1330:
1328:
1323:
1322:
1318:
1313:. 20 June 2017.
1305:
1304:
1300:
1290:
1288:
1284:
1280:
1279:
1250:
1240:
1238:
1233:
1232:
1228:
1222:Wayback Machine
1213:
1209:
1160:
1159:
1155:
1145:
1143:
1134:
1133:
1129:
1119:
1117:
1116:on 13 June 2019
1104:
1103:
1099:
1089:
1087:
1078:
1077:
1073:
1063:
1061:
1056:
1055:
1051:
1041:
1039:
1030:
1029:
1025:
1015:
1013:
1004:
1003:
996:
986:
984:
973:
972:
965:
961:
930:
907:LISA Pathfinder
894:
852:Cassini–Huygens
845:
839:
827:
815:
806:
782:
775:
764:
749:
736:
724:
711:
690:
684:
644:
623:
595:
493:
480:LISA Pathfinder
476:
474:LISA Pathfinder
470:
468:LISA Pathfinder
446:GRACE Follow-On
413:
397:payload fairing
389:
353:
317:compact objects
272:long-term plans
213:
212:
205:
166:Semi-major axis
75:
45:
28:
23:
22:
15:
12:
11:
5:
8493:
8491:
8483:
8482:
8477:
8472:
8467:
8462:
8457:
8452:
8447:
8442:
8432:
8431:
8427:
8426:
8414:
8402:
8390:
8378:
8366:
8354:
8331:
8330:
8328:
8327:
8322:
8316:
8313:
8312:
8310:
8309:
8308:(28 September)
8303:
8302:(11 September)
8297:
8296:(10 September)
8291:
8284:
8282:
8276:
8275:
8272:
8271:
8269:
8268:
8263:
8257:
8252:
8247:
8242:
8236:
8234:
8228:
8227:
8225:
8224:
8218:
8212:
8206:
8200:
8194:
8188:
8182:
8176:
8170:
8164:
8161:
8155:
8149:
8143:
8133:
8127:
8121:
8115:
8109:
8100:
8094:
8088:
8082:
8076:
8070:
8063:
8061:
8055:
8054:
8052:
8051:
8046:
8037:
8031:
8026:
8020:
8018:
8012:
8011:
8009:
8008:
8003:
7998:
7993:
7988:
7982:
7977:
7972:
7967:
7958:
7948:
7946:
7940:
7939:
7937:
7936:
7930:
7924:
7919:
7909:
7904:
7899:
7894:
7889:
7884:
7879:
7873:
7867:
7861:
7856:
7851:
7846:
7841:
7836:
7826:
7816:
7811:
7805:
7803:
7797:
7796:
7794:
7793:
7787:
7781:
7767:
7762:
7757:
7752:
7747:
7744:Europa Clipper
7741:
7736:
7730:
7724:
7718:
7716:
7707:
7703:
7702:
7699:
7698:
7696:
7695:
7689:
7683:
7677:
7672:
7666:
7659:
7657:
7653:
7652:
7650:
7649:
7644:
7639:
7634:
7628:
7622:
7616:
7610:
7605:
7599:
7596:SpaceX Crew-10
7592:
7590:
7584:
7583:
7581:
7580:
7574:
7567:
7565:
7556:
7550:
7549:
7546:
7544:
7543:
7536:
7529:
7521:
7512:
7511:
7509:
7508:
7498:
7486:
7474:
7457:
7454:
7453:
7450:
7449:
7447:
7446:
7441:
7436:
7431:
7425:
7423:
7419:
7418:
7416:
7415:
7410:
7405:
7400:
7395:
7390:
7385:
7380:
7375:
7370:
7365:
7360:
7355:
7350:
7345:
7340:
7335:
7330:
7325:
7323:Darwin Mission
7320:
7315:
7310:
7305:
7300:
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7268:(2019–present)
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7115:Edoardo Amaldi
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7105:(2010–present)
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6482:Related topics
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4558:HXMT (Insight)
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4550:Einstein Probe
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3966:Chirp signal (
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3632:LIGO-Australia
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3625:Past proposals
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3543:Advanced Virgo
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3469:(downsized to
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3440:Past proposals
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3160:External links
3158:
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3123:
3109:
3106:on 2013-12-03.
3091:
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3038:
3006:
2977:
2912:
2869:Gen. Rel. Grav
2856:
2811:(23): 231102.
2795:
2774:
2763:(9): 858–866.
2743:
2714:
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2326:(12): 124016.
2309:
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2048:(23): 231101.
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1999:
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1327:. 20 June 2017
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1170:(12): 124016.
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813:Memory effects
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804:Exotic sources
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792:, first-order
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686:Main article:
683:
680:
643:
640:
622:
619:
615:ZTF J1539+5027
594:
591:
583:cosmic strings
575:compact object
530:, such as the
528:binary pulsars
492:
489:
484:Lagrange point
472:Main article:
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412:
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388:
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341:cosmic strings
295:speed of light
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8445:Cosmic Vision
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8306:SpaceX Crew-9
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8240:Europa Lander
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8118:Solar-C EUVST
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7216:demonstrators
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6843:
6842:
6838:
6835:
6834:
6830:
6827:
6826:
6822:
6819:
6818:
6814:
6811:
6810:
6806:
6803:
6800:
6797:
6794:
6791:
6788:
6785:
6782:
6779:
6776:
6773:
6770:
6767:
6764:
6761:
6758:
6755:
6752:
6749:
6746:
6743:
6740:
6737:
6734:
6731:
6728:
6725:
6722:
6719:
6716:
6713:
6710:
6709:
6707:
6702:Astronomy and
6699:
6692:
6691:
6687:
6684:
6683:
6679:
6676:
6674:
6670:
6667:
6666:
6662:
6659:
6656:
6653:
6650:
6647:
6646:
6641:
6638:
6637:Venus Express
6635:
6632:
6628:
6625:
6622:
6619:
6616:
6613:
6610:
6607:
6604:
6601:
6600:
6598:
6594:
6587:
6586:
6582:
6579:
6578:Solar Orbiter
6576:
6573:
6570:
6567:
6564:
6561:
6558:
6555:
6552:
6551:
6549:
6547:Solar physics
6545:
6542:
6538:
6534:
6529:
6525:
6515:
6512:
6510:
6507:
6505:
6502:
6500:
6497:
6495:
6492:
6490:
6487:
6486:
6484:
6480:
6474:
6471:
6469:
6466:
6465:
6463:
6459:
6453:
6450:
6446:
6445:Cosmic Vision
6443:
6441:
6438:
6437:
6436:
6433:
6431:
6428:
6426:
6423:
6421:
6418:
6416:
6413:
6411:
6408:
6406:
6403:
6401:
6398:
6396:
6393:
6391:
6388:
6384:
6381:
6380:
6379:
6376:
6374:
6371:
6369:
6366:
6362:
6359:
6358:
6357:
6354:
6353:
6351:
6347:
6341:
6338:
6336:
6333:
6332:
6330:
6326:
6320:
6317:
6315:
6312:
6310:
6307:
6305:
6302:
6300:
6297:
6295:
6292:
6290:
6287:
6285:
6282:
6281:
6279:
6275:
6269:
6266:
6264:
6261:
6259:
6256:
6255:
6253:
6251:
6247:
6241:
6238:
6236:
6233:
6232:
6230:
6228:
6224:
6220:
6216:
6209:
6204:
6202:
6197:
6195:
6190:
6189:
6186:
6174:
6166:
6165:
6162:
6156:
6153:
6151:
6148:
6146:
6143:
6141:
6138:
6136:
6133:
6131:
6128:
6127:
6125:
6121:
6115:
6112:
6110:
6107:
6105:
6102:
6100:
6097:
6095:
6092:
6090:
6087:
6085:
6082:
6080:
6077:
6075:
6072:
6070:
6067:
6065:
6062:
6060:
6057:
6055:
6052:
6050:
6047:
6045:
6042:
6040:
6037:
6035:
6032:
6030:
6027:
6025:
6024:
6020:
6018:
6015:
6013:
6010:
6008:
6007:
6003:
6001:
5998:
5996:
5993:
5991:
5988:
5986:
5983:
5982:
5980:
5976:
5967:
5964:
5959:
5956:
5951:
5948:
5943:
5940:
5935:
5932:
5927:
5924:
5919:
5916:
5911:
5908:
5903:
5900:
5895:
5892:
5887:
5884:
5883:
5881:
5877:
5868:
5865:
5860:
5857:
5856:
5854:
5846:
5837:
5834:
5829:
5826:
5821:
5818:
5813:
5810:
5805:
5802:
5797:
5796:Taiyo (SRATS)
5794:
5789:
5786:
5781:
5778:
5773:
5770:
5765:
5762:
5757:
5754:
5749:
5746:
5741:
5738:
5733:
5730:
5725:
5722:
5717:
5714:
5709:
5706:
5701:
5698:
5693:
5690:
5685:
5682:
5677:
5674:
5669:
5666:
5662:
5659:
5657:
5654:
5652:
5649:
5647:
5644:
5642:
5639:
5637:
5634:
5632:
5629:
5627:
5624:
5623:
5622:
5619:
5614:
5611:
5606:
5603:
5598:
5595:
5590:
5587:
5582:
5579:
5574:
5571:
5566:
5563:
5558:
5555:
5550:
5547:
5542:
5539:
5534:
5531:
5526:
5523:
5518:
5515:
5510:
5507:
5502:
5499:
5494:
5491:
5486:
5483:
5478:
5475:
5470:
5467:
5462:
5459:
5454:
5451:
5446:
5443:
5438:
5435:
5430:
5427:
5422:
5419:
5414:
5411:
5406:
5403:
5398:
5395:
5390:
5387:
5382:
5379:
5374:
5371:
5366:
5363:
5358:
5355:
5350:
5347:
5342:
5339:
5334:
5331:
5326:
5323:
5318:
5315:
5310:
5307:
5302:
5299:
5294:
5291:
5286:
5283:
5278:
5275:
5270:
5267:
5262:
5259:
5254:
5251:
5246:
5243:
5237:
5233:
5230:
5226:
5223:
5221:
5218:
5217:
5213:
5210:
5205:
5202:
5197:
5194:
5189:
5186:
5181:
5178:
5173:
5170:
5165:
5162:
5157:
5154:
5149:
5146:
5141:
5138:
5133:
5130:
5125:
5122:
5117:
5114:
5109:
5106:
5105:
5103:
5099:
5093:
5090:
5088:
5085:
5083:
5080:
5078:
5075:
5073:
5070:
5068:
5065:
5063:
5060:
5058:
5055:
5053:
5050:
5048:
5045:
5043:
5040:
5038:
5035:
5033:
5030:
5028:
5025:
5023:
5020:
5018:
5015:
5013:
5010:
5008:
5005:
5003:
5000:
4998:
4995:
4993:
4990:
4988:
4985:
4983:
4980:
4978:
4975:
4973:
4970:
4968:
4965:
4964:
4962:
4960:
4956:
4947:
4944:
4939:
4936:
4931:
4928:
4923:
4920:
4915:
4912:
4907:
4904:
4899:
4896:
4891:
4888:
4883:
4882:Solar-C EUVST
4880:
4875:
4872:
4867:
4864:
4859:
4856:
4851:
4848:
4843:
4840:
4835:
4832:
4827:
4824:
4819:
4816:
4811:
4808:
4803:
4800:
4799:
4797:
4793:
4780:
4777:
4772:
4771:Solar Orbiter
4769:
4764:
4761:
4756:
4753:
4748:
4745:
4740:
4737:
4732:
4729:
4724:
4721:
4716:
4713:
4708:
4705:
4704:
4702:
4696:
4687:
4684:
4679:
4676:
4671:
4668:
4663:
4660:
4655:
4652:
4647:
4644:
4639:
4636:
4631:
4628:
4623:
4620:
4615:
4612:
4607:
4604:
4599:
4596:
4591:
4588:
4583:
4580:
4575:
4572:
4567:
4564:
4559:
4556:
4551:
4548:
4543:
4540:
4535:
4532:
4527:
4524:
4523:
4521:
4519:
4515:
4511:
4502:
4499:
4494:
4491:
4486:
4485:Solar Orbiter
4483:
4478:
4475:
4470:
4467:
4462:
4459:
4454:
4451:
4446:
4443:
4438:
4435:
4430:
4427:
4422:
4419:
4414:
4411:
4410:
4408:
4406:
4402:
4393:
4390:
4385:
4382:
4377:
4374:
4369:
4366:
4361:
4358:
4353:
4350:
4345:
4342:
4337:
4334:
4329:
4326:
4321:
4318:
4313:
4310:
4305:
4302:
4297:
4294:
4289:
4286:
4281:
4278:
4273:
4270:
4264:
4261:
4256:
4253:
4248:
4245:
4244:
4242:
4240:
4236:
4227:
4224:
4219:
4216:
4211:
4208:
4203:
4200:
4199:
4197:
4195:
4191:
4182:
4179:
4174:
4171:
4166:
4163:
4158:
4155:
4150:
4149:Solar Orbiter
4147:
4142:
4139:
4138:
4136:
4134:
4130:
4127:
4123:
4119:
4112:
4107:
4105:
4100:
4098:
4093:
4092:
4089:
4074:
4073:other unknown
4070:
4069:cosmic string
4066:
4065:
4063:
4058:
4054:
4051:
4050:
4048:
4043:
4042:
4040:
4036:
4033:
4031:
4030:Neutron stars
4028:
4026:
4023:
4021:
4018:
4017:
4015:
4011:
4008:
4006:
4002:
3999:
3998:
3997:
3994:
3993:
3991:
3987:
3981:
3978:
3976:
3972:
3969:
3965:
3962:
3960:
3956:
3954:
3951:
3949:
3946:
3944:
3941:
3940:
3938:
3934:
3928:
3925:
3923:
3920:
3918:
3915:
3913:
3910:
3909:
3907:
3903:
3891:
3890:Binary pulsar
3888:
3886:
3883:
3881:
3877:
3874:
3873:
3871:
3867:
3866:
3861:
3858:
3856:
3853:
3852:
3850:
3849:
3847:
3843:
3836:
3833:
3830:
3827:
3824:
3821:
3819:
3816:
3813:
3809:
3806:
3804:
3801:
3799:
3796:
3794:
3791:
3789:
3786:
3784:
3781:
3779:
3776:
3775:
3773:
3769:
3766:
3762:
3756:: Gravity Spy
3755:
3752:
3750:
3747:
3745:
3744:Einstein@Home
3742:
3741:
3739:
3737:Data analysis
3735:
3729:
3726:
3724:
3721:
3719:
3716:
3714:
3711:
3710:
3708:
3706:
3702:
3688:
3685:
3683:
3680:
3678:
3675:
3674:
3672:
3668:
3662:
3659:
3658:
3656:
3652:
3649:
3643:
3633:
3630:
3629:
3627:
3623:
3617:
3614:
3612:
3609:
3608:
3606:
3602:
3596:
3593:
3592:
3590:
3586:
3580:
3577:
3575:
3572:
3570:
3567:
3565:
3562:
3561:
3559:
3555:
3548:
3544:
3541:
3539:
3536:
3533:
3529:
3528:Advanced LIGO
3526:
3524:
3521:
3519:
3516:
3514:
3511:
3508:
3504:
3501:
3500:
3498:
3494:
3491:
3489:
3483:
3472:
3468:
3465:
3463:
3460:
3458:
3455:
3452:
3448:
3445:
3444:
3442:
3438:
3432:
3429:
3428:
3426:
3422:
3416:
3413:
3411:
3408:
3406:
3403:
3401:
3398:
3396:
3393:
3390:
3386:
3383:
3380:
3376:
3373:
3370:
3366:
3363:
3362:
3360:
3356:
3350:
3347:
3345:
3342:
3339:
3335:
3332:
3329:
3325:
3322:
3321:
3319:
3315:
3312:
3310:
3307:Resonant mass
3304:
3301:
3299:
3295:
3289:
3286:
3284:
3281:
3280:
3277:
3273:
3266:
3261:
3259:
3254:
3252:
3247:
3246:
3243:
3229:
3225:
3215:on 2010-07-21
3214:
3210:
3206:
3196:
3192:
3182:
3178:
3168:
3164:
3163:
3159:
3143:
3139:
3138:
3133:
3127:
3124:
3119:
3113:
3110:
3105:
3101:
3095:
3092:
3086:
3081:
3074:
3071:
3058:
3057:Gijs Nelemans
3051:
3045:
3043:
3039:
3026:
3019:
3013:
3011:
3007:
3003:
2992:
2988:
2981:
2978:
2973:
2969:
2965:
2961:
2957:
2953:
2949:
2945:
2940:
2935:
2932:(8): 084036.
2931:
2927:
2923:
2916:
2913:
2908:
2904:
2900:
2896:
2892:
2888:
2883:
2878:
2874:
2870:
2863:
2861:
2857:
2852:
2848:
2844:
2840:
2836:
2832:
2828:
2824:
2819:
2814:
2810:
2806:
2799:
2796:
2790:
2785:
2778:
2775:
2770:
2766:
2762:
2758:
2754:
2747:
2744:
2733:on 2019-08-11
2732:
2728:
2724:
2718:
2715:
2704:
2700:
2693:
2690:
2685:
2681:
2677:
2673:
2669:
2665:
2660:
2655:
2651:
2647:
2639:
2636:
2631:
2627:
2622:
2617:
2613:
2609:
2604:
2599:
2595:
2591:
2587:
2580:
2577:
2572:
2568:
2564:
2560:
2556:
2552:
2547:
2542:
2538:
2534:
2526:
2523:
2518:
2514:
2510:
2506:
2502:
2498:
2493:
2492:gr-qc/9701039
2488:
2484:
2480:
2473:
2470:
2465:
2461:
2457:
2453:
2449:
2445:
2440:
2435:
2431:
2427:
2420:
2417:
2412:
2408:
2404:
2400:
2396:
2392:
2387:
2382:
2379:(9): 094030.
2378:
2374:
2367:
2364:
2359:
2355:
2351:
2347:
2343:
2339:
2334:
2329:
2325:
2321:
2313:
2310:
2299:
2295:
2289:
2286:
2281:
2277:
2273:
2269:
2265:
2261:
2257:
2253:
2248:
2243:
2240:(6): 061102.
2239:
2235:
2228:
2225:
2214:
2210:
2206:
2202:
2198:
2194:
2187:
2184:
2179:
2175:
2170:
2165:
2160:
2155:
2151:
2147:
2142:
2137:
2133:
2129:
2125:
2118:
2115:
2102:
2098:
2091:
2088:
2083:
2079:
2074:
2069:
2064:
2059:
2055:
2051:
2047:
2043:
2039:
2032:
2029:
2017:
2013:
2009:
2003:
2000:
1988:
1984:
1978:
1975:
1962:
1956:
1953:
1941:
1937:
1933:
1929:
1925:
1921:
1917:
1913:
1908:
1903:
1900:(3): 031101.
1899:
1895:
1891:
1884:
1881:
1876:
1872:
1868:
1864:
1860:
1856:
1851:
1846:
1843:(1): 012024.
1842:
1838:
1831:
1828:
1823:
1819:
1815:
1811:
1807:
1803:
1798:
1793:
1790:(6): 065011.
1789:
1785:
1778:
1775:
1770:
1763:
1762:
1754:
1751:
1738:
1734:
1728:
1725:
1712:
1708:
1702:
1699:
1686:
1682:
1676:
1673:
1660:
1656:
1650:
1648:
1644:
1639:
1635:
1630:
1625:
1621:
1617:
1608:
1605:
1600:
1596:
1591:
1586:
1582:
1578:
1569:
1566:
1561:
1557:
1552:
1547:
1543:
1539:
1535:
1528:
1526:
1522:
1517:
1513:
1508:
1503:
1499:
1495:
1486:
1483:
1478:
1474:
1469:
1464:
1460:
1456:
1447:
1444:
1439:
1435:
1430:
1425:
1421:
1417:
1408:
1405:
1400:
1394:
1391:
1378:
1374:
1368:
1365:
1352:
1348:
1342:
1339:
1326:
1320:
1317:
1312:
1308:
1302:
1299:
1283:
1277:
1275:
1273:
1271:
1269:
1267:
1265:
1263:
1261:
1259:
1257:
1255:
1253:
1249:
1236:
1230:
1227:
1223:
1219:
1216:
1211:
1208:
1203:
1199:
1195:
1191:
1187:
1183:
1178:
1173:
1169:
1165:
1157:
1154:
1141:
1137:
1131:
1128:
1115:
1111:
1107:
1101:
1098:
1086:on 2011-03-03
1085:
1081:
1075:
1072:
1059:
1053:
1050:
1037:
1033:
1027:
1024:
1011:
1007:
1001:
999:
995:
982:
981:
976:
970:
968:
964:
958:
953:
950:
948:program – ESA
947:
946:Cosmic Vision
944:
941:
938:
935:
932:
931:
927:
925:
923:
918:
915:
910:
908:
904:
898:
891:
889:
887:
883:
878:
874:
870:
866:
862:
858:
854:
853:
843:
837:
831:
824:
822:
820:
812:
810:
803:
801:
799:
795:
791:
787:
779:
777:
772:
768:
761:
758:
754:
746:
744:
742:
733:
731:
729:
721:
719:
717:
708:
706:
704:
700:
696:
693:events up to
689:
681:
679:
677:
673:
669:
665:
661:
657:
653:
649:
641:
639:
637:
633:
628:
620:
618:
616:
612:
608:
604:
603:neutron stars
600:
592:
590:
588:
584:
580:
576:
572:
568:
564:
560:
554:
552:
548:
543:
541:
537:
536:Advanced LIGO
533:
529:
525:
522:'s theory of
521:
517:
510:
506:
502:
501:Advanced LIGO
497:
491:Science goals
490:
488:
485:
481:
475:
467:
465:
462:
457:
455:
449:
447:
443:
439:
434:
430:
426:
417:
410:
408:
404:
402:
398:
394:
386:
384:
382:
378:
374:
369:
367:
357:
350:
348:
346:
342:
338:
334:
330:
326:
322:
318:
314:
310:
307:
302:
300:
296:
292:
288:
283:
279:
275:
273:
269:
265:
261:
257:
253:
248:
246:
242:
238:
234:
230:
226:
222:
211:
208:←
204:
203:
202:Cosmic Vision
197:
193:
189:
187:
183:
179:
177:
173:
169:
167:
163:
160:
157:
153:
148:
144:
140:
137:
134:
130:
127:
124:
121:
117:
114:
111:
107:
103:
99:
94:
90:
86:
82:
74:
70:
67:
64:
60:
56:
52:
48:
41:
36:
30:
19:
8400:Solar System
8294:Polaris Dawn
8255:Nano-JASMINE
8220:
8103:
8091:MBR Explorer
8034:NEO Surveyor
7665:(March 2026)
7493:
7482:
7469:
7459:
7368:Lunar Lander
7286:and proposed
7271:
7058:
7050:
7042:
7034:
7026:
7018:
7010:
7004:
6996:
6988:
6840:
6839:
6831:
6823:
6815:
6807:
6688:
6680:
6672:
6663:
6644:
6621:Mars Express
6583:
6461:Predecessors
6440:Horizon 2000
6021:
6004:
5848:Hibernating
5600:(2016–2019?)
5143:(1962, 1964)
5042:Nano-JASMINE
4945:
4866:NEO Surveyor
4782:(since 2006)
4774:(since 2020)
4766:(since 1995)
4758:(since 2019)
4750:(since 2017)
4742:(since 2008)
4734:(since 2015)
4726:(since 2015)
4718:(since 2011)
4710:(since 1997)
4689:(since 1999)
4681:(since 2024)
4673:(since 2023)
4665:(since 2022)
4657:(since 2012)
4649:(since 2017)
4641:(since 2018)
4633:(since 2009)
4625:(since 2017)
4617:(since 2004)
4609:(since 2024)
4601:(since 2019)
4593:(since 2021)
4585:(since 2020)
4577:(since 2008)
4569:(since 2002)
4561:(since 2017)
4553:(since 2024)
4545:(since 2015)
4537:(since 1999)
4529:(since 2015)
4504:(since 2004)
4496:(since 2006)
4488:(since 2020)
4480:(since 2008)
4472:(since 1995)
4464:(since 2010)
4456:(since 2013)
4448:(since 2006)
4440:(since 2021)
4432:(since 2015)
4424:(since 2022)
4416:(since 2023)
4395:(since 2018)
4387:(since 2004)
4379:(since 2008)
4371:(since 1995)
4363:(since 2010)
4355:(since 2001)
4347:(since 2013)
4339:(since 2006)
4331:(since 1990)
4323:(since 2005)
4315:(since 2013)
4307:(since 2021)
4299:(since 2023)
4291:(since 2015)
4283:(since 2019)
4275:(since 2021)
4267:(since 2013)
4258:(since 2015)
4250:(since 2018)
4229:(since 2009)
4221:(since 2008)
4213:(since 2001)
4205:(since 2022)
4184:(since 2024)
4176:(since 1994)
4168:(since 2018)
4160:(since 2006)
4152:(since 2020)
4144:(since 2018)
4072:
4056:
3957:Travel with
3943:Polarization
3862:
3764:Observations
3660:
3486:Ground-based
3231:. Retrieved
3217:. Retrieved
3213:the original
3198:. Retrieved
3184:. Retrieved
3170:. Retrieved
3146:. Retrieved
3142:the original
3135:
3126:
3112:
3104:the original
3094:
3073:
3061:. Retrieved
3056:
3029:. Retrieved
3025:Monica Colpi
3024:
3001:
2996:17 September
2994:. Retrieved
2990:
2980:
2929:
2925:
2915:
2872:
2868:
2808:
2804:
2798:
2777:
2760:
2756:
2746:
2735:. Retrieved
2731:the original
2726:
2717:
2706:. Retrieved
2702:
2692:
2649:
2645:
2638:
2593:
2589:
2579:
2536:
2532:
2525:
2482:
2478:
2472:
2429:
2425:
2419:
2376:
2372:
2366:
2323:
2319:
2312:
2301:. Retrieved
2297:
2288:
2237:
2233:
2227:
2216:. Retrieved
2196:
2186:
2131:
2127:
2117:
2105:. Retrieved
2101:the original
2090:
2045:
2041:
2031:
2020:. Retrieved
2016:the original
2011:
2002:
1991:. Retrieved
1986:
1977:
1965:. Retrieved
1955:
1943:. Retrieved
1897:
1893:
1883:
1840:
1836:
1830:
1787:
1783:
1777:
1760:
1753:
1741:. Retrieved
1737:the original
1727:
1715:. Retrieved
1711:the original
1701:
1689:. Retrieved
1685:the original
1675:
1663:. Retrieved
1659:the original
1619:
1615:
1607:
1580:
1576:
1568:
1541:
1537:
1497:
1493:
1485:
1458:
1454:
1446:
1419:
1415:
1407:
1393:
1381:. Retrieved
1377:the original
1367:
1355:. Retrieved
1350:
1341:
1329:. Retrieved
1319:
1310:
1301:
1289:. Retrieved
1239:. Retrieved
1229:
1210:
1167:
1163:
1156:
1144:. Retrieved
1139:
1130:
1118:. Retrieved
1114:the original
1109:
1100:
1088:. Retrieved
1084:the original
1074:
1062:. Retrieved
1052:
1040:. Retrieved
1036:the original
1026:
1014:. Retrieved
1010:the original
985:. Retrieved
978:
919:
911:
899:
895:
850:
848:
841:
835:
816:
807:
783:
770:
759:
752:
750:
737:
725:
715:
712:
699:eccentricity
694:
691:
671:
663:
659:
652:solar masses
645:
627:brown dwarfs
624:
599:white dwarfs
596:
555:
544:
514:
507:such as the
503:(aLIGO) and
477:
458:
450:
422:
405:
393:lightseconds
390:
370:
362:
303:
284:
280:
276:
267:
263:
249:
224:
220:
218:
200:
159:Heliocentric
79:.lisamission
54:Mission type
29:
8412:Outer space
8388:Spaceflight
8300:Soyuz MS-26
8262:(mid 2020s)
8205:(2031–2032)
8160:(2029–2031)
8049:Superbird-9
8036:(September)
7987:(2026–2027)
7902:Space Rider
7844:Gaganyaan-3
7839:Gaganyaan-2
7786:(September)
7765:Hakuto-R M2
7750:Gaganyaan-1
7729:(September)
7727:Bion-M No.2
7675:Gaganyaan-5
7669:Artemis III
7663:Soyuz MS-29
7647:Gaganyaan-4
7642:Shenzhou 21
7633:(September)
7627:(September)
7625:Soyuz MS-28
7608:Shenzhou 20
7602:Soyuz MS-27
7579:(late 2024)
7571:Shenzhou 19
7506:WikiProject
7378:MarcoPolo-R
7328:Don Quijote
7298:Ariane 5 ME
7262:(2015–2017)
7192:Galileo FOC
7186:Galileo IOV
7158:(1989–1993)
7097:Jules Verne
7078:spaceflight
6909:(2009–2013)
6897:(2003–2007)
6895:Double Star
6891:(2002–2012)
6879:(1995–2011)
6873:(1991–2000)
6867:(1977–1997)
6780:(2009–2013)
6774:(2009–2013)
6750:(1995–1998)
6732:(1989–1993)
6726:(1983–1986)
6720:(1978–1996)
6714:(1975–1982)
6652:BepiColombo
6639:(2005–2014)
6633:(2004–2016)
6617:(2003–2006)
6611:(1997–2005)
6605:(1985–1992)
6574:(2000–2024)
6562:(1990–2009)
6556:(1977–1987)
6489:Arianespace
5961:(2014–2015)
5913:(2012–2013)
5879:Lost/Failed
5870:(1998–2010)
5862:(1998–2005)
5839:(1991–2001)
5831:(2001–2010)
5815:(1970–1973)
5807:(1983–1985)
5799:(1975–1980)
5791:(2005–2015)
5783:(2003–2020)
5775:(2011–2019)
5767:(1979–1985)
5759:(1975–1979)
5751:(1972–1973)
5743:(1992–2004)
5735:(1995–2012)
5727:(1990–1999)
5719:(2002–2018)
5711:(1983–1984)
5703:(2009–2013)
5687:(2006–2016)
5616:(1972–1981)
5608:(1968–1973)
5592:(1996–1997)
5584:(2003–2019)
5576:(2015–2017)
5568:(2015–2017)
5560:(1997–2002)
5552:(1990–2001)
5544:(2009–2018)
5536:(1996–2004)
5528:(1978–1996)
5520:(1996–1998)
5512:(1995–1996)
5488:(1989–1993)
5480:(2000–2008)
5472:(1979–1981)
5464:(1978–1982)
5456:(2013–2023)
5448:(1981–1991)
5440:(2009–2013)
5432:(1977–1979)
5424:(1997–2005)
5416:(1979–1985)
5408:(1989–1998)
5400:(1987–1991)
5392:(1990–1992)
5384:(2003–2013)
5376:(1987–2001)
5368:(1999–2007)
5360:(1992–2001)
5352:(1983–1986)
5341:Explorer 11
5312:(2017–2019)
5304:(1989–1993)
5296:(1975–1982)
5288:(2006–2013)
5280:(1991–2000)
5272:(2003–2008)
5264:(1996–2003)
5256:(1974–1976)
5248:(1983–1991)
5207:(1993–2000)
5199:(1973–1974)
5191:(2017–2019)
5183:(1979–1982)
5175:(1974–1980)
5167:(1971–1972)
5159:(1967–1969)
5135:(1962–1972)
5127:(1993–2005)
5119:(2006–2011)
5111:(2007–2024)
4405:Ultraviolet
4064:Hypothesis
4041:Continuous
3645:Space-based
3148:10 November
2197:Nature News
2073:2117/102419
1967:12 November
1743:12 November
1717:12 November
1691:12 November
1665:12 November
1383:15 November
1241:29 November
1064:12 November
1042:12 November
1016:12 November
914:Large class
882:ultraviolet
796:related to
703:inclination
607:black holes
547:black holes
461:Fabry–Pérot
438:phase shift
319:, known as
309:black holes
136:Arianespace
119:Launch site
101:Launch date
8434:Categories
8288:Türksat 6A
7922:SSC Demo-1
7918:(February)
7866:(February)
7792:(November)
7733:Blue Ghost
7680:Artemis IV
7631:Artemis II
7598:(February)
7573:(November)
7393:Phootprint
7373:Marco Polo
7214:Technology
7044:MetOp-SG-B
7036:MetOp-SG-A
7012:Sentinel-4
6983:ADM-Aeolus
6963:Sentinel-3
6945:Sentinel-2
6931:Sentinel-1
6859:Copernicus
6754:XMM-Newton
6572:Cluster II
6378:Copernicus
6349:Programmes
6277:Facilities
6227:Spaceports
5820:Vanguard 3
5132:Alouette 1
4977:AstroSat-2
4686:XMM-Newton
4202:James Webb
4067:Colliding
3996:Stochastic
3968:chirp mass
3863:Proposed:
3754:Zooniverse
3233:2010-08-13
3219:2010-08-13
3200:2013-05-22
3186:2010-08-13
3172:2013-11-13
3063:14 January
3031:14 January
2882:2001.09793
2818:1602.06951
2789:1812.04330
2737:2019-08-11
2708:2019-08-01
2652:(6): 027.
2303:2016-02-11
2247:1602.03837
2218:2016-02-11
2022:2016-04-06
1993:2016-02-12
1945:3 February
1907:1907.00104
1850:1703.09858
1551:1910.05414
1357:29 January
1291:14 January
1146:21 January
1120:21 January
987:25 January
959:References
863:, such as
648:chirp mass
551:picometres
387:Arm length
373:solar wind
132:Contractor
8364:Astronomy
8179:Spektr-UV
8173:SAOCOM-2B
8152:Tianwen-4
8124:Tianwen-3
8112:SAOCOM-2A
8073:Dragonfly
8067:Chang'e 8
7970:ispace M3
7961:Chang'e 7
7927:Tianwen-2
7849:Garatéa-L
7825:(January)
7780:(October)
7746:(October)
7686:Artemis V
7434:CryoSat-1
7408:STE-QUEST
7343:Eddington
7333:e.Deorbit
7284:Cancelled
7156:Olympus-1
6998:EarthCARE
6919:CryoSat-2
6768:(2006–13)
6744:(1992–93)
6730:Hipparcos
6704:cosmology
6023:Eddington
5978:Cancelled
5485:Hipparcos
4898:Spektr-UV
4755:Mini-EUSO
4747:ISS-CREAM
4598:Spektr-RG
4518:Gamma-ray
4413:Aditya-L1
4304:Hayabusa2
4181:Queqiao 2
4125:Operating
4053:Supernova
3948:Spin-flip
3574:TENKO-100
3451:MiniGRAIL
3415:Weber bar
3344:MiniGRAIL
3298:Detectors
3085:1305.5720
2964:0264-9381
2939:1003.3486
2907:210921122
2875:(8): 81.
2851:118612123
2684:119184947
2659:1201.0983
2603:1307.7276
2386:0901.1778
2333:1202.0839
2280:124959784
2213:182916902
1940:195766777
1875:119335855
1822:118356648
1797:1204.2125
1629:1201.3621
1590:1201.3621
1507:1201.3621
1468:1201.3621
1429:1201.3621
1177:1202.0839
855:), using
790:inflation
668:accretion
611:Milky Way
609:) in the
565:in other
559:Milky Way
436:relative
299:radiation
291:spacetime
233:spacetime
8290:(8 July)
8281:launched
8279:Recently
8209:LiteBIRD
8191:EnVision
8185:Spektr-M
8158:Venera-D
8001:ULTRASAT
7965:Rashid 2
7878:Series B
7876:MetOp-SG
7872:Series A
7870:MetOp-SG
7814:ESCAPADE
7778:Juventas
7755:GOSAT-GW
7706:Uncrewed
7621:(August)
7615:(Spring)
7495:Wikinews
7471:Category
7091:Columbus
7015:) (2024)
6825:ARRAKIHS
6778:Herschel
6760:INTEGRAL
6690:EnVision
6643:ExoMars
6499:EUMETSAT
6390:Columbus
6383:Sentinel
6263:Ariane 6
6258:Ariane 5
6074:Sentinel
5772:Spektr-R
5708:RELIKT-1
5549:Kristall
5437:Herschel
5261:BeppoSAX
5022:JEM-EUSO
5017:iWF-MAXI
4959:Proposed
4922:LiteBIRD
4914:Spektr-M
4638:MinXSS-2
4566:INTEGRAL
4429:Astrosat
4255:Astrosat
4194:Infrared
4055:or from
3973:Carried
3963:h strain
3953:Redshift
3927:Graviton
3835:GW200105
3829:GW190814
3823:GW190521
3818:GW190412
3808:GW170817
3803:GW170814
3798:GW170608
3793:GW170104
3788:GW151226
3723:NANOGrav
3670:Proposed
3604:Proposed
3564:TAMA 300
3467:Graviton
3424:Proposed
3365:EXPLORER
3324:NAUTILUS
3309:antennas
2972:28414218
2843:27341222
2630:55334359
2571:37683679
2517:33309772
2411:11275836
2358:54822413
2272:26918975
2178:28163640
2134:(1): 5.
2107:14 April
2082:27341221
1932:31386438
1616:GW Notes
1577:GW Notes
1494:GW Notes
1455:GW Notes
1416:GW Notes
1311:BBC News
1218:Archived
1202:54822413
928:See also
922:Ariane 6
886:infrared
877:NANOGrav
842:Figure 2
836:Figure 1
656:redshift
567:galaxies
520:Einstein
337:Big Bang
325:binaries
313:galaxies
254:and the
113:Ariane 6
62:Operator
8424:Science
8376:Physics
8338:Portals
8260:TEREX-1
8203:DAVINCI
8197:VERITAS
8187:(2030+)
8167:Luna 28
8146:Harmony
8085:Luna 27
8079:JASMINE
8029:Luna 26
7991:Xuntian
7935:(April)
7933:TRACERS
7912:SPHEREx
7864:LOXSAT1
7835:(April)
7833:SWFO-L1
7809:DESTINY
7784:PROBA-3
7760:GSAT-20
7722:Biomass
7694:(~2030)
7604:(March)
7483:Commons
7460:italics
7429:Cluster
7413:THESEUS
7398:SOLARIS
7273:PROBA-3
7266:OPS-SAT
7248:PROBA-V
7242:PROBA-2
7230:PROBA-1
7180:HYLAS-1
7174:GIOVE-B
7168:GIOVE-A
7162:Artemis
6990:Biomass
6889:Envisat
6828:(2030s)
6627:Rosetta
6615:SMART-1
6609:Huygens
6560:Ulysses
6540:Science
6415:ExoMars
6405:GALILEO
6395:CryoSat
6356:Artemis
6335:ESTRACK
6240:Esrange
6123:Related
6034:FINESSE
6012:Destiny
5995:Astro-G
5958:Tsubame
5950:Astro-E
5926:ABRIXAS
5780:Spitzer
5764:Solwind
5716:R/HESSI
5676:Orion 2
5668:Orion 1
5373:Kvant-1
5269:CHIPSat
5232:Astro-2
5212:Astro-1
5188:ASTERIA
5180:Ariel 6
5172:Ariel 5
5164:Ariel 4
5156:Ariel 3
5148:Ariel 2
5140:Ariel 1
5101:Retired
5092:THESEUS
5077:Solar-D
5072:PhoENiX
4917:(2030+)
4874:JASMINE
4842:Xuntian
4810:SPHEREx
4795:Planned
4344:NEOSSat
4239:Optical
4165:Queqiao
4075:sources
4059:sources
4057:unknown
3876:B-modes
3845:Methods
3810:(first
3687:TianQin
3654:Planned
3588:Planned
3405:GEOGRAV
3375:ALLEGRO
2944:Bibcode
2887:Bibcode
2823:Bibcode
2664:Bibcode
2608:Bibcode
2551:Bibcode
2497:Bibcode
2464:9338900
2444:Bibcode
2391:Bibcode
2338:Bibcode
2298:nsf.gov
2252:Bibcode
2169:5253800
2146:Bibcode
2050:Bibcode
1912:Bibcode
1855:Bibcode
1802:Bibcode
1634:Bibcode
1595:Bibcode
1512:Bibcode
1473:Bibcode
1434:Bibcode
1331:20 June
1182:Bibcode
892:History
658:around
524:gravity
306:massive
190:planned
72:Website
8223:(2035)
8217:(2035)
8215:Athena
8211:(2032)
8199:(2031)
8193:(2031)
8181:(2030)
8175:(2030)
8169:(2030)
8154:(2029)
8148:(2029)
8142:(2029)
8132:(2028)
8126:(2028)
8120:(2028)
8114:(2028)
8108:(2028)
8099:(2028)
8093:(2028)
8087:(2028)
8081:(2028)
8075:(2028)
8069:(2028)
7952:ALTIUS
7907:SPARCS
7892:PETREL
7854:HTV-X1
7774:Milani
7688:(2030)
7682:(2028)
7671:(2026)
7637:Vast-1
7554:Crewed
7439:GEOS 1
7422:Failed
7388:ODINUS
7358:Hopper
7353:Hermes
7348:EXPERT
7276:(2024)
7256:(2015)
7238:(2007)
7226:(1998)
7152:(1978)
7150:GEOS 2
7135:(2021)
7129:(2014)
7123:(2013)
7117:(2012)
7111:(2011)
7103:Cupola
7099:(2008)
7063:(2027)
7055:(2025)
7047:(2025)
7039:(2025)
7031:(2025)
7023:(2025)
7020:ALTIUS
7001:(2024)
6993:(2024)
6844:(2035)
6836:(2035)
6833:Athena
6820:(2029)
6812:(2026)
6802:Euclid
6790:CHEOPS
6772:Planck
6742:Eureca
6724:EXOSAT
6693:(2031)
6685:(2029)
6677:(2028)
6668:(2024)
6660:(2023)
6631:Philae
6603:Giotto
6588:(2031)
6554:ISEE-2
6368:Aurora
6099:TAUVEX
6006:Darwin
5985:Aelita
5969:(2016)
5953:(2000)
5945:(1999)
5937:(1996)
5934:HETE-1
5929:(1999)
5921:(1965)
5905:(1976)
5897:(1970)
5889:(1966)
5823:(1959)
5740:SAMPEX
5700:Planck
5695:(2018)
5692:PicSat
5684:PAMELA
5679:(1973)
5671:(1971)
5573:MinXSS
5541:Kepler
5504:(1983)
5496:(2024)
5477:HETE-2
5469:HEAO-3
5429:HEAO-1
5405:Granat
5349:EXOSAT
5344:(1961)
5336:(2010)
5328:(2008)
5320:(1993)
5309:CXBN-2
5245:Astron
5240:(1995)
5215:(1990)
5151:(1964)
5124:ALEXIS
5032:LUVOIR
4982:EXCEDE
4949:(2035)
4941:(2035)
4938:Athena
4933:(2033)
4925:(2032)
4909:(2030)
4901:(2030)
4893:(2029)
4885:(2028)
4877:(2028)
4869:(2027)
4861:(2027)
4853:(2027)
4845:(2026)
4837:(2026)
4829:(2026)
4821:(2026)
4818:K-EUSO
4813:(2025)
4805:(2025)
4802:PETREL
4779:STEREO
4715:AMS-02
4678:XPoSat
4654:NuSTAR
4493:STEREO
4437:Hibari
4328:Hubble
4320:HiRISE
4296:Euclid
4288:DSCOVR
4280:CHEOPS
4157:STEREO
4049:Burst
3975:energy
3905:Theory
3771:Events
3682:DECIGO
3523:GEO600
3496:Active
3400:ALTAIR
3334:AURIGA
3317:Active
2970:
2962:
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2849:
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2682:
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1938:
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1200:
1142:. CERN
1060:. NASA
936:– NASA
873:GEO600
871:, and
676:quasar
605:, and
569:; and
210:ATHENA
180:1 year
176:Period
123:Kourou
109:Rocket
8352:Stars
8250:MOM 2
8245:Janus
8136:ARIEL
8106:rover
8059:2028+
8024:FORUM
8006:VOICE
7996:PLATO
7975:LUPEX
7929:(May)
7916:PUNCH
7897:SMILE
7887:NISAR
7739:DISHA
7656:2026+
7577:Fram2
7403:SPICA
7198:EGNOS
7060:FORUM
7052:SMILE
6925:Swarm
6901:MetOp
6877:ERS-2
6871:ERS-1
6817:ARIEL
6809:PLATO
6766:CoRoT
6712:Cos-B
6675:rover
6585:Vigil
6509:GEWEX
6452:Pride
6410:ELIPS
6400:EGNOS
6094:SPOrt
6089:SPICA
6069:OSO K
6064:OSO J
5918:OSO C
5902:CORSA
5894:OAO-B
5886:OAO-1
5867:TRACE
5812:Uhuru
5756:SAS-C
5748:SAS-B
5724:ROSAT
5661:OSO 8
5656:OSO 7
5651:OSO 6
5646:OSO 5
5641:OSO 4
5636:OSO 3
5631:OSO B
5626:OSO 1
5605:OAO-2
5557:LEGRI
5493:ILO-X
5389:Gamma
5381:GALEX
5333:EPOXI
5325:EPOCh
5293:Cos-B
5285:CoRoT
5220:BBXRT
5108:AGILE
5087:THEIA
5062:ORBIS
5012:ILO-1
4997:HabEx
4992:FOCAL
4967:Arcus
4930:Taiji
4890:ARIEL
4834:PLATO
4731:DAMPE
4723:CALET
4670:XRISM
4646:NICER
4614:Swift
4582:GECAM
4574:Fermi
4542:DAMPE
4526:CALET
4514:X-ray
4501:Swift
4477:SOLAR
4421:ASO-S
4384:Swift
4376:SOLAR
4272:CHASE
4263:BRITE
4218:SOLAR
3749:PyCBC
3538:KAGRA
3507:ACIGA
3462:SFERA
3447:GRAIL
3410:AGATA
3385:NIOBE
3080:arXiv
3053:(PDF)
3021:(PDF)
2968:S2CID
2934:arXiv
2903:S2CID
2877:arXiv
2847:S2CID
2813:arXiv
2784:arXiv
2680:S2CID
2654:arXiv
2626:S2CID
2598:arXiv
2567:S2CID
2541:arXiv
2513:S2CID
2487:arXiv
2460:S2CID
2434:arXiv
2407:S2CID
2381:arXiv
2354:S2CID
2328:arXiv
2276:S2CID
2242:arXiv
2209:S2CID
2136:arXiv
1936:S2CID
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186:Epoch
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8221:LISA
8044:HALO
8016:2027
7956:FLEX
7944:2026
7882:MULA
7859:IM-3
7829:IMAP
7819:IM-2
7801:2025
7770:Hera
7714:2024
7588:2025
7563:2024
7363:LOFT
7338:EChO
7318:CSTS
7293:AIDA
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7028:FLEX
6913:SMOS
6907:GOCE
6841:LISA
6784:Gaia
6665:Hera
6566:SOHO
6420:FLPP
6268:Vega
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6084:SNAP
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6029:FAME
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5990:AOSO
5942:WIRE
5910:CXBN
5859:SWAS
5828:WMAP
5732:RXTE
5581:MOST
5533:IXAE
5509:IRTS
5501:IRAS
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5357:EUVE
5301:COBE
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3389:IGEC
3379:IGEC
3369:IGEC
3358:Past
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3150:2021
3065:2018
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1769:SLAC
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1719:2013
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1385:2013
1359:2024
1333:2017
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1148:2020
1122:2020
1092:2011
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1044:2013
1018:2013
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343:and
260:CERN
252:NASA
225:LISA
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170:1 AU
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7980:MMX
7254:IXV
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7076:ISS
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6373:ATV
6361:ESM
6104:TPF
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5525:IUE
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5253:ANS
5236:HUT
5225:HUT
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4707:ACE
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4247:Aoi
3880:CMB
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