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508:
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992:, including sunspots. Their statistical analysis also found that many stellar flares are seen regardless of the position of the exoplanet, therefore debunking the earlier claims. The magnetic fields of the host star and exoplanet do not interact, and this system is no longer believed to have a "star-planet interaction." Some researchers had also suggested that HD 189733 accretes, or pulls, gas from its orbiting exoplanet at a rate similar to those found around young
904:
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38:
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803:± 33 K to 1,212 ± 11 K was discovered, indicating that the absorbed energy from the parent star is distributed fairly evenly through the planet's atmosphere. The region of peak temperature was offset 30 degrees east of the substellar point, as predicted by theoretical models of hot Jupiters taking into account a parameterized day to night redistribution mechanism.
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988:, and the Automated Photoelectric Telescope, in addition to historical observations of the star at radio, optical, ultraviolet, and X-ray wavelengths to examine these claims. They found that the previous claims were exaggerated and the host star failed to display many of the brightness and spectral characteristics associated with stellar flaring and solar
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was used to map the planet's temperature emissions. The planet and star system was observed for 33 consecutive hours, starting when only the night side of the planet was in view. Over the course of one-half of the planet's orbit, more and more of the dayside came into view. A temperature range of 973
443:
The closest transiting hot
Jupiter to Earth, HD 189733 b has been the subject of close atmospheric observation. Scientists have studied it with high- and low-resolution instruments, both from the ground and from space. Researchers have found that the planet's weather includes raining molten glass. HD
773:
which lack titanium and vanadium oxides. Follow-up measurements, tested against a stratospheric model, yielded inconclusive results. Atmospheric condensates form a haze 1,000 kilometres (620 mi) above the surface as viewed in the infrared. A sunset viewed from that surface would be red. Sodium
632:
and molecular absorption in the red. The blue color of the planet was subsequently confirmed in 2013, which would have made HD 189733 the first planet to have its overall color determined by two different techniques. The measurements in polarized light have since been disputed by two separate teams
750:
observed. The parent stars of these two planets are the brightest transiting-planet host stars, so these planets will continue to receive the most attention from astronomers. Like most hot
Jupiters, this planet is thought to be tidally locked to its parent star, meaning it has a permanent day and
3137:
Albrecht, Simon; Winn, Joshua N.; Johnson, John A.; Howard, Andrew W.; Marcy, Geoffrey W.; Butler, R. Paul; Arriagada, Pamela; Crane, Jeffrey D.; Shectman, Stephen A.; Thompson, Ian B.; Hirano, Teruyuki; Bakos, Gaspar; Hartman, Joel D. (2012), "Obliquities of Hot
Jupiter Host Stars: Evidence for
761:
The international team under the direction of
Svetlana Berdyugina of Zurich University of Technology, using the Swedish 60-centimeter telescope KVA, which is located in Spain, was able to directly see the polarized light reflected from the planet. The polarization indicates that the scattering
704:
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Keles, E.; Kitzmann, D.; Mallonn, M.; Alexoudi, X.; Fossati, L.; Pino, L.; Seidel, J. V.; Carroll, T. A.; Steffen, M.; Ilyin, I.; Poppenhäger, K.; Strassmeier, K. G.; Von Essen, C.; Nascimbeni, V.; Turner, J. D. (2020), "Probing the atmosphere of HD189733b with the Na i and K i lines",
706:
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Oza, Apurva V.; Johnson, Robert E.; Lellouch, Emmanuel; Schmidt, Carl; Schneider, Nick; Huang, Chenliang; Gamborino, Diana; Gebek, Andrea; Wyttenbach, Aurelien; Demory, Brice-Olivier; Mordasini, Christoph; Saxena, Prabal; Dubois, David; Moullet, Arielle; Thomas, Nicolas (2019-08-28).
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temperature should cause the water and methane to react, replacing the atmosphere with carbon monoxide. Nonetheless, the presence of roughly 0.004% of water vapour fraction by volume in atmosphere of HD 189733 b was confirmed with high-resolution emission spectra taken in 2021.
778:'s sodium layer. The potassium was also detected in 2020, although in significantly smaller concentrations. HD 189733 is also the first extrasolar planet confirmed to have carbon dioxide in its atmosphere. In 2024, hydrogen sulfide was detected in HD 189733 b's atmosphere.
702:
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determined that HD 189733 b has winds of up to 8,700 km/h (5,400 mph) blowing from the day side to the night side. NASA released a brightness map of the surface temperature of HD 189733 b; it is the first map ever published of an extra-solar planet.
3418:
Keles, Engin; Mallonn, Matthias; von Essen, Carolina; Carroll, Thorsten; Alexoudi, Xanthippi; Pino, Lorenzo; Ilyin, Ilya; Poppenhager, Katja; Kitzmann, Daniel; Nascimbeni, Valerio; Turner, Jake D; Strassmeier, Klaus G (October 2019).
1963:
Wiktorowicz, Sloane J.; Nofi, Larissa A.; Jontof-Hutter, Daniel; Kopparla, Pushkar; Laughlin, Gregory P.; Hermis, Ninos; Yung, Yuk L.; Swain, Mark R. (2015-10-27). "A GROUND-BASED ALBEDO UPPER LIMIT FOR HD 189733b FROM POLARIMETRY".
1169:
Bonomo, A. S.; Desidera, S.; et al. (June 2017). "The GAPS Programme with HARPS-N at TNG. XIV. Investigating giant planet migration history via improved eccentricity and mass determination for 231 transiting planets".
1526:
Khalafinejad, S.; Essen, C. von; Hoeijmakers, H. J.; Zhou, G.; Klocová, T.; Schmitt, J. H. M. M.; Dreizler, S.; Lopez-Morales, M.; Husser, T.-O. (2017-02-01). "Exoplanetary atmospheric sodium revealed by orbital motion".
831:
published the results of their observations using the
Spitzer Space Telescope concluding there is solid evidence for significant amounts of water vapor in the planet's atmosphere. Follow-up observations made using the
1232:
Evans, Thomas M.; Pont, Frédéric; et al. (August 2013). "The Deep Blue Color of HD 189733b: Albedo
Measurements with Hubble Space Telescope/Space Telescope Imaging Spectrograph at Visible Wavelengths".
668:
of approximately 10 to 10 μm. Using both models, the planet's temperature would be between 1340 and 1540 K. The
Rayleigh effect is confirmed in other models, and by the apparent lack of a cooler, shaded
673:
below its outer atmosphere. In the visible region of the spectrum, thanks to their high absorption cross sections, atomic sodium and potassium can be investigated. For example, using high-resolution
701:
689:
In July 2013, NASA reported the first observations of planet transit studied in the X-ray spectrum. It was found that the planet's atmosphere blocks three times more X-rays than visible light.
888:
The
Rossiter–McLaughlin effect allows the measurement of the angle between the planet's orbital plane and the equatorial plane of the star. These are well aligned, misalignment equal to -0.5
714:
In March 2010, transit observations using HI Lyman-alpha found that this planet is evaporating at a rate of 1-100 gigagrams per second. This indication was found by detecting the extended
1710:
Berdyugina, S.V.; Berdyugin, A.V.; Fluri, D.M.; Piirola, V. (2011). "Polarized reflected light from the exoplanet HD189733b: First multicolor observations and confirmation of detection".
1343:
Knutson, Heather A.; Lewis, Nikole; et al. (July 2012). "3.6 and 4.5 μm Phase Curves and
Evidence for Non-equilibrium Chemistry in the Atmosphere of Extrasolar Planet HD 189733b".
2566:
Redfield; Endl, Michael; Cochran, William D.; Koesterke, Lars (2008). "Sodium
Absorption from the Exoplanetary Atmosphere of HD 189733b Detected in the Optical Transmission Spectrum".
1812:
Berdyugina, Svetlana V.; Andrei V. Berdyugin; Dominique M. Fluri; Vilppu Piirola (20 January 2008). "First detection of polarized scattered light from an exoplanetary atmosphere".
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around HD 189733 b. A 2014 study proposed a moon based on studying periodic increases and decreases in light given off from HD 189733 b. This moon would be outside of the planet's
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flares. Theoretical research since 2000 suggested that an exoplanet very near to the star that it orbits may cause increased flaring due to the interaction of their
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and potassium signals were predicted by Tinetti 2007. First obscured by the haze of condensates, sodium was eventually observed at three times the concentration of
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spectral lines caused by the planet occulting a part of the rotating stellar surface. Due to its high mass and close orbit, the parent star has a very large
3251:"ROME (Radio Observations of Magnetized Exoplanets). II. HD 189733 Does Not Accrete Significant Material from Its Exoplanet Like a T Tauri Star from a Disk"
2399:; Marley, M. S.; Freedman, R. S. (2008). "A Unified Theory for the Atmospheres of the Hot and Very Hot Jupiters: Two Classes of Irradiated Atmospheres".
2507:"Detection of atmospheric haze on an extrasolar planet: The 0.55 – 1.05 micron transmission spectrum of HD189733b with the Hubble Space Telescope"
2330:
Frédéric Pont; et al. (2008). "Hubble Space Telescope time-series photometry of the planetary transit of HD189733: no moon, no rings, starspots".
2755:
1794:
624:, which would have been the first such success. This result seemed to be confirmed and refined by the same team in 2011. They found that the planet
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In 2008, a team of astronomers first described how as the exoplanet orbiting HD 189733 A reaches a certain place in its orbit, it causes increased
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caused by the planet passing in front of its star before photometric measurements confirmed that the planet was transiting. In 2006, a team led by
602:
containing the first publication on the spectroscopic observation of the other exoplanet, HD 209458 b. A paper was submitted and published by the
681:, sodium has been detected on this atmosphere and further physical characteristics of the atmosphere such as temperature has been investigated.
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2025:
Bott, Kimberly; Bailey, Jeremy; Kedziora-Chudczer, Lucyna; Cotton, Daniel V.; Lucas, P. W.; Marshall, Jonathan P.; Hough, J. H. (2016-03-20).
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Deming; Harrington, Joseph; Seager, Sara; Jeremy Richardson (2006-02-20). "Strong Infrared Emission from the Extrasolar Planet HD189733b".
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Ben-Jaffel, Lotfi; Ballester, Gilda (May 18, 2013). "Hubble Space Telescope detection of oxygen in the atmosphere of exoplanet HD189733b".
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from the transiting exoplanet planet HD 189733 b, by measuring the flux decrement (decrease of total light) during its prominent secondary
2957:
3843:
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Knutson, Heather A.; Charbonneau, David; et al. (May 2007). "A map of the day-night contrast of the extrasolar planet HD 189733b".
534:
On October 6, 2005, a team of astronomers announced the discovery of transiting planet HD 189733 b. The planet was then detected using
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Swain, Mark R.; Vasisht, Gautam; Tinetti, Giovanna (2008-03-20). "The presence of methane in the atmosphere of an extrasolar planet".
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Berdyugina; Berdyugin; Fluri; Piirola (2008-02-02). "First Detection of Polarized Scattered Light from an Exoplanetary Atmosphere".
1648:
1235:
968:. In 2010, a different team found that every time they observe the exoplanet at a certain position in its orbit, they also detected
53:
2088:
1646:
Majeau, Carl; Agol, Eric; Cowan, Nicolas B. (March 2012). "A Two-dimensional Infrared Map of the Extrasolar Planet HD 189733b".
84:
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Krenn, A. F.; Lendl, M.; et al. (April 2023). "The geometric albedo of the hot Jupiter HD 189733b measured with CHEOPS".
870:
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109:
1400:"Estimating dayside effective temperatures of hot Jupiters and associated uncertainties through Gaussian process regression"
1113:"ELODIE metallicity-biased search for transiting Hot Jupiters II. A very hot Jupiter transiting the bright K star HD 189733"
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507:
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Ivan Hubeny; Adam Burrows (2008). "Spectrum and atmosphere models of irradiated transiting extrasolar giant planets".
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of 0.1564 solar radii. The Mie approximation model also found that there is a possible condensate in its atmosphere,
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4371:
3863:
1902:
Wiktorowicz, Sloane J. (2009-04-22). "NONDETECTION OF POLARIZED, SCATTERED LIGHT FROM THE HD 189733b HOT JUPITER".
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644:. In mid January 2008, spectral observation during the planet's transit using that model found that if molecular
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In 2008, a team of astrophysicists appeared to have detected and monitored the planet's visible light using
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2979:"Characterizing Exoplanetary Atmospheres at High Resolution with SPIRou: Detection of Water on HD 189733 b"
1000:. Later analysis demonstrated that very little, if any, gas was accreted from the "hot Jupiter" companion.
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3192:"The Rise of ROME. I. A Multiwavelength Analysis of the Star-Planet Interaction in the HD 189733 System"
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An artist's conception of HD 189733 b following the 2013 confirmation of the planet's blue color by the
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on the day side of the planet. It is currently unknown how the methane originated as the planet's high
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atmosphere is considerably larger (> 30%) than the opaque body of the planet seen during transits.
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3363:"Spectrally resolved detection of sodium in the atmosphere of HD 189733b with the HARPS spectrograph"
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Ben-Jaffel, Lotfi; Ballester, Gilda (3 April 2014). "Transit of Exomoon Plasma Tori: New Diagnosis".
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2901:"Detection of carbon monoxide in the high-resolution day-side spectrum of the exoplanet HD 189733b"
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Gregory W. Henry; et al. (2008). "The Rotation Period of the Planet-Hosting Star HD 189733".
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using more sensitive polarimeters, with upper limits of the polarimetric signal provided therein.
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452:, its overall color determined (deep blue), its transit viewed in the X-ray spectrum, and to have
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of 152.0 kilometers per second (152,000 meters per second; 340,000 miles per hour), making it a
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3481:"Sodium and Potassium Signatures of Volcanic Satellites Orbiting Close-in Gas Giant Exoplanets"
1016:, making its existence implausible. Two studies by the same team in 2019 and 2020 proposed exo-
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Eric Agol; et al. (2008). "Transits and secondary eclipses of HD 189733 with Spitzer".
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3608:"Radio-loud Exoplanet-exomoon Survey: GMRT Search for Electron Cyclotron Maser Emission"
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900:. A much larger angle would have suggested a violent interplay with other protoplanets.
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and a radius 11.4% greater, HD 189733 b orbits its host star once every 2.2 days at an
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2675:"James Webb telescope reveals rare, 'rotten egg' atmosphere around nearby hell planet"
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1036:. A follow-up study in 2022 did not find evidence for an exomoon around HD 189733 b.
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608:. The spectroscopic observations of HD 189733 b were led by Carl Grillmair of NASA's
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568:'s, with the planet completing an orbit around its host star every 2.2 days and an
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confirm the presence of water vapor, neutral oxygen and also the organic compound
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The atmosphere was at first predicted "pL class", lacking a temperature-inversion
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An artist's impression of HD 189733 b showing rapid evaporation of the atmosphere
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of its orbit is 16 degrees +/- 8 away from the north–south in our sky. It and
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2003:
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3542:"Alkaline exospheres of exoplanet systems: evaporative transmission spectra"
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Wyttenbach, A.; Ehrenreich, D.; Lovis, C.; Udry, S.; Pepe, F. (5 May 2015).
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is significantly larger in blue light than in the red, most probably due to
596:. The release came simultaneously with the public release of a new issue of
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1795:"Press Release: NASA's Spitzer First To Crack Open Light of Faraway Worlds"
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0.03100 ± 0.0006 AU (4,638,000 ± 90,000 km)
17:
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2089:"For First Time, Alien Planet's True Color Revealed: 'Deep Cobalt Blue'"
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NASA Exoplanet Exploration Program "horror film poster" for HD 189733 b
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2756:"Press Release: NASA's Spitzer Finds Water Vapor on Hot, Alien Planet"
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candidates around a number of hot Jupiters, including HD 189733 b and
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Short narrated video about the evaporation of HD 189733 b's atmosphere
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A. Lecavelier des Etangs; F. Pont; A. Vidal-Madjar; D. Sing (2008).
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1765:"RELEASE 14-197 - Hubble Finds Three Surprisingly Dry Exoplanets"
794:. The appearance of HD 189733 b beyond the blue color is unknown.
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2270:"Evaporation of the planet HD189733b observed in HI Lyman-alpha"
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416:. Astronomers in France discovered the planet orbiting the star
255:
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2251:"NASA's Chandra Sees Eclipsing Planet in X-rays for First Time"
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Pass, Emily K.; Cowan, Nicolas B.; et al. (October 2019).
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on three exoplanets that orbited Sun-like stars: HD 189733 b,
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across the star's face. With a mass 11.2% higher than that of
146:
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Data Release 3. Summary of the content and survey properties"
3606:
Narang, Mayank; Oza, Apurva V.; et al. (January 2023).
2138:"Rayleigh scattering in the transit spectrum of HD 189733b"
718:
of atomic hydrogen. HD 189733 b is the second planet after
3425:
Monthly Notices of the Royal Astronomical Society: Letters
2034:
Monthly Notices of the Royal Astronomical Society: Letters
564:
The mass of the planet is estimated to be 16% larger than
1789:
1787:
1451:
Vallenari, A.; et al. (Gaia collaboration) (2023).
2958:"Organic molecules found on alien world for first time"
527:
The planet's blue color was revealed using polarimetry.
2117:
Exoplanet Exploration: Planets Beyond our Solar System
869:
While transiting the system also clearly exhibits the
4810:
3421:"The potassium absorption on HD189733b and HD209458b"
722:
for which atmospheric evaporation has been detected.
3249:
Route, Matthew; Looney, Leslie (December 20, 2019).
27:
Hot Jupiter exoplanet in the constellation Vulpecula
4772:
4748:
4725:
4716:
4684:
4648:
4617:
4513:
4460:
4302:
4089:
3904:
3886:
3877:
2454:
Proceedings of the International Astronomical Union
2206:
Proceedings of the International Astronomical Union
1867:"First distant planet to be seen in colour is blue"
572:of 152.5 kilometres per second (341,000 mph).
358:
326:
304:
278:
254:
228:
223:
213:
192:
176:
158:
129:
119:
107:
100:
82:
74:
62:
52:
47:
3138:Tidal Interactions and Primordial Misalignments",
444:189733 b was also the first exoplanet to have its
3546:Monthly Notices of the Royal Astronomical Society
2778:
2776:
2622:Monthly Notices of the Royal Astronomical Society
2512:Monthly Notices of the Royal Astronomical Society
2268:Lecavelier des Etangs; et al. (2010-03-10).
1705:
1703:
1701:
1699:
1697:
1405:Monthly Notices of the Royal Astronomical Society
1763:Harrington, J.D.; Villard, Ray (July 24, 2014).
738:so far observed, approximately 3%. The apparent
2701:"Exoplanet's Global Winds Let Rip at 5,400 MPH"
734:(amount of the parent star's light blocked) of
2977:Boucher, Anne; et al. (9 November 2021).
456:confirmed as being present in its atmosphere.
3837:
1586:
1584:
448:constructed, possibly to be detected through
8:
1164:
1162:
1160:
1106:
1104:
1102:
30:
3540:Gebek, Andrea; Oza, Apurva (29 July 2020).
1227:
1225:
1223:
1221:
844:observations also detected the presence of
640:colour of HD 189733 b may be the result of
4769:
4722:
4681:
4645:
4614:
3883:
3844:
3830:
3822:
2660:"Carbon Dioxide Detected on Faraway World"
980:. In 2019, astronomers analyzed data from
823:Water vapor, oxygen, and organic compounds
746:were the first two planets to be directly
561:(when the planet passes behind the star).
36:
3744:
3676:
3643:
3625:
3575:
3557:
3516:
3498:
3454:
3436:
3378:
3321:
3284:
3266:
3225:
3207:
3151:
3097:
3032:"Rains of Terror on Exoplanet HD 189733b"
3014:
3004:
2994:
2916:
2859:
2798:
2643:
2633:
2579:
2542:
2524:
2465:
2412:
2343:
2290:
2217:
2155:
2063:
2045:
1977:
1915:
1878:
1825:
1723:
1661:
1606:
1540:
1490:
1472:
1435:
1417:
1358:
1303:
1248:
1185:
1148:
1138:
1128:
2383:Polarization technique focuses limelight
730:This planet exhibits one of the largest
696:
4817:
2199:
2197:
1098:
513:A global temperature map of HD 189733 b
4911:Exoplanets detected by radial velocity
2658:Robert Roy Britt (November 24, 2008).
29:
1521:
1519:
1008:Some studies have proposed candidate
420:on October 5, 2005, by observing its
7:
3190:Route, Matthew (February 10, 2019).
499:The infrared spectrum of HD 189733 b
463:announced the discovery of very dry
3712:"The Best Transiting Exoplanet Yet"
2899:de Kok, R. J.; et al. (2013).
960:Star-planet interaction controversy
2699:Klotz, Irene (November 16, 2015).
25:
2568:The Astrophysical Journal Letters
2113:"Exoplanet Catalog - HD 189733 b"
1649:The Astrophysical Journal Letters
1236:The Astrophysical Journal Letters
4868:
4856:
4844:
4832:
4820:
4797:
4796:
2956:Stephen Battersby (2008-02-11).
2544:10.1111/j.1365-2966.2008.12852.x
1111:Bouchy, F.; et al. (2005).
827:On July 11, 2007, a team led by
520:
506:
492:
484:Transit and Doppler spectroscopy
42:Jupiter and HD 189733 b compared
2027:"The polarization of HD 189733"
1865:Powell, Devin (July 11, 2013).
1507:Gaia DR3 record for this source
3869:Vulpecula in Chinese astronomy
915:From top left to lower right:
912:" exoplanets (artist concept).
550:announced detection of strong
383:(1,220 °C; 2,220 °F)
1:
4906:Exoplanets discovered in 2005
2505:F. Pont; et al. (2008).
2249:Boen, Brooke (May 20, 2015).
1712:Astrophysical Journal Letters
881:, the "wobble" in the star's
605:Astrophysical Journal Letters
3710:Naeye, Robert (2005-10-07).
3367:Astronomy & Astrophysics
3062:. 2007-03-05. Archived from
2848:Astronomy & Astrophysics
2673:Baker, Harry (8 July 2024).
2278:Astronomy & Astrophysics
2143:Astronomy & Astrophysics
1934:10.1088/0004-637X/696/2/1116
1529:Astronomy & Astrophysics
1291:Astronomy & Astrophysics
1173:Astronomy & Astrophysics
374:(919 °C; 1,686 °F)
3397:10.1051/0004-6361/201525729
3340:10.1088/2041-8205/785/2/L30
2935:10.1051/0004-6361/201321381
2878:10.1051/0004-6361/201221014
2309:10.1051/0004-6361/200913347
2174:10.1051/0004-6361:200809388
1891:– via www.nature.com.
1680:10.1088/2041-8205/747/2/L20
1559:10.1051/0004-6361/201629473
1492:10.1051/0004-6361/202243940
1322:10.1051/0004-6361/202245016
1267:10.1088/2041-8205/772/2/L16
1204:10.1051/0004-6361/201629882
1150:10.1051/0004-6361:200500201
740:longitude of ascending node
4927:
3864:List of stars in Vulpecula
3853:Constellation of Vulpecula
3170:10.1088/0004-637X/757/1/18
3116:10.1088/0004-6256/135/1/68
3030:Loff, Sarah (2016-10-31).
2905:Astronomy and Astrophysics
2725:"First Map of Alien World"
2362:10.1051/0004-6361:20078269
2332:Astronomy and Astrophysics
1996:10.1088/0004-637X/813/1/48
1742:10.1088/2041-8205/728/1/L6
1461:Astronomy and Astrophysics
1377:10.1088/0004-637X/754/1/22
1117:Astronomy and Astrophysics
871:Rossiter–McLaughlin effect
592:from both HD 189733 b and
544:Rossiter–McLaughlin effect
542:measurements detected the
69:Haute-Provence Observatory
4794:
4768:
4680:
4644:
4613:
3859:
3733:The Astrophysical Journal
3665:The Astrophysical Journal
3486:The Astrophysical Journal
3310:The Astrophysical Journal
3255:The Astrophysical Journal
3196:The Astrophysical Journal
3140:The Astrophysical Journal
2735:Jet Propulsion Laboratory
2484:10.1017/S1743921308026458
2228:10.1017/S1743921308026422
1966:The Astrophysical Journal
1904:The Astrophysical Journal
1880:10.1038/nature.2013.13376
1814:The Astrophysical Journal
1346:The Astrophysical Journal
732:photometric transit depth
648:exists, it would have an
387:
132:Orbital period (sidereal)
35:
3645:10.3847/1538-3881/ac9eb8
3613:The Astronomical Journal
3518:10.3847/1538-4357/ab40cc
3286:10.3847/1538-4357/ab594e
3227:10.3847/1538-4357/aafc25
3086:The Astronomical Journal
3016:10.3847/1538-3881/ac1f8e
2983:The Astronomical Journal
726:Physical characteristics
436:with poor prospects for
400:in the constellation of
224:Physical characteristics
3389:2015A&A...577A..62W
2927:2013A&A...554A..82D
2870:2013A&A...553A..52B
2730:Spitzer Space Telescope
2354:2007A&A...476.1347P
2301:2010A&A...514A..72L
2166:2008A&A...481L..83L
1551:2017A&A...598A.131K
1483:2023A&A...674A...1G
1314:2023A&A...672A..24K
1196:2017A&A...602A.107B
1140:2005A&A...444L..15B
800:Spitzer Space Telescope
586:Spitzer Space Telescope
584:released news that the
479:Detection and discovery
102:Orbital characteristics
3577:10.1093/mnras/staa2193
2645:10.1093/mnras/staa2435
956:
892:0.4°. By analogy with
861:
834:Hubble Space Telescope
811:
795:
792:Hubble Space Telescope
711:
610:Spitzer Science Center
588:had measured detailed
580:On February 21, 2007,
4901:Transiting exoplanets
3456:10.1093/mnrasl/slz123
2401:Astrophysical Journal
2065:10.1093/mnrasl/slw046
1437:10.1093/mnras/stz2226
906:
859:
816:University of Warwick
809:
789:
709:
438:extraterrestrial life
341:<0.12 (450–570 nm)
3060:University of Geneva
1024:, based on detected
998:T Tauri Star systems
842:Very Large Telescope
679:Very Large Telescope
677:spectrograph on the
650:atmospheric pressure
536:Doppler spectroscopy
91:Doppler spectroscopy
4774:Astronomical events
3817:Articles and images
3755:2006ApJ...644..560D
3717:Sky & Telescope
3687:2008ApJ...673L..83B
3636:2023AJ....165....1N
3568:2020MNRAS.497.5271G
3509:2019ApJ...885..168O
3447:2019MNRAS.489L..37K
3332:2014ApJ...785L..30B
3277:2019ApJ...887..229R
3218:2019ApJ...872...79R
3162:2012ApJ...757...18A
3108:2008AJ....135...68H
3006:2021AJ....162..233B
2817:10.1038/nature06823
2809:2008Natur.452..329S
2590:2008ApJ...673L..87R
2535:2008MNRAS.385..109P
2476:2009IAUS..253..239H
2423:2008ApJ...678.1419F
2056:2016MNRAS.459L.109B
1988:2015ApJ...813...48W
1926:2009ApJ...696.1116W
1836:2008ApJ...673L..83B
1734:2011ApJ...728L...6B
1672:2012ApJ...747L..20M
1625:10.1038/nature05782
1617:2007Natur.447..183K
1428:2019MNRAS.489..941P
1369:2012ApJ...754...22K
1259:2013ApJ...772L..16E
982:Arecibo Observatory
898:protoplanetary disc
885:, of 205 m/s.
642:Rayleigh scattering
630:Rayleigh scattering
404:approximately 64.5
75:Discovery date
64:Discovery site
32:
957:
879:semi-amplitude (K)
862:
814:Scientists at the
812:
796:
754:The planet is not
736:extrasolar planets
712:
658:magnesium silicate
54:Discovered by
4808:
4807:
4790:
4789:
4764:
4763:
4712:
4711:
4676:
4675:
4658:Brocchi's Cluster
4640:
4639:
4609:
4608:
2793:(7185): 329–331.
1801:on July 15, 2007.
1601:(7141): 183–186.
1004:Possible exomoons
782:Map of the planet
748:spectroscopically
707:
576:Infrared spectrum
391:
390:
16:(Redirected from
4918:
4873:
4872:
4871:
4861:
4860:
4859:
4849:
4848:
4847:
4837:
4836:
4825:
4824:
4823:
4816:
4800:
4799:
4770:
4723:
4682:
4646:
4615:
4521:ASKAP J1935+2148
3884:
3846:
3839:
3832:
3823:
3774:
3748:
3746:astro-ph/0602443
3727:
3725:
3724:
3706:
3680:
3650:
3649:
3647:
3629:
3603:
3597:
3596:
3594:
3592:
3579:
3561:
3552:(4): 5271–5291.
3537:
3531:
3530:
3520:
3502:
3475:
3469:
3468:
3458:
3440:
3415:
3409:
3408:
3382:
3358:
3352:
3351:
3325:
3305:
3299:
3298:
3288:
3270:
3246:
3240:
3239:
3229:
3211:
3187:
3181:
3180:
3155:
3134:
3128:
3127:
3101:
3081:
3075:
3074:
3072:
3071:
3056:"HD 189733 page"
3052:
3046:
3045:
3043:
3042:
3027:
3021:
3020:
3018:
3008:
2998:
2974:
2968:
2967:
2965:
2964:
2953:
2947:
2946:
2920:
2896:
2890:
2889:
2863:
2843:
2837:
2836:
2802:
2780:
2771:
2770:
2768:
2767:
2758:. Archived from
2752:
2746:
2745:
2743:
2742:
2721:
2715:
2714:
2712:
2711:
2696:
2690:
2689:
2687:
2685:
2670:
2664:
2663:
2655:
2649:
2648:
2647:
2637:
2616:
2610:
2609:
2583:
2563:
2557:
2556:
2546:
2528:
2502:
2496:
2495:
2469:
2449:
2443:
2442:
2416:
2407:(2): 1419–1435.
2395:Fortney, J. J.;
2392:
2386:
2380:
2374:
2373:
2347:
2338:(3): 1347–1355.
2327:
2321:
2320:
2294:
2274:
2265:
2259:
2258:
2246:
2240:
2239:
2221:
2201:
2192:
2191:
2189:
2188:
2159:
2133:
2127:
2126:
2124:
2123:
2109:
2103:
2102:
2100:
2099:
2087:Kramer, Miriam.
2084:
2078:
2077:
2067:
2049:
2040:(1): L109–L113.
2031:
2022:
2016:
2015:
1981:
1960:
1954:
1953:
1919:
1910:(2): 1116–1124.
1899:
1893:
1892:
1882:
1862:
1856:
1855:
1829:
1809:
1803:
1802:
1797:. Archived from
1791:
1782:
1781:
1779:
1777:
1760:
1754:
1753:
1727:
1707:
1692:
1691:
1665:
1643:
1637:
1636:
1610:
1588:
1579:
1578:
1544:
1523:
1514:
1504:
1494:
1476:
1448:
1442:
1441:
1439:
1421:
1395:
1389:
1388:
1362:
1340:
1334:
1333:
1307:
1285:
1279:
1278:
1252:
1229:
1216:
1215:
1189:
1166:
1155:
1154:
1152:
1142:
1132:
1130:astro-ph/0510119
1108:
976:, or because of
891:
851:
829:Giovanna Tinetti
708:
555:thermal emission
524:
510:
496:
412:) away from the
382:
380:
373:
368:
349:
347:
338:
336:
317:
300:
295:
294:
274:
264:
250:
240:
209:
204:
197:
188:
186:
172:
149:
144:
141:
85:Detection method
40:
33:
21:
4926:
4925:
4921:
4920:
4919:
4917:
4916:
4915:
4881:
4880:
4879:
4869:
4867:
4857:
4855:
4845:
4843:
4831:
4821:
4819:
4811:
4809:
4804:
4786:
4760:
4744:
4708:
4694:Dumbbell Nebula
4672:
4636:
4605:
4509:
4456:
4298:
4085:
3900:
3873:
3855:
3850:
3779:HD 189733 b on
3730:
3722:
3720:
3709:
3662:
3659:
3654:
3653:
3605:
3604:
3600:
3590:
3588:
3539:
3538:
3534:
3477:
3476:
3472:
3417:
3416:
3412:
3360:
3359:
3355:
3307:
3306:
3302:
3248:
3247:
3243:
3189:
3188:
3184:
3136:
3135:
3131:
3083:
3082:
3078:
3069:
3067:
3054:
3053:
3049:
3040:
3038:
3029:
3028:
3024:
2976:
2975:
2971:
2962:
2960:
2955:
2954:
2950:
2898:
2897:
2893:
2845:
2844:
2840:
2782:
2781:
2774:
2765:
2763:
2754:
2753:
2749:
2740:
2738:
2723:
2722:
2718:
2709:
2707:
2698:
2697:
2693:
2683:
2681:
2672:
2671:
2667:
2657:
2656:
2652:
2618:
2617:
2613:
2565:
2564:
2560:
2504:
2503:
2499:
2451:
2450:
2446:
2394:
2393:
2389:
2381:
2377:
2329:
2328:
2324:
2272:
2267:
2266:
2262:
2248:
2247:
2243:
2203:
2202:
2195:
2186:
2184:
2135:
2134:
2130:
2121:
2119:
2111:
2110:
2106:
2097:
2095:
2086:
2085:
2081:
2029:
2024:
2023:
2019:
1962:
1961:
1957:
1901:
1900:
1896:
1864:
1863:
1859:
1811:
1810:
1806:
1793:
1792:
1785:
1775:
1773:
1762:
1761:
1757:
1709:
1708:
1695:
1645:
1644:
1640:
1590:
1589:
1582:
1525:
1524:
1517:
1450:
1449:
1445:
1397:
1396:
1392:
1342:
1341:
1337:
1287:
1286:
1282:
1231:
1230:
1219:
1168:
1167:
1158:
1110:
1109:
1100:
1095:
1090:
1042:
1006:
974:magnetic fields
966:stellar flaring
962:
914:
913:
908:Comparison of "
889:
883:radial velocity
867:
849:
846:carbon monoxide
825:
784:
728:
697:
695:
687:
663:
618:
578:
540:radial velocity
532:
531:
530:
529:
528:
525:
516:
515:
514:
511:
502:
501:
500:
497:
486:
481:
378:
376:
375:
366:
364:
345:
343:
342:
340:
334:
332:
312:
309:
307:Surface gravity
292:
290:
289:
287:
284:
272:
262:
260:
248:
238:
236:
233:
202:
200:
193:
184:
182:
167:
164:
150:
142:
139:
137:
134:
112:
110:Semi-major axis
93:
87:
78:October 5, 2005
43:
28:
23:
22:
15:
12:
11:
5:
4924:
4922:
4914:
4913:
4908:
4903:
4898:
4893:
4883:
4882:
4878:
4877:
4865:
4853:
4841:
4829:
4806:
4805:
4795:
4792:
4791:
4788:
4787:
4785:
4784:
4778:
4776:
4766:
4765:
4762:
4761:
4759:
4758:
4752:
4750:
4746:
4745:
4743:
4742:
4737:
4731:
4729:
4720:
4714:
4713:
4710:
4709:
4707:
4706:
4701:
4696:
4690:
4688:
4678:
4677:
4674:
4673:
4671:
4670:
4665:
4660:
4654:
4652:
4642:
4641:
4638:
4637:
4635:
4634:
4629:
4623:
4621:
4611:
4610:
4607:
4606:
4604:
4603:
4598:
4593:
4588:
4583:
4581:PSR J2007+2722
4578:
4576:PSR J1946+2052
4573:
4568:
4563:
4558:
4553:
4548:
4543:
4538:
4533:
4528:
4523:
4517:
4515:
4511:
4510:
4508:
4507:
4502:
4497:
4492:
4487:
4482:
4477:
4472:
4466:
4464:
4458:
4457:
4455:
4454:
4449:
4444:
4439:
4434:
4429:
4424:
4419:
4414:
4409:
4404:
4399:
4394:
4389:
4384:
4379:
4374:
4369:
4364:
4359:
4354:
4349:
4344:
4339:
4334:
4329:
4324:
4319:
4314:
4308:
4306:
4300:
4299:
4297:
4296:
4291:
4286:
4281:
4276:
4271:
4266:
4261:
4256:
4251:
4246:
4241:
4236:
4231:
4226:
4221:
4216:
4211:
4206:
4201:
4196:
4191:
4186:
4181:
4176:
4171:
4166:
4161:
4156:
4151:
4146:
4141:
4136:
4131:
4126:
4121:
4116:
4111:
4106:
4101:
4095:
4093:
4087:
4086:
4084:
4083:
4076:
4071:
4066:
4061:
4056:
4051:
4046:
4041:
4036:
4031:
4026:
4021:
4016:
4011:
4006:
4001:
3996:
3991:
3986:
3981:
3976:
3971:
3966:
3961:
3956:
3951:
3946:
3941:
3936:
3931:
3926:
3921:
3916:
3910:
3908:
3902:
3901:
3899:
3898:
3892:
3890:
3881:
3875:
3874:
3872:
3871:
3866:
3860:
3857:
3856:
3851:
3849:
3848:
3841:
3834:
3826:
3820:
3819:
3777:
3775:
3763:10.1086/503358
3739:(1): 560–564.
3728:
3707:
3695:10.1086/527320
3671:(1): L83–L86.
3658:
3657:External links
3655:
3652:
3651:
3598:
3532:
3470:
3431:(1): L37-L41.
3410:
3353:
3300:
3241:
3182:
3129:
3076:
3047:
3022:
2969:
2948:
2891:
2838:
2772:
2747:
2716:
2691:
2665:
2650:
2611:
2598:10.1086/527475
2574:(1): L87–L90.
2558:
2519:(1): 109–118.
2497:
2444:
2431:10.1086/528370
2387:
2375:
2322:
2260:
2241:
2193:
2150:(2): L83–L86.
2128:
2104:
2079:
2017:
1955:
1894:
1857:
1844:10.1086/527320
1820:(1): L83–L86.
1804:
1783:
1755:
1693:
1638:
1580:
1515:
1443:
1412:(1): 941–950.
1390:
1335:
1280:
1217:
1156:
1123:(1): L15–L19.
1097:
1096:
1094:
1091:
1089:
1088:
1083:
1078:
1073:
1066:
1061:
1056:
1051:
1043:
1041:
1038:
1005:
1002:
990:active regions
961:
958:
907:
873:, shifting in
866:
863:
824:
821:
783:
780:
727:
724:
694:
691:
686:
685:X-ray spectrum
683:
661:
617:
614:
577:
574:
526:
519:
518:
517:
512:
505:
504:
503:
498:
491:
490:
489:
488:
487:
485:
482:
480:
477:
459:In July 2014,
454:carbon dioxide
389:
388:
385:
384:
362:
356:
355:
330:
324:
323:
310:
305:
302:
301:
285:
279:
276:
275:
270:
258:
252:
251:
246:
234:
229:
226:
225:
221:
220:
215:
211:
210:
198:
195:Semi-amplitude
190:
189:
180:
174:
173:
165:
159:
156:
155:
135:
130:
127:
126:
123:
117:
116:
113:
108:
105:
104:
98:
97:
88:
83:
80:
79:
76:
72:
71:
66:
60:
59:
56:
50:
49:
45:
44:
41:
26:
24:
14:
13:
10:
9:
6:
4:
3:
2:
4923:
4912:
4909:
4907:
4904:
4902:
4899:
4897:
4894:
4892:
4889:
4888:
4886:
4876:
4866:
4864:
4854:
4852:
4842:
4840:
4835:
4830:
4828:
4818:
4814:
4803:
4793:
4783:
4780:
4779:
4777:
4775:
4771:
4767:
4757:
4754:
4753:
4751:
4747:
4741:
4738:
4736:
4733:
4732:
4730:
4728:
4724:
4721:
4719:
4715:
4705:
4702:
4700:
4697:
4695:
4692:
4691:
4689:
4687:
4683:
4679:
4669:
4666:
4664:
4661:
4659:
4656:
4655:
4653:
4651:
4650:Star clusters
4647:
4643:
4633:
4630:
4628:
4625:
4624:
4622:
4620:
4616:
4612:
4602:
4601:SGR 1935+2154
4599:
4597:
4596:XTE J1859+226
4594:
4592:
4589:
4587:
4584:
4582:
4579:
4577:
4574:
4572:
4569:
4567:
4564:
4562:
4559:
4557:
4554:
4552:
4549:
4547:
4544:
4542:
4539:
4537:
4534:
4532:
4529:
4527:
4524:
4522:
4519:
4518:
4516:
4512:
4506:
4503:
4501:
4498:
4496:
4493:
4491:
4488:
4486:
4483:
4481:
4478:
4476:
4473:
4471:
4468:
4467:
4465:
4463:
4459:
4453:
4450:
4448:
4445:
4443:
4440:
4438:
4435:
4433:
4430:
4428:
4425:
4423:
4420:
4418:
4415:
4413:
4410:
4408:
4405:
4403:
4400:
4398:
4395:
4393:
4390:
4388:
4385:
4383:
4380:
4378:
4375:
4373:
4370:
4368:
4365:
4363:
4360:
4358:
4355:
4353:
4350:
4348:
4345:
4343:
4340:
4338:
4335:
4333:
4330:
4328:
4325:
4323:
4320:
4318:
4315:
4313:
4310:
4309:
4307:
4305:
4301:
4295:
4292:
4290:
4287:
4285:
4282:
4280:
4277:
4275:
4272:
4270:
4267:
4265:
4262:
4260:
4257:
4255:
4252:
4250:
4247:
4245:
4242:
4240:
4237:
4235:
4232:
4230:
4227:
4225:
4222:
4220:
4217:
4215:
4212:
4210:
4207:
4205:
4202:
4200:
4197:
4195:
4192:
4190:
4187:
4185:
4182:
4180:
4177:
4175:
4172:
4170:
4167:
4165:
4162:
4160:
4157:
4155:
4152:
4150:
4147:
4145:
4142:
4140:
4137:
4135:
4132:
4130:
4127:
4125:
4122:
4120:
4117:
4115:
4112:
4110:
4107:
4105:
4102:
4100:
4097:
4096:
4094:
4092:
4088:
4082:
4081:
4077:
4075:
4072:
4070:
4067:
4065:
4062:
4060:
4057:
4055:
4052:
4050:
4047:
4045:
4042:
4040:
4037:
4035:
4032:
4030:
4027:
4025:
4022:
4020:
4017:
4015:
4012:
4010:
4007:
4005:
4002:
4000:
3997:
3995:
3992:
3990:
3987:
3985:
3982:
3980:
3977:
3975:
3972:
3970:
3967:
3965:
3962:
3960:
3957:
3955:
3952:
3950:
3947:
3945:
3942:
3940:
3937:
3935:
3932:
3930:
3927:
3925:
3922:
3920:
3917:
3915:
3912:
3911:
3909:
3907:
3903:
3897:
3894:
3893:
3891:
3889:
3885:
3882:
3880:
3876:
3870:
3867:
3865:
3862:
3861:
3858:
3854:
3847:
3842:
3840:
3835:
3833:
3828:
3827:
3824:
3818:
3814:
3810:
3806:
3802:
3798:
3794:
3790:
3786:
3782:
3778:
3776:
3772:
3768:
3764:
3760:
3756:
3752:
3747:
3742:
3738:
3734:
3729:
3719:
3718:
3713:
3708:
3704:
3700:
3696:
3692:
3688:
3684:
3679:
3674:
3670:
3666:
3661:
3660:
3656:
3646:
3641:
3637:
3633:
3628:
3623:
3619:
3615:
3614:
3609:
3602:
3599:
3587:
3583:
3578:
3573:
3569:
3565:
3560:
3555:
3551:
3547:
3543:
3536:
3533:
3528:
3524:
3519:
3514:
3510:
3506:
3501:
3496:
3492:
3488:
3487:
3482:
3474:
3471:
3466:
3462:
3457:
3452:
3448:
3444:
3439:
3434:
3430:
3426:
3422:
3414:
3411:
3406:
3402:
3398:
3394:
3390:
3386:
3381:
3376:
3372:
3368:
3364:
3357:
3354:
3349:
3345:
3341:
3337:
3333:
3329:
3324:
3319:
3315:
3311:
3304:
3301:
3296:
3292:
3287:
3282:
3278:
3274:
3269:
3264:
3260:
3256:
3252:
3245:
3242:
3237:
3233:
3228:
3223:
3219:
3215:
3210:
3205:
3201:
3197:
3193:
3186:
3183:
3179:
3175:
3171:
3167:
3163:
3159:
3154:
3149:
3145:
3141:
3133:
3130:
3125:
3121:
3117:
3113:
3109:
3105:
3100:
3095:
3091:
3087:
3080:
3077:
3066:on 2008-02-06
3065:
3061:
3057:
3051:
3048:
3037:
3033:
3026:
3023:
3017:
3012:
3007:
3002:
2997:
2992:
2988:
2984:
2980:
2973:
2970:
2959:
2952:
2949:
2944:
2940:
2936:
2932:
2928:
2924:
2919:
2914:
2910:
2906:
2902:
2895:
2892:
2887:
2883:
2879:
2875:
2871:
2867:
2862:
2857:
2853:
2849:
2842:
2839:
2834:
2830:
2826:
2822:
2818:
2814:
2810:
2806:
2801:
2796:
2792:
2788:
2787:
2779:
2777:
2773:
2762:on 2007-07-15
2761:
2757:
2751:
2748:
2736:
2732:
2731:
2726:
2720:
2717:
2706:
2702:
2695:
2692:
2680:
2676:
2669:
2666:
2661:
2654:
2651:
2646:
2641:
2636:
2631:
2628:: 1023–1033,
2627:
2623:
2615:
2612:
2607:
2603:
2599:
2595:
2591:
2587:
2582:
2577:
2573:
2569:
2562:
2559:
2554:
2550:
2545:
2540:
2536:
2532:
2527:
2522:
2518:
2514:
2513:
2508:
2501:
2498:
2493:
2489:
2485:
2481:
2477:
2473:
2468:
2463:
2459:
2455:
2448:
2445:
2440:
2436:
2432:
2428:
2424:
2420:
2415:
2410:
2406:
2402:
2398:
2391:
2388:
2384:
2379:
2376:
2371:
2367:
2363:
2359:
2355:
2351:
2346:
2341:
2337:
2333:
2326:
2323:
2318:
2314:
2310:
2306:
2302:
2298:
2293:
2288:
2284:
2280:
2279:
2271:
2264:
2261:
2256:
2252:
2245:
2242:
2237:
2233:
2229:
2225:
2220:
2215:
2211:
2207:
2200:
2198:
2194:
2183:
2179:
2175:
2171:
2167:
2163:
2158:
2153:
2149:
2145:
2144:
2139:
2132:
2129:
2118:
2114:
2108:
2105:
2094:
2090:
2083:
2080:
2075:
2071:
2066:
2061:
2057:
2053:
2048:
2043:
2039:
2035:
2028:
2021:
2018:
2013:
2009:
2005:
2001:
1997:
1993:
1989:
1985:
1980:
1975:
1971:
1967:
1959:
1956:
1951:
1947:
1943:
1939:
1935:
1931:
1927:
1923:
1918:
1913:
1909:
1905:
1898:
1895:
1890:
1886:
1881:
1876:
1872:
1868:
1861:
1858:
1853:
1849:
1845:
1841:
1837:
1833:
1828:
1823:
1819:
1815:
1808:
1805:
1800:
1796:
1790:
1788:
1784:
1772:
1771:
1766:
1759:
1756:
1751:
1747:
1743:
1739:
1735:
1731:
1726:
1721:
1717:
1713:
1706:
1704:
1702:
1700:
1698:
1694:
1689:
1685:
1681:
1677:
1673:
1669:
1664:
1659:
1655:
1651:
1650:
1642:
1639:
1634:
1630:
1626:
1622:
1618:
1614:
1609:
1604:
1600:
1596:
1595:
1587:
1585:
1581:
1576:
1572:
1568:
1564:
1560:
1556:
1552:
1548:
1543:
1538:
1534:
1530:
1522:
1520:
1516:
1512:
1508:
1502:
1498:
1493:
1488:
1484:
1480:
1475:
1470:
1466:
1462:
1458:
1456:
1447:
1444:
1438:
1433:
1429:
1425:
1420:
1415:
1411:
1407:
1406:
1401:
1394:
1391:
1386:
1382:
1378:
1374:
1370:
1366:
1361:
1356:
1352:
1348:
1347:
1339:
1336:
1331:
1327:
1323:
1319:
1315:
1311:
1306:
1301:
1297:
1293:
1292:
1284:
1281:
1276:
1272:
1268:
1264:
1260:
1256:
1251:
1246:
1242:
1238:
1237:
1228:
1226:
1224:
1222:
1218:
1213:
1209:
1205:
1201:
1197:
1193:
1188:
1183:
1179:
1175:
1174:
1165:
1163:
1161:
1157:
1151:
1146:
1141:
1136:
1131:
1126:
1122:
1118:
1114:
1107:
1105:
1103:
1099:
1092:
1087:
1084:
1082:
1079:
1077:
1074:
1071:
1067:
1065:
1062:
1060:
1057:
1055:
1052:
1049:
1045:
1044:
1039:
1037:
1035:
1031:
1027:
1023:
1019:
1015:
1011:
1003:
1001:
999:
995:
991:
987:
983:
979:
975:
971:
967:
959:
954:
950:
946:
942:
938:
934:
930:
926:
922:
918:
911:
905:
901:
899:
895:
886:
884:
880:
876:
872:
864:
858:
854:
847:
843:
839:
835:
830:
822:
820:
817:
808:
804:
801:
798:In 2007, the
793:
788:
781:
779:
777:
772:
768:
763:
759:
757:
752:
749:
745:
741:
737:
733:
725:
723:
721:
717:
692:
690:
684:
682:
680:
676:
672:
667:
666:particle size
659:
655:
651:
647:
643:
639:
634:
631:
627:
623:
616:Visible color
615:
613:
611:
607:
606:
601:
600:
595:
591:
587:
583:
575:
573:
571:
570:orbital speed
567:
562:
560:
556:
553:
549:
545:
541:
537:
523:
509:
495:
483:
478:
476:
474:
470:
466:
462:
457:
455:
451:
447:
441:
439:
435:
431:
430:orbital speed
427:
423:
419:
415:
411:
407:
403:
399:
395:
386:
372:
363:
361:
357:
353:
331:
329:
325:
321:
316:
311:
308:
303:
299:
286:
283:
277:
273:
269:
259:
257:
253:
249:
245:
235:
232:
227:
222:
219:
216:
212:
208:
199:
196:
191:
181:
179:
175:
171:
166:
163:
162:orbital speed
157:
154:
148:
136:
133:
128:
124:
122:
118:
114:
111:
106:
103:
99:
96:
92:
89:
86:
81:
77:
73:
70:
67:
65:
61:
58:Bouchy et al.
57:
55:
51:
46:
39:
34:
19:
4896:Hot Jupiters
4875:Solar System
4631:
4571:PSR B2020+28
4566:PSR B1953+29
4561:PSR B1937+21
4556:PSR B1930+22
4551:PSR B1919+21
4078:
3736:
3732:
3721:. Retrieved
3715:
3668:
3664:
3617:
3611:
3601:
3589:. Retrieved
3549:
3545:
3535:
3490:
3484:
3473:
3428:
3424:
3413:
3370:
3366:
3356:
3313:
3309:
3303:
3258:
3254:
3244:
3199:
3195:
3185:
3143:
3139:
3132:
3092:(1): 68–71.
3089:
3085:
3079:
3068:. Retrieved
3064:the original
3050:
3039:. Retrieved
3035:
3025:
2986:
2982:
2972:
2961:. Retrieved
2951:
2908:
2904:
2894:
2851:
2847:
2841:
2790:
2784:
2764:. Retrieved
2760:the original
2750:
2739:. Retrieved
2737:. 2007-05-09
2728:
2719:
2708:. Retrieved
2704:
2694:
2682:. Retrieved
2678:
2668:
2662:. Space.com.
2653:
2625:
2621:
2614:
2571:
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2378:
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2254:
2244:
2209:
2205:
2185:. Retrieved
2147:
2141:
2131:
2120:. Retrieved
2116:
2107:
2096:. Retrieved
2092:
2082:
2037:
2033:
2020:
1969:
1965:
1958:
1907:
1903:
1897:
1870:
1860:
1817:
1813:
1807:
1799:the original
1774:. Retrieved
1768:
1758:
1718:(1): L6–L9.
1715:
1711:
1653:
1647:
1641:
1598:
1592:
1532:
1528:
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1350:
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1338:
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1240:
1234:
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1120:
1116:
1007:
978:tidal forces
963:
932:
887:
875:photospheric
868:
826:
813:
797:
767:stratosphere
764:
760:
753:
729:
713:
688:
671:stratosphere
652:of 410 ± 30
635:
619:
603:
597:
579:
563:
548:Drake Deming
538:. Real-time
533:
458:
442:
414:Solar System
393:
392:
339:(290–450 nm)
267:
243:
121:Eccentricity
4863:Outer space
4851:Spaceflight
4632:HD 189733 b
4627:HD 188015 b
2679:LiveScience
2460:: 239–245.
2397:Lodders, K.
2212:: 209–215.
1070:HD 209458 b
1064:Kepler-186f
1059:HD 149026 b
1048:51 Pegasi b
1014:Hill sphere
953:HD 209458 b
933:HD 189733 b
910:hot Jupiter
894:HD 149026 b
776:HD 209458 b
744:HD 209458 b
720:HD 209458 b
693:Evaporation
638:cobalt blue
622:polarimetry
594:HD 209458 b
469:HD 209458 b
465:atmospheres
450:polarimetry
446:thermal map
434:hot Jupiter
406:light-years
394:HD 189733 b
360:Temperature
265:0.045
241:0.027
231:Mean radius
178:Inclination
168:152.0
151:53.2458048
31:HD 189733 b
4885:Categories
4782:AT 2021lwx
4619:Exoplanets
4546:HIP 100963
4541:GS 2000+25
4526:BD+23 3912
3809:Astrophoto
3801:Hydrogen α
3723:2008-06-21
3627:2210.13298
3591:8 December
3559:2005.02536
3500:1908.10732
3493:(2): 168.
3438:1909.04884
3380:1503.05581
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3268:1911.08357
3261:(2): 229.
3209:1901.02048
3070:2008-02-18
3041:2019-12-13
2996:2108.08390
2989:(6). 233.
2963:2008-02-12
2766:2007-07-11
2741:2009-09-30
2710:2015-11-17
2635:2008.04044
2187:2008-08-08
2122:2024-01-28
2098:2024-01-28
2047:1603.05745
1979:1507.03588
1656:(2): L20.
1542:1610.01610
1474:2208.00211
1419:1908.02631
1305:2301.07731
1243:(2): L16.
1187:1704.00373
1093:References
1086:WASP-189 b
1046:Dimidium (
994:protostars
313:21.5
145:(77)
125:<0.0039
4891:Vulpecula
4827:Astronomy
4699:Hen 2-437
4586:Wolf 1346
3906:Flamsteed
3896:α (Anser)
3678:0712.0193
3586:218516741
3527:201651224
3465:202134796
3348:119282630
3323:1404.1084
3295:208158242
3236:119350145
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3146:(1): 18,
3099:0709.2142
2918:1304.4014
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2861:1303.4232
2833:205212651
2800:0802.1030
2581:0712.0761
2526:0712.1374
2467:0807.3588
2414:0710.2558
2345:0707.1940
2292:1003.2206
2219:0807.2434
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2093:SpaceNews
2074:1745-3925
2012:118086125
2004:1538-4357
1972:(1): 48.
1942:0004-637X
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1889:130070356
1827:0712.0193
1725:1101.0059
1688:118492172
1663:1202.1883
1608:0705.0993
1567:0004-6361
1501:244398875
1360:1206.6887
1353:(1): 22.
1330:255999905
1250:1307.3239
1212:118923163
1054:HD 2039 b
1034:gas torus
1030:potassium
937:HAT-P-12b
865:Evolution
840:. Later,
716:exosphere
664:) with a
636:The rich
418:HD 189733
402:Vulpecula
398:exoplanet
381:68 K
352:geometric
218:HD 189733
205:1.6
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18:HD189733b
4802:Category
4718:Galaxies
4668:NGC 6940
4663:NGC 6885
4531:G 185-32
4091:Variable
3771:14434391
3703:14366978
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2492:13978248
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1068:Osiris (
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1022:WASP-49b
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941:WASP-17b
929:WASP-39b
925:WASP-31b
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771:L dwarfs
646:hydrogen
552:infrared
473:WASP-12b
160:Average
4813:Portals
4686:Nebulae
3813:Sky Map
3781:WikiSky
3751:Bibcode
3683:Bibcode
3632:Bibcode
3564:Bibcode
3505:Bibcode
3443:Bibcode
3385:Bibcode
3373:: A62.
3328:Bibcode
3273:Bibcode
3214:Bibcode
3158:Bibcode
3104:Bibcode
3001:Bibcode
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2805:Bibcode
2684:10 July
2606:2028887
2586:Bibcode
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2162:Bibcode
2052:Bibcode
1984:Bibcode
1922:Bibcode
1832:Bibcode
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1424:Bibcode
1365:Bibcode
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1135:Bibcode
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751:night.
590:spectra
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559:eclipse
426:Jupiter
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410:parsecs
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4704:Sh2-88
4591:WR 125
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4490:190066
4485:189671
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850:700 °C
756:oblate
660:(MgSiO
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599:Nature
471:, and
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396:is an
328:Albedo
296:
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291:+0.081
187:0.060°
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4514:Other
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3888:Bayer
3879:Stars
3805:X-Ray
3793:GALEX
3767:S2CID
3741:arXiv
3699:S2CID
3673:arXiv
3622:arXiv
3582:S2CID
3554:arXiv
3523:S2CID
3495:arXiv
3461:S2CID
3433:arXiv
3401:S2CID
3375:arXiv
3344:S2CID
3318:arXiv
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3263:arXiv
3232:S2CID
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3174:S2CID
3148:arXiv
3120:S2CID
3094:arXiv
2991:arXiv
2939:S2CID
2913:arXiv
2882:S2CID
2856:arXiv
2829:S2CID
2795:arXiv
2705:Space
2630:arXiv
2602:S2CID
2576:arXiv
2549:S2CID
2521:arXiv
2488:S2CID
2462:arXiv
2435:S2CID
2409:arXiv
2366:S2CID
2340:arXiv
2313:S2CID
2287:arXiv
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2178:S2CID
2152:arXiv
2042:arXiv
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2008:S2CID
1974:arXiv
1946:S2CID
1912:arXiv
1885:S2CID
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1746:S2CID
1720:arXiv
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1658:arXiv
1603:arXiv
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1271:S2CID
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1182:arXiv
1125:arXiv
970:X-ray
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365:1,192
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344:0.076
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280:Mean
261:1.123
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201:201.3
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