1148:
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682:
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689:
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1116:
2102:; Robertson, Paul; Ninan, Joe P.; Beard, Corey; Bender, Chad F.; Cochran, William D.; Cunha, Katia; Diddams, Scott A.; Fredrick, Connor; Halverson, Samuel; Hearty, Fred; Ickler, Adam; Kanodia, Shubham; Libby-Roberts, Jessica E.; Lubin, Jack; Metcalf, Andrew J.; Olsen, Freja; Ramsey, Lawrence W.; Roy, Arpita; Schwab, Christian; Smith, Verne V.; Turner, Ben (3 March 2022).
6524:
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1546:'s orbit, it would reach Barnard's Star in 47 years under parameters similar to those of the original Project Daedalus. Once at the star, it would begin automated self-replication, constructing a factory, initially to manufacture exploratory probes and eventually to create a copy of the original spacecraft after 1,000 years.
2738:
Benedict, G. Fritz; McArthur, Barbara; Nelan, E.; Story, D.; Whipple, A. L.; Shelus, P. J.; Jefferys, W. H.; Hemenway, P. D.; Franz, Otto G.; Wasserman, L. H.; Duncombe, R. L.; Van Altena, W.; Fredrick, L. W. (1998). "Photometry of
Proxima Centauri and Barnard's star using Hubble Space Telescope fine
1035:
range; this, plus its high space motion, have led to the designation "intermediate population II star", between a halo and disk star. However, some recently published scientific papers have given much higher estimates for the metallicity of the star, very close to the Sun's level, between 75 and 125%
970:
is the closest star to the Sun at a position currently 4.24 light-years distant from it. However, despite
Barnard's Star's even closer pass to the Sun in 11,800 CE, it will still not then be the nearest star, since by that time Proxima Centauri will have moved to a yet-nearer proximity to the Sun. At
3932:
France, Kevin; Duvvuri, Girish; Egan, Hilary; Koskinen, Tommi; Wilson, David J.; Youngblood, Allison; Froning, Cynthia S.; Brown, Alexander; Alvarado-Gomez, Julian D.; Berta-Thompson, Zachory K.; Drake, Jeremy J.; Garraffo, Cecilia; Kaltenegger, Lisa; Kowalski, Adam F.; Linsky, Jeffrey L.; Loyd, R.
1167:
orbiting in relatively close proximity to
Barnard's Star. Led by Ignasi Ribas of Spain their work, conducted over two decades of observation, provided strong evidence of the planet's existence. However, the existence of the planet was refuted in 2021, because the radial velocity signal was found to
1127:
and
Heinrich Eichhorn, at a different observatory and using newer plate measuring techniques, failed to verify the planetary companion. Another paper published by John L. Hershey four months earlier, also using the Swarthmore observatory, found that changes in the astrometric field of various stars
1326:
on the outer edge of the optimistic habitable zone, corresponding to orbital periods of up to 10 and 40 days respectively. Therefore, it appears that
Barnard's Star indeed does not host Earth-mass planets or larger, in hot and temperate orbits, unlike other M-dwarf stars that commonly have these
3639:
Benedict, G. Fritz; McArthur, Barbara; Chappell, D. W.; Nelan, E.; Jefferys, W. H.; Van Altena, W.; Lee, J.; Cornell, D.; Shelus, P. J.; Hemenway, P. D.; Franz, Otto G.; Wasserman, L. H.; Duncombe, R. L.; Story, D.; Whipple, A. L.; Fredrick, L. W. (1999). "Interferometric
Astrometry of Proxima
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and lead to sudden outbursts: strong magnetic fields occur in rapidly rotating stars, while old stars tend to rotate slowly. For
Barnard's Star to undergo an event of such magnitude is thus presumed to be a rarity. Research on the star's periodicity, or changes in stellar activity over a given
1925:
Cutri, R. M.; Skrutskie, M. F.; Van Dyk, S.; Beichman, C. A.; Carpenter, J. M.; Chester, T.; Cambresy, L.; Evans, T.; Fowler, J.; Gizis, J.; Howard, E.; Huchra, J.; Jarrett, T.; Kopan, E. L.; Kirkpatrick, J. D.; Light, R. M.; Marsh, K. A.; McCallon, H.; Schneider, S.; Stiening, R.; Sykes, M.;
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for both circular and eccentric orbits, upper masses for planets out to 1,000-day orbits were determined. Planets above two Earth masses in orbits of less than 10 days were excluded, and planets of more than ten Earth masses out to a two-year orbit were also confidently ruled out. It was also
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correlated to the timing of adjustments and modifications that had been carried out on the refractor telescope's objective lens; the claimed planet was attributed to an artifact of maintenance and upgrade work. The affair has been discussed as part of a broader scientific review.
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the time of the star's closest pass by the Sun, Barnard's Star will still be too dim to be seen with the naked eye, since its apparent magnitude will only have increased by one magnitude to about 8.5 by then, still being 2.5 magnitudes short of visibility to the naked eye.
1504:. Undertaken between 1973 and 1978, the study suggested that rapid, uncrewed travel to another star system was possible with existing or near-future technology. Barnard's Star was chosen as a target partly because it was believed to have planets.
1309:
The analysis of radial velocities that eventually led to discovery of the candidate super-Earth orbiting
Barnard's Star was also used to set more precise upper mass limits for possible planets, up to and within the habitable zone: a maximum of
1403:
with energy 1.6×10 joules. The flare rate observed to date is enough to cause loss of 87 Earth atmospheres per billion years through thermal processes and ≈3 Earth atmospheres per billion years through ion loss processes on
Barnard's Star b.
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For the more than four decades between van de Kamp's rejected claim and the eventual announcement of a planet candidate, Barnard's Star was carefully studied and the mass and orbital boundaries for possible planets were slowly tightened.
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Riedel, A. R.; Guinan, E. F.; DeWarf, L. E.; Engle, S. G.; McCook, G. P. (May 2005). "Barnard's Star as a Proxy for Old Disk dM Stars: Magnetic
Activity, Light Variations, XUV Irradiances, and Planetary Habitable Zones".
1085:
that would indicate a planetary companion; this involved as many as ten people averaging their results in looking at plates, to avoid systemic individual errors. Van de Kamp's initial suggestion was a planet having about
1352:
K, more than twice the normal temperature of the star. Given the essentially random nature of flares, Diane Paulson, one of the authors of that study, noted that "the star would be fantastic for amateurs to observe".
1424:
Barnard's Star shares much the same neighborhood as the Sun. The neighbors of Barnard's Star are generally of red dwarf size, the smallest and most common star type. Its closest neighbor is currently the red dwarf
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on 17 July during an unrelated search for variations in the proper motion. Four years passed before the flare was fully analyzed, at which point it was suggested that the flare's temperature was 8,000
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were impossible around Barnard's Star, in a paper which helped refine the negative certainty regarding planetary objects in general. In 1999, the Hubble work further excluded planetary companions of
2935:
Matthews, R. A. J.; Weissman, P. R.; Preston, R. A.; Jones, D. L.; Lestrade, J.-F.; Latham, D. W.; Stefanik, R. P.; Paredes, J. M. (1994). "The Close Approach of Stars in the Solar Neighborhood".
1008:. Barnard's Star is so faint that if it were at the same distance from Earth as the Sun is, it would appear only 100 times brighter than a full moon, comparable to the brightness of the Sun at 80
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Kürster, M.; Endl, M.; Rouesnel, F.; Els, S.; Kaufer, A.; Brillant, S.; Hatzes, A. P.; Saar, S. H.; Cochran, W. D. (23 May 2003). "The low-level radial velocity variability in Barnard's Star".
3764:
Choi, Jieun; McCarthy, Chris; Marcy, Geoffrey W; Howard, Andrew W; Fischer, Debra A; Johnson, John A; Isaacson, Howard; Wright, Jason T (2012). "Precise Doppler Monitoring of Barnard's Star".
1200:
would have been possible in the decade after its discovery. Further faint and unaccounted-for perturbations in the system suggested there may be a second planetary companion even farther out.
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timescale, also suggest it ought to be quiescent; 1998 research showed weak evidence for periodic variation in the star's brightness, noting only one possible starspot over 130 days.
1953:
Samus, N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (2009) . "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+, 2007–2017)".
1298:, which was to begin searching for extrasolar Earth-like planets, was reported to have chosen Barnard's Star as an early search target, however the mission was shut down in 2010.
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In 2013, a research paper was published that further refined planet mass boundaries for the star. Using radial velocity measurements, taken over a period of 25 years, from the
1101:
AU in a slightly eccentric orbit, and these measurements were apparently refined in a 1969 paper. Later that year, Van de Kamp suggested that there were two planets of 1.1 and
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The flare was surprising because intense stellar activity is not expected in stars of such age. Flares are not completely understood, but are believed to be caused by strong
4245:
3877:
Paulson, Diane B.; Allred, Joel C.; Anderson, Ryan B.; Hawley, Suzanne L.; Cochran, William D.; Yelda, Sylvana (2006). "Optical Spectroscopy of a Flare on Barnard's Star".
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1192:. The planet would have most likely been frigid, with an estimated surface temperature of about −170 °C (−274 °F), and lie outside Barnard Star's presumed
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galaxy. Barnard's Star has lost a great deal of rotational energy, and the periodic slight changes in its brightness indicate that it rotates once in 130 days (the
681:
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3933:
O. Parke; Mauas, Pablo J. D.; Miguel, Yamila; Pineda, J. Sebastian; Rugheimer, Sarah; Schneider, P. Christian; Tian, Feng; Vieytes, Mariela (2 September 2020).
2169:
1371:
Stellar activity of this sort has created interest in using Barnard's Star as a proxy to understand similar stars. It is hoped that photometric studies of its
890:
At 7–12 billion years of age, Barnard's Star is considerably older than the Sun, which is 4.5 billion years old, and it might be among the oldest stars in the
2966:
2593:
4242:
4218:
1926:
Weinberg, M.; Wheaton, W. A.; Wheelock, S.; Zacarias, N. (June 2003). "VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)".
3581:
Endl, Michael; Cochran, William D.; Tull, Robert G.; MacQueen, Phillip J. (2003). "A Dedicated M Dwarf Planet Search Using the Hobby-Eberly Telescope".
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km/s. The 10.3 arcseconds it travels in a year amount to a quarter of a degree in a human lifetime, roughly half the angular diameter of the full Moon.
1437:
are, respectively, the next closest systems. From Barnard's Star, the Sun would appear on the diametrically opposite side of the sky at coordinates RA=
1383:
implications: given that the habitable zones of M dwarfs are close to the star, any planet located therein would be strongly affected by solar flares,
898:
rotates in 25). Given its age, Barnard's Star was long assumed to be quiescent in terms of stellar activity. In 1998, astronomers observed an intense
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1139:, questioned his findings and began publishing criticisms from 1976 onwards. The two men were reported to have become estranged because of this.
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Even though this research greatly restricted the possible properties of planets around Barnard's Star, it did not rule them out completely as
1213:
such as Barnard's Star are more easily studied than larger stars in this regard because their lower masses render perturbations more obvious.
2320:
1523:. The star could then be reached in 50 years, within a human lifetime. Along with detailed investigation of the star and any companions, the
1598:" means the mass of the planet times the sine of the angle of inclination of its orbit, and hence provides the minimum mass for the planet.
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with an orbital period of less than 1,000 days (Jupiter's orbital period is 4,332 days), while Kuerster determined in 2003 that within the
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Other astronomers subsequently repeated Van de Kamp's measurements, and two papers in 1973 undermined the claim of a planet or planets.
1031:. While sub-solar, Barnard's Star's metallicity is higher than that of a halo star and is in keeping with the low end of the metal-rich
4085:
831:
planetary companion known as Barnard's Star b was reported to orbit Barnard's Star. It was believed to have a minimum mass of 3.2
3458:"Super-Earth Orbiting Barnard's Star – Red Dots campaign uncovers compelling evidence of exoplanet around closest single star to Sun"
1283:
discovered that the habitable zone of the star seemed to be devoid of roughly Earth-mass planets or larger, save for face-on orbits.
952:. Barnard's Star will make its closest approach to the Sun around 11,800 CE, when it will approach to within about 3.75 light-years.
914:
of a star caused by its motion. Further variability in the radial velocity of Barnard's Star was attributed to its stellar activity.
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1131:
Van de Kamp never acknowledged any error and published a further claim of two planets' existence as late as 1982; he died in 1995.
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Barnard's Star has been subject to multiple claims of planets that were later disproven. From the early 1960s to the early 1970s,
6645:
2714:
2684:
2284:
Seeliger, Hugo; Bauschinger, Julius (1890). "Erstes Müchner Sternverzeichniss enthaltend die mittleren Örter von 33082 Sternen".
856:
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Paulson, Diane B.; Allred, Joel C.; Anderson, Ryan B.; Hawley, Suzanne L.; Cochran, William D.; Yelda, Sylvana (February 2006).
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60:
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Centauri and Barnard's Star Using Hubble Space Telescope Fine Guidance Sensor 3: Detection Limits for Substellar Companions".
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Barnard's Star is among the most studied red dwarfs because of its proximity and favorable location for observation near the
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within 9 light years (ly) from the map's center, the Sun (Sol). The diamond-shapes are their positions entered according to
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3002:
987:), and a radius about 0.2 times that of the Sun. Thus, although Barnard's Star has roughly 150 times the mass of Jupiter (
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1445:. The absolute magnitude of the Sun is 4.83, and at a distance of 1.834 parsecs, it would be a first-magnitude star, as
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602:
598:
1267:), or with a mass greater than 3.1 times the mass of Neptune (much lower than van de Kamp's smallest suggested value).
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and helps classify stars relative to the galactic population. Barnard's Star seems to be typical of the old, red dwarf
3155:
van de Kamp, Peter (1963). "Astrometric study of Barnard's star from plates taken with the 24-inch Sproul refractor".
3026:"Exploring the stellar properties of M dwarfs with high-resolution spectroscopy from the optical to the near-infrared"
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per year relative to the Sun, the highest known for any star. The star had previously appeared on Harvard University
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6361:
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2336:
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1412:
4991:
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4328:
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2198:
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3359:"The Search for the Extrasolar Planets: A Brief History of the Search, the Findings and the Future Implications"
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Animated image with frames approx. one year apart, beginning in 2007, showing the movement of Barnard's Star.
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3508:
Artigau, Étienne; Cadieux, Charles; Cook, Neil J.; Doyon, René; Vandal, Thomas; et al. (23 June 2022).
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is about 16% of the Sun's, and it has 19% of the Sun's diameter. Despite its proximity, the star has a dim
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1175:, which is an ideal spot for the icy accretion of proto-planetary material. It was thought to orbit at 0.4
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575:
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1865:
Gizis, John E. (February 1997). "M-Subdwarfs: Spectroscopic Classification and the Metallicity Scale".
3315:"Astrometric analysis of the field of AC +65 6955 from plates taken with the Sproul 24-inch refractor"
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Bobylev, Vadim V. (13 March 2010). "Searching for stars closely encountering with the solar system".
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2014:
1962:
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804:. Historically, research on Barnard's Star has focused on measuring its stellar characteristics, its
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emissions will shed light on the large population of old M dwarfs in the galaxy. Such research has
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2004:
1993:"The M-dwarf Ultraviolet Spectroscopic Sample. I. Determining Stellar Parameters for Field Stars"
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for this star on 1 February 2017 and it is now included in the List of IAU-approved Star Names.
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5926:
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1689:{\displaystyle {\begin{smallmatrix}m=4.83+5\cdot ((\log _{10}1.834)-1)=1.15\end{smallmatrix}}}
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For a decade from 1963 to about 1973, a substantial number of astronomers accepted a claim by
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53:
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due to its motion toward the Sun. Combined with its proper motion and distance, this gives a
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4679:
4372:
4077:
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3174:
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2418:
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2133:
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2022:
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1501:
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1441:, Dec=−04° 41′ 36″, in the westernmost part of the constellation
1361:
1271:
967:
621:
528:
493:
471:
338:
3510:"Line-by-line velocity measurements, an outlier-resistant method for precision velocimetry"
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4712:
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Null results for planetary companions continued throughout the 1980s and 1990s, including
1124:
911:
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83:
2615:"Stellar Activity Manifesting at a One-year Alias Explains Barnard b as a False Positive"
1061:
of Barnard's Star consistent with its having one or more planets comparable in mass with
4196:
4129:
4047:
3960:
3902:
3787:
3665:
3606:
3531:
3398:
3330:
3289:
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3211:
3170:
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2541:
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2297:
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2211:
2182:
2129:
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2018:
1966:
1939:
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were detected, each with far-ultraviolet energy of 3×10 joules, together with one X-ray
1065:. Van de Kamp had been observing the star from 1938, attempting, with colleagues at the
6449:
5931:
5179:
5169:
4772:
4742:
4707:
4697:
4674:
4669:
4659:
4356:
1531:
1520:
1508:
1434:
1357:
1247:
1193:
863:(WGSN) to catalogue and standardize proper names for stars. The WGSN approved the name
747:
633:
567:
346:
326:
314:
4111:
3795:
2964:
Ochsenbein, F. (March 1982). "A list of stars with large expected angular diameters".
2505:
Ribas, I.; Tuomi, M.; Reiners, Ansgar; Butler, R. P.; et al. (14 November 2018).
6574:
6137:
6132:
6081:
5154:
5149:
4702:
4684:
4664:
4436:
4291:
3978:
3724:
3406:
3077:
2921:
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2147:
2036:
1845:
1818:
1775:
1446:
1400:
1396:
1341:
1058:
910:
V2500 Ophiuchi. In 2003, Barnard's Star presented the first detectable change in the
899:
876:
786:
723:
303:
255:
70:
17:
3918:
3852:
3803:
3681:
3622:
3235:
van de Kamp, Peter (August 1969). "Alternate dynamical analysis of Barnard's star".
2866:
2778:
2479:
2374:
1906:
1168:
originate from a stellar activity cycle, and a study in 2022 confirmed this result.
6540:
6371:
6151:
5249:
4767:
4762:
4757:
4747:
4737:
4692:
4541:
4347:
3935:"The High-Energy Radiation Environment Around a 10 Gyr M Dwarf: Habitable at Last?"
3695:
Gatewood, George D. (1995). "A study of the astrometric motion of Barnard's star".
1384:
1303:
1180:
1132:
1028:
988:
755:
449:
405:
3060:
3025:
2710:
2098:
Terrien, Ryan C.; Keen, Allison; Oda, Katy; Parts, Winter; Stefánsson, Guðmundur;
1766:
1727:
1530:
The initial Project Daedalus model sparked further theoretical research. In 1980,
1159:
In November 2018, an international team of astronomers announced the detection by
996:), its radius is only roughly 2 times larger, due to its much higher density. Its
3272:"An unsuccessful search for a planetary companion of Barnard's star (BD +4 3561)"
2858:
2613:
Lubin, Jack; Robertson, Paul; Stefansson, Gudmundur; et al. (15 July 2021).
1019:. Metallicity is the proportion of stellar mass made up of elements heavier than
925:
The proper motion of Barnard's Star corresponds to a relative lateral speed of 90
6356:
6286:
6251:
5019:
4974:
4969:
4964:
4959:
4954:
4949:
4944:
4939:
4934:
4929:
4924:
4919:
4914:
4909:
4904:
4895:
4890:
4885:
4880:
4875:
4870:
4865:
4860:
4855:
4850:
4845:
4840:
4835:
4830:
4825:
4820:
4815:
4810:
4805:
4800:
4795:
4790:
4727:
4722:
4717:
4498:
4489:
4379:
3358:
2196:
Perepelkin, E. (April 1927). "Einweißer Stern mit bedeutender absoluter Größe".
1620:
1478:
1171:
Dubbed Barnard's Star b, the planet was thought to be near the stellar system's
1164:
1152:
1136:
1016:
828:
763:
245:
234:
223:
212:
96:
4154:
3969:
3934:
3540:
3509:
2998:
2649:
2614:
2138:
2103:
2027:
1992:
1306:
interferometry mission had the same goal, but was stripped of funding in 2007.
827:
were refuted in the mid-1970s after much debate. In November 2018, a candidate
6281:
6276:
6271:
6266:
6261:
6036:
5966:
5956:
4980:
2913:
2549:
2507:"A candidate super-Earth planet orbiting near the snow line of Barnard's star"
2340:
1558:– Nearly identical to Barnard's star, and hosts three sub-Earth sized planets.
1482:
1474:
1364:
1311:
1259:
1184:
1074:
979:
975:
903:
832:
813:
805:
782:
731:
422:
361:
267:
40:
27:
Red dwarf star about six light-years from Earth in the constellation Ophiuchus
4580:
3069:
2658:
2573:
2565:
2219:
847:. However, work presented in July 2021 refuted the existence of this planet.
6291:
6256:
6127:
6122:
6117:
6099:
6061:
5905:
5900:
5890:
5885:
5865:
5835:
5830:
5820:
5622:
5557:
5269:
5264:
4506:
4449:
4401:
3194:"Parallax, proper motion acceleration, and orbital motion of Barnard's Star"
2104:"Rotational Modulation of Spectroscopic Zeeman Signatures in Low-mass Stars"
1555:
1512:
1477:(indicated at the edge of the map's reference disc), and according to their
1442:
1115:
1032:
937:
891:
880:
824:
790:
727:
719:
702:
75:
3482:
3457:
2581:
1991:
Pineda, J. Sebastian; Youngblood, Allison; France, Kevin (September 2021).
6415:
6410:
6405:
6400:
6325:
6320:
6230:
6225:
6220:
6215:
6210:
6205:
6200:
6195:
6190:
6185:
6180:
6175:
6170:
6112:
5961:
5946:
5941:
4462:
4423:
4200:
3893:
3656:
3597:
2841:
2753:
2454:
1881:
1519:) and accelerating for four years could achieve a velocity of 12% of the
1516:
1426:
823:
argued that planets orbited Barnard's Star. His specific claims of large
767:
556:
1564: – Stars and brown dwarfs within 20 light years of the Solar System
917:
6246:
6051:
5976:
5936:
5239:
3716:
1543:
1210:
1062:
63:
56:
2557:
1607:
The Sun's apparent magnitude from Barnard's Star, assuming negligible
1507:
The theoretical model suggested that a nuclear pulse rocket employing
921:
Barnard's Star, showing position every 5 years in the period 1985–2005
6431:
6385:
6305:
4310:
3994:"NASA's Spitzer and WISE Telescopes Find Close, Cold Neighbor of Sun"
3385:
Van de Kamp, Peter (1982). "The planetary system of Barnard's star".
3096:
1785:
1430:
1020:
1001:
735:
651:
520:
435:
366:
4176:
2286:
Neue Annalen der Koeniglichen Sternwarte in Bogenhausen bei Muenchen
6535:
3951:
3910:
3673:
3614:
3522:
3339:
3314:
3298:
3271:
3256:
3220:
3193:
3178:
3042:
2770:
2631:
2532:
2471:
2422:
2120:
2083:
2056:
2009:
1898:
1748:
6016:
3778:
2896:
1456:
1411:
1372:
1146:
1114:
954:
916:
771:
611:
4642:
3998:
1291:
617:
330:
318:
4584:
4214:
1527:
would be examined and baseline astrometric readings performed.
4336:
1819:"UBV(RI)C JHK observations of Hipparcos-selected nearby stars"
1417:
1299:
895:
743:
540:
1732:
Data Release 3. Summary of the content and survey properties"
1224:
in 1999. Gatewood was able to show in 1995 that planets with
4168:
The Encyclopedia of Astrobiology, Astronomy, and Spaceflight
4082:
The Encyclopedia of Astrobiology, Astronomy, and Spaceflight
2399:(September 1916). "A small star with large proper motion".
1481:. The second mark shows each's distance from Sol, with the
1376:
1119:
Artist's conception of a planet in orbit around a red dwarf
812:. Although Barnard's Star is ancient, it still experiences
3375:(Full description of the Van de Kamp planet controversy.)
1250:
around Barnard's Star, planets are not possible with an "
1135:, Van de Kamp's successor at Swarthmore and an expert on
3122:. July 2005. Archived from the original on 4 August 2011
1817:
Koen, C.; Kilkenny, D.; Van Wyk, F.; Marang, F. (2010).
1726:
Vallenari, A.; et al. (Gaia collaboration) (2023).
4181:
Amateur work showing Barnard's Star movement over time.
3880:
Publications of the Astronomical Society of the Pacific
2442:
Publications of the Astronomical Society of the Pacific
1566:
Pages displaying short descriptions of redirect targets
1344:
on Barnard's Star was detected based on changes in the
1258:" value greater than 7.5 times the mass of the Earth (
963:
from 20,000 years ago until 80,000 years in the future
578:, "Barnard's Runaway Star", "Greyhound of the Skies",
6512:
1617:
45:
The location of Barnard's Star, c. 2006 (south is up)
3992:
Clavin, Whitney; Harrington, J. D. (25 April 2014).
3431:. Swarthmore College. pp. 28–31. Archived from
6474:
6448:
6424:
6393:
6384:
6334:
6313:
6304:
6239:
6161:
6150:
6098:
5914:
5806:
5328:
4990:
4781:
4650:
4641:
4549:
4535:
4497:
4488:
4400:
4327:
4301:
4290:
4256:
3024:Rajpurohit, A. S.; Allard, F.; et al. (2018).
2938:
Quarterly Journal of the Royal Astronomical Society
2438:"Optical Spectroscopy of a Flare on Barnard's Star"
1573: – M-type red dwarf in the constellation Aries
1485:
circles indicating the distance in steps of one ly.
4071:
4069:
2057:"Barnard's Star and the M Dwarf Temperature Scale"
1688:
1824:Monthly Notices of the Royal Astronomical Society
1196:. Direct imaging of the planet and its tell-tale
701:Location of Barnard's Star in the constellation
4197:"Exoplanet discovered around neighbouring star"
3557:"A Frozen Super-Earth May Orbit Barnard's Star"
2733:
2731:
2236:(1960). "A Model of our Stellar Neighborhood".
688:
3845:"Darwin factsheet: Finding Earth-like planets"
3516:. 164:84 (3) (published 8 August 2022): 18pp.
2055:Dawson, P. C.; De Robertis, M. M. (May 2004).
4596:
4226:
4117:Journal of the British Interplanetary Society
4035:Journal of the British Interplanetary Society
4023:
4021:
3102:Centre de Données astronomiques de Strasbourg
2993:
2991:
2989:
2170:Bulletin of the American Astronomical Society
1538:intended to search for and make contact with
1290:were always going to be difficult to detect.
101:+04° 41′ 36.1139″
8:
3270:Gatewood, George & Eichhorn, H. (1973).
2967:Astronomy and Astrophysics Supplement Series
2608:
2606:
2238:Astronomical Society of the Pacific Leaflets
2161:
2159:
2157:
1986:
1984:
1982:
1980:
1978:
1976:
3634:
3632:
808:, and also refining the limits of possible
6471:
6445:
6390:
6310:
6158:
6095:
4647:
4603:
4589:
4581:
4546:
4532:
4494:
4485:
4368:K-type main-sequence star B (Toliman)
4298:
4287:
4268:
4253:
4233:
4219:
4211:
3872:
3870:
2822:
2820:
2818:
1420:, including Barnard's Star (25 April 2014)
1027:, yet these are also generally metal-poor
3968:
3950:
3892:
3777:
3655:
3596:
3539:
3521:
3338:
3297:
3219:
3059:
3041:
2895:
2840:
2752:
2648:
2630:
2531:
2453:
2137:
2119:
2082:
2026:
2008:
1880:
1844:
1765:
1747:
1721:
1719:
1717:
1715:
1713:
1651:
1618:
1616:
1004:, and it has a luminosity of only 0.0034
932:The radial velocity of Barnard's Star is
879:M4, and it is too faint to see without a
875:Barnard's Star is a red dwarf of the dim
4105:
4103:
4030:"Project Daedalus – The mission profile"
2790:
2788:
2681:"IAU Working Group on Star Names (WGSN)"
2625:(2). American Astronomical Society: 61.
2500:
2498:
2496:
2360:
2358:
2263:"Barnard's Star and its Perturbations".
2050:
2048:
2046:
1151:Artist's impression of the surface of a
974:Barnard's Star has a mass of about 0.16
6636:Objects with variable star designations
6586:Astronomical objects discovered in 1916
6519:
4243:Celestial objects within 10 light-years
4112:"A Self-Reproducing Interstellar Probe"
3361:. Arizona State University. Section 2.
3352:
3350:
1920:
1918:
1916:
1860:
1858:
1856:
1709:
1583:
1511:(specifically, electron bombardment of
1015:Barnard's Star has 10–32% of the solar
750:system, and is the closest star in the
310:
4446:2 (3?) planets: b, d?, c
3133:
1812:
1810:
1808:
1806:
1804:
1802:
1800:
1798:
1796:
1794:
1562:List of nearest stars and brown dwarfs
1500:Barnard's Star was studied as part of
1073:, to find minuscule variations of one
944:(actual speed relative to the Sun) of
31:
6596:Discoveries by Edward Emerson Barnard
4028:Bond, A. & Martin, A. R. (1976).
3483:"Super-Earth Orbiting Barnard's Star"
1327:types of planets in close-in orbits.
1179:AU every 233 days and had a proposed
7:
4110:Freitas, Robert A. Jr. (July 1980).
3740:"Barnard's Star: No Sign of Planets"
2315:. Sterling Publishing. p. 158.
1461:The position of Barnard's Star on a
1395:In 2019, two additional ultraviolet
816:events, one being observed in 1998.
59:
4179:. Jack Schmidling Productions, Inc.
4088:from the original on 31 August 2006
3365:from the original on 13 August 2006
3005:from the original on 20 August 2006
2599:from the original on 26 March 2019.
1955:VizieR On-line Data Catalog: B/gcvs
1928:VizieR On-line Data Catalog: II/246
1534:suggested a more ambitious plan: a
902:, showing that Barnard's Star is a
322:
4006:from the original on 26 April 2014
3819:"Updates from the Project Manager"
3555:Billings, Lee (14 November 2018).
3092:"VizieR record for Barnard's Star"
1319:up to the inner edge and 1.2
746:after the three components of the
25:
4195:Rincon, Paul (14 November 2018).
3851:. 23 October 2009. Archived from
2691:from the original on 10 June 2016
2367:"Barnard's Star (V2500 Ophiuchi)"
2365:Kaler, James B. (November 2005).
1619:
1465:map among all stellar objects or
345:546.9759 ± 0.0401
6558:
6546:
6534:
6522:
6499:
6498:
3738:Gilster, Paul (16 August 2012).
2715:International Astronomical Union
2685:International Astronomical Union
2373:. James B. Kaler. Archived from
1846:10.1111/j.1365-2966.2009.16182.x
1433:(5.41 light-years). The Sun and
857:International Astronomical Union
762:of +9.5 and is invisible to the
687:
680:
39:
3817:Marr, James (8 November 2010).
2795:Croswell, Ken (November 2005).
1782:Gaia DR3 record for this source
1053:that he had detected, by using
6621:Hypothetical planetary systems
4623:Ophiuchus in Chinese astronomy
4378:2 (5?) planets:
3697:Astrophysics and Space Science
3357:Bell, George H. (April 2001).
3313:Hershey, John L. (June 1973).
1672:
1663:
1644:
1641:
1387:, and plasma ejection events.
1:
4273:Celestial objects by systems.
4199:. Science & Environment.
3487:European Southern Observatory
1204:Refining planetary boundaries
766:; it is much brighter in the
752:northern celestial hemisphere
4433:1? planets: b?
4311:Sirius (Alpha Canis Majoris)
4076:Darling, David (July 2005).
3407:10.1016/0083-6656(82)90004-6
3116:"The Barnard's Star Blunder"
3030:Astronomy & Astrophysics
2797:"A Flare for Barnard's Star"
2524:Holtzbrinck Publishing Group
2337:"Astronomy Survey Fall 2010"
1296:Space Interferometry Mission
1045:Astrometric planetary claims
3796:10.1088/0004-637X/764/2/131
3429:Swarthmore College Bulletin
3192:van de Kamp, Peter (1969).
3061:10.1051/0004-6361/201833500
1767:10.1051/0004-6361/202243940
1536:self-replicating spacecraft
1278:Observatories and applying
861:Working Group on Star Names
6662:
6631:M-type main-sequence stars
6362:Rho Ophiuchi cloud complex
4628:List of stars in Ophiuchus
4612:Constellation of Ophiuchus
4459:red dwarf B (UV Ceti)
2859:10.1051/0004-6361:20030396
2829:Astronomy and Astrophysics
1736:Astronomy and Astrophysics
1493:
1036:of the solar metallicity.
628:J17578+046, Munich 15040,
6496:
6470:
6444:
6094:
6072:WISEP J180026.60+013453.1
4618:
4531:
4516:T-type brown dwarf B
4484:
4286:
4271:
4252:
3766:The Astrophysical Journal
3420:Kent, Bill (March 2001).
3140:: CS1 maint: unfit URL (
2914:10.1134/S1063773710030060
2550:10.1038/s41586-018-0677-y
2199:Astronomische Nachrichten
2108:The Astrophysical Journal
1997:The Astrophysical Journal
908:variable star designation
906:. Barnard's Star has the
785:who in 1916 measured its
760:apparent visual magnitude
675:
644:
573:
566:
562:
399:
394:
390:
273:
266:
118:
50:
37:
6626:Local Interstellar Cloud
5831:149143 (Rosalíadecastro)
3970:10.3847/1538-3881/abb465
3939:The Astronomical Journal
3643:The Astronomical Journal
3584:The Astronomical Journal
3541:10.3847/1538-3881/ac7ce6
3514:The Astronomical Journal
3319:The Astronomical Journal
3277:The Astronomical Journal
3237:The Astronomical Journal
3199:The Astronomical Journal
3158:The Astronomical Journal
2803:. Kalmbach Publishing Co
2741:The Astronomical Journal
2650:10.3847/1538-3881/ac0057
2619:The Astronomical Journal
2402:The Astronomical Journal
2220:10.1002/asna.19272300406
2139:10.3847/2041-8213/ac4fc8
2062:The Astronomical Journal
2028:10.3847/1538-4357/ac0aea
1868:The Astronomical Journal
1542:. Built and launched in
1429:, at a distance of 1.66
1057:, a perturbation in the
777:The star is named after
738:) from Earth, it is the
730:. At a distance of 5.96
6646:Stars with proper names
6027:2MASS J16452211-1319516
4357:α Cen (Rigil Kentaurus)
3709:1995Ap&SS.223...91G
3052:2018A&A...620A.180R
2980:1982A&AS...47..523O
2851:2003A&A...403.1077K
2313:Constellation Guidebook
1758:2023A&A...674A...1G
1155:orbiting Barnard's Star
936:, as measured from the
742:individual star to the
462:Luminosity (bolometric)
376:Absolute magnitude
201:Apparent magnitude
190:Apparent magnitude
179:Apparent magnitude
168:Apparent magnitude
157:Apparent magnitude
146:Apparent magnitude
108:Apparent magnitude
6601:Durchmusterung objects
6458:Ophiuchus Supercluster
5305:V2500 (Barnard's Star)
3821:. NASA. Archived from
2311:Rukl, Antonin (1999).
1690:
1486:
1421:
1222:Hubble Space Telescope
1156:
1142:
1120:
964:
922:
779:Edward Emerson Barnard
637:
365:(1.8282 ± 0.0001
6611:Gliese and GJ objects
6591:BY Draconis variables
6352:Ophiuchus Superbubble
6128:GJ 1214 b (Enaiposha)
4450:Gliese 65 A (BL Ceti)
3849:European Space Agency
3120:Astrobiology Magazine
2234:Lippincott, Sarah Lee
1691:
1540:extraterrestrial life
1460:
1416:Stars closest to the
1415:
1150:
1118:
1083:orbital perturbations
998:effective temperature
958:
920:
484:Luminosity (visual, L
360:5.9629 ± 0.0004
325: 10362.394
18:Barnard's Star b
4375:(4.2465 ± 0.0003 ly)
4373:C (Proxima Centauri)
1615:
1453:Proposed exploration
1280:Monte Carlo analysis
1097:at a distance of 4.4
740:fourth-nearest-known
313: −801.551
6476:Astronomical events
6367:Serpens–Aquila Rift
6347:Double Helix Nebula
4241:
4130:1980JBIS...33..251F
4078:"Daedalus, Project"
4048:1976JBIS...29..101B
3961:2020AJ....160..237F
3903:2006PASP..118..227P
3788:2013ApJ...764..131C
3666:1999AJ....118.1086B
3607:2003AJ....126.3099E
3561:Scientific American
3532:2022AJ....164...84A
3399:1982VA.....26..141V
3387:Vistas in Astronomy
3331:1973AJ.....78..421H
3290:1973AJ.....78..769G
3249:1969AJ.....74..757V
3212:1969AJ.....74..238V
3171:1963AJ.....68..515V
2951:1994QJRAS..35....1M
2906:2010AstL...36..220B
2763:1998AJ....116..429B
2739:guidance senso 3".
2641:2021AJ....162...61L
2542:2018Natur.563..365R
2464:2006PASP..118..227P
2415:1916AJ.....29..181B
2377:on 5 September 2006
2298:1890AnBog...1....1S
2250:1960ASPL....8..207L
2212:1927AN....230...77P
2183:2005AAS...206.0904R
2130:2022ApJ...927L..11T
2075:2004AJ....127.2909D
2019:2021ApJ...918...40P
1967:2009yCat....102025S
1940:2003yCat.2246....0C
1891:1997AJ....113..806G
1837:2010MNRAS.403.1949K
1525:interstellar medium
1449:is from the Earth.
1288:terrestrial planets
1079:photographic plates
1077:in its position on
1025:population II stars
795:photographic plates
695:Barnard's Star
645:Database references
34:
6484:Kepler's Supernova
4320:white dwarf B
4175:Schmidling, Jack.
4054:on 20 October 2007
3717:10.1007/BF00989158
3489:. 14 November 2018
3422:"Barnard's Wobble"
2801:Astronomy Magazine
2100:Mahadevan, Suvrath
1686:
1684:
1683:
1487:
1422:
1346:spectral emissions
1157:
1121:
1071:Swarthmore College
1067:Sproul Observatory
1040:Search for planets
1010:astronomical units
1006:solar luminosities
965:
923:
885:apparent magnitude
810:extrasolar planets
797:in 1888 and 1890.
568:Other designations
256:Variable type
135:Apparent magnitude
125:Spectral type
32:
6616:Hipparcos objects
6510:
6509:
6492:
6491:
6466:
6465:
6440:
6439:
6380:
6379:
6300:
6299:
6146:
6145:
6090:
6089:
6007:Great Annihilator
4680:ε (Yed Posterior)
4633:Taurus Poniatovii
4578:
4577:
4574:
4573:
4570:
4569:
4527:
4526:
4523:
4522:
4480:
4479:
4476:
4475:
4282:
4281:
4278:
4277:
3591:(12): 3099–3107.
2883:Astronomy Letters
2322:978-0-8069-3979-7
1360:, which suppress
1051:Peter van de Kamp
959:Distances to the
821:Peter van de Kamp
802:celestial equator
713:
712:
614:J17574849+0441405
16:(Redirected from
6653:
6563:
6562:
6561:
6551:
6550:
6549:
6539:
6538:
6527:
6526:
6525:
6518:
6502:
6501:
6472:
6446:
6391:
6311:
6159:
6108:CFHTWIR-Oph 98 b
6096:
6057:Van Biesbroeck 8
5977:GJ 1214 (Okaria)
5861:152581 (Mahsati)
4866:36 (A, Guniibuu)
4648:
4605:
4598:
4591:
4582:
4562:
4547:
4537:Sub-brown dwarfs
4533:
4512:
4495:
4486:
4468:
4455:
4442:
4429:
4419:
4406:
4362:
4350:
4345:
4316:
4299:
4288:
4269:
4265:
4260:
4254:
4235:
4228:
4221:
4212:
4204:
4190:
4187:"Barnard's Star"
4180:
4177:"Barnard's Star"
4171:
4164:"Barnard's Star"
4162:Darling, David.
4158:
4155:"Barnard's Star"
4141:
4140:
4138:
4136:
4107:
4098:
4097:
4095:
4093:
4073:
4064:
4063:
4061:
4059:
4050:. Archived from
4025:
4016:
4015:
4013:
4011:
3989:
3983:
3982:
3972:
3954:
3929:
3923:
3922:
3896:
3894:astro-ph/0511281
3874:
3865:
3864:
3862:
3860:
3841:
3835:
3834:
3832:
3830:
3814:
3808:
3807:
3781:
3761:
3755:
3754:
3752:
3750:
3735:
3729:
3728:
3692:
3686:
3685:
3659:
3657:astro-ph/9905318
3650:(2): 1086–1100.
3636:
3627:
3626:
3600:
3598:astro-ph/0308477
3578:
3572:
3571:
3569:
3567:
3552:
3546:
3545:
3543:
3525:
3505:
3499:
3498:
3496:
3494:
3479:
3473:
3472:
3470:
3468:
3454:
3448:
3447:
3445:
3443:
3437:
3426:
3417:
3411:
3410:
3382:
3376:
3374:
3372:
3370:
3354:
3345:
3344:
3342:
3310:
3304:
3303:
3301:
3267:
3261:
3260:
3232:
3226:
3225:
3223:
3189:
3183:
3182:
3152:
3146:
3145:
3139:
3131:
3129:
3127:
3112:
3106:
3105:
3088:
3082:
3081:
3063:
3045:
3021:
3015:
3014:
3012:
3010:
2999:"Barnard's Star"
2995:
2984:
2983:
2961:
2955:
2954:
2932:
2926:
2925:
2899:
2877:
2871:
2870:
2844:
2842:astro-ph/0303528
2835:(6): 1077–1088.
2824:
2813:
2812:
2810:
2808:
2792:
2783:
2782:
2756:
2754:astro-ph/9806276
2735:
2726:
2725:
2723:
2721:
2707:
2701:
2700:
2698:
2696:
2677:
2671:
2670:
2652:
2634:
2610:
2601:
2600:
2598:
2535:
2511:
2502:
2491:
2490:
2488:
2486:
2457:
2455:astro-ph/0511281
2448:(840): 227–235.
2433:
2427:
2426:
2409:(695): 181–183.
2393:
2387:
2386:
2384:
2382:
2362:
2353:
2352:
2350:
2348:
2339:. Archived from
2333:
2327:
2326:
2308:
2302:
2301:
2281:
2275:
2274:
2260:
2254:
2253:
2230:
2224:
2223:
2193:
2187:
2186:
2163:
2152:
2151:
2141:
2123:
2095:
2089:
2088:
2086:
2069:(5): 2909–2914.
2052:
2041:
2040:
2030:
2012:
1988:
1971:
1970:
1950:
1944:
1943:
1922:
1911:
1910:
1884:
1882:astro-ph/9611222
1862:
1851:
1850:
1848:
1814:
1789:
1779:
1769:
1751:
1723:
1697:
1695:
1693:
1692:
1687:
1685:
1656:
1655:
1605:
1599:
1588:
1571:Teegarden's Star
1567:
1502:Project Daedalus
1496:Project Daedalus
1490:Project Daedalus
1440:
1351:
1238:
1227:
1178:
1143:Barnard's Star b
1104:
1100:
1089:
1081:consistent with
968:Proxima Centauri
951:
949:
942:"space velocity"
935:
928:
846:
770:than in visible
691:
690:
684:
615:
588:
576:Proxima Ophiuchi
543:
538:
518:
516:
469:
447:
445:
420:
419:
418:
324:
312:
296:
294:
119:Characteristics
111:
91:
86:
51:Observation data
43:
35:
21:
6661:
6660:
6656:
6655:
6654:
6652:
6651:
6650:
6571:
6570:
6569:
6559:
6557:
6547:
6545:
6533:
6523:
6521:
6513:
6511:
6506:
6488:
6462:
6450:Galaxy clusters
6436:
6420:
6376:
6330:
6296:
6235:
6153:
6142:
6086:
6012:IRAS 16293−2422
5910:
5802:
5324:
4986:
4777:
4637:
4614:
4609:
4579:
4566:
4560:
4539:
4519:
4510:
4472:
4466:
4453:
4440:
4427:
4417:
4404:
4403:
4396:
4371:red dwarf
4360:
4353:Alpha Centauri
4342:
4323:
4314:
4293:
4274:
4257:
4248:
4239:
4208:
4194:
4185:Johnson, Rick.
4184:
4174:
4161:
4153:
4150:
4145:
4144:
4134:
4132:
4109:
4108:
4101:
4091:
4089:
4075:
4074:
4067:
4057:
4055:
4027:
4026:
4019:
4009:
4007:
3991:
3990:
3986:
3931:
3930:
3926:
3876:
3875:
3868:
3858:
3856:
3843:
3842:
3838:
3828:
3826:
3825:on 2 March 2011
3816:
3815:
3811:
3763:
3762:
3758:
3748:
3746:
3744:Centauri Dreams
3737:
3736:
3732:
3694:
3693:
3689:
3638:
3637:
3630:
3580:
3579:
3575:
3565:
3563:
3554:
3553:
3549:
3507:
3506:
3502:
3492:
3490:
3481:
3480:
3476:
3466:
3464:
3456:
3455:
3451:
3441:
3439:
3438:on 19 July 2011
3435:
3424:
3419:
3418:
3414:
3384:
3383:
3379:
3368:
3366:
3356:
3355:
3348:
3312:
3311:
3307:
3269:
3268:
3264:
3234:
3233:
3229:
3191:
3190:
3186:
3154:
3153:
3149:
3132:
3125:
3123:
3114:
3113:
3109:
3090:
3089:
3085:
3023:
3022:
3018:
3008:
3006:
3001:. Sol Station.
2997:
2996:
2987:
2963:
2962:
2958:
2934:
2933:
2929:
2879:
2878:
2874:
2826:
2825:
2816:
2806:
2804:
2794:
2793:
2786:
2737:
2736:
2729:
2719:
2717:
2709:
2708:
2704:
2694:
2692:
2679:
2678:
2674:
2612:
2611:
2604:
2596:
2509:
2504:
2503:
2494:
2484:
2482:
2435:
2434:
2430:
2395:
2394:
2390:
2380:
2378:
2364:
2363:
2356:
2346:
2344:
2343:on 26 June 2013
2335:
2334:
2330:
2323:
2310:
2309:
2305:
2283:
2282:
2278:
2262:
2261:
2257:
2232:
2231:
2227:
2195:
2194:
2190:
2165:
2164:
2155:
2097:
2096:
2092:
2054:
2053:
2044:
1990:
1989:
1974:
1952:
1951:
1947:
1924:
1923:
1914:
1864:
1863:
1854:
1816:
1815:
1792:
1725:
1724:
1711:
1706:
1701:
1700:
1682:
1681:
1647:
1613:
1612:
1606:
1602:
1589:
1585:
1580:
1565:
1552:
1498:
1492:
1471:right ascension
1467:stellar systems
1455:
1438:
1410:
1393:
1381:astrobiological
1358:magnetic fields
1349:
1338:
1333:
1325:
1322:
1317:
1314:
1265:
1262:
1245:
1242:
1236:
1234:
1231:
1225:
1218:interferometric
1206:
1198:light signature
1190:
1187:
1176:
1163:of a candidate
1161:radial velocity
1145:
1125:George Gatewood
1111:
1108:
1102:
1098:
1096:
1093:
1087:
1047:
1042:
1000:is about 3,220
994:
991:
985:
982:
947:
945:
933:
926:
912:radial velocity
873:
853:
841:
838:
835:
709:
708:
707:
706:
705:
699:
698:
697:
696:
692:
640:
610:
583:
536:
534:
514:
512:
499:
496:
487:
477:
474:
467:
455:
452:
443:
441:
428:
425:
416:
414:
413:
411:
381:
364:
321:
292:
290:
285:
280:Radial velocity
106:
89:
84:Right ascension
82:
52:
46:
44:
33:Barnard's Star
28:
23:
22:
15:
12:
11:
5:
6659:
6657:
6649:
6648:
6643:
6638:
6633:
6628:
6623:
6618:
6613:
6608:
6603:
6598:
6593:
6588:
6583:
6573:
6572:
6568:
6567:
6555:
6543:
6531:
6508:
6507:
6497:
6494:
6493:
6490:
6489:
6487:
6486:
6480:
6478:
6468:
6467:
6464:
6463:
6461:
6460:
6454:
6452:
6442:
6441:
6438:
6437:
6435:
6434:
6428:
6426:
6422:
6421:
6419:
6418:
6413:
6408:
6403:
6397:
6395:
6388:
6382:
6381:
6378:
6377:
6375:
6374:
6369:
6364:
6359:
6354:
6349:
6344:
6338:
6336:
6332:
6331:
6329:
6328:
6323:
6317:
6315:
6308:
6302:
6301:
6298:
6297:
6295:
6294:
6289:
6284:
6279:
6274:
6269:
6264:
6259:
6254:
6249:
6243:
6241:
6237:
6236:
6234:
6233:
6228:
6223:
6218:
6213:
6208:
6203:
6198:
6193:
6188:
6183:
6178:
6173:
6167:
6165:
6156:
6148:
6147:
6144:
6143:
6141:
6140:
6135:
6130:
6125:
6120:
6115:
6110:
6104:
6102:
6092:
6091:
6088:
6087:
6085:
6084:
6079:
6074:
6069:
6067:WISE 1800+0134
6064:
6059:
6054:
6049:
6044:
6039:
6034:
6029:
6024:
6019:
6014:
6009:
6004:
5999:
5994:
5989:
5984:
5979:
5974:
5969:
5964:
5959:
5954:
5949:
5944:
5939:
5934:
5932:CFHTWIR-Oph 98
5929:
5924:
5918:
5916:
5912:
5911:
5909:
5908:
5903:
5898:
5893:
5888:
5883:
5878:
5873:
5868:
5863:
5858:
5853:
5848:
5843:
5838:
5833:
5828:
5823:
5821:148427 (Timir)
5818:
5812:
5810:
5804:
5803:
5801:
5800:
5795:
5790:
5785:
5780:
5775:
5770:
5765:
5760:
5755:
5750:
5745:
5740:
5735:
5730:
5725:
5720:
5715:
5710:
5705:
5700:
5695:
5690:
5685:
5680:
5675:
5670:
5665:
5660:
5655:
5650:
5645:
5640:
5635:
5630:
5625:
5620:
5615:
5610:
5605:
5600:
5595:
5590:
5585:
5580:
5575:
5570:
5565:
5560:
5555:
5550:
5545:
5540:
5535:
5530:
5525:
5520:
5515:
5510:
5505:
5500:
5495:
5490:
5485:
5480:
5475:
5470:
5465:
5460:
5455:
5450:
5445:
5440:
5435:
5430:
5425:
5420:
5415:
5410:
5405:
5400:
5395:
5390:
5385:
5380:
5375:
5370:
5365:
5360:
5355:
5350:
5345:
5340:
5334:
5332:
5326:
5325:
5323:
5322:
5317:
5312:
5307:
5302:
5297:
5292:
5287:
5282:
5277:
5272:
5267:
5262:
5257:
5252:
5247:
5242:
5237:
5232:
5227:
5222:
5217:
5212:
5207:
5202:
5197:
5192:
5187:
5182:
5177:
5172:
5167:
5162:
5157:
5152:
5147:
5142:
5137:
5132:
5127:
5122:
5117:
5112:
5107:
5102:
5097:
5092:
5087:
5082:
5077:
5072:
5067:
5062:
5057:
5052:
5047:
5042:
5037:
5032:
5027:
5022:
5017:
5012:
5007:
5002:
4996:
4994:
4988:
4987:
4985:
4984:
4977:
4972:
4967:
4962:
4957:
4952:
4947:
4942:
4937:
4932:
4927:
4922:
4917:
4912:
4907:
4902:
4893:
4888:
4883:
4878:
4873:
4868:
4863:
4858:
4853:
4848:
4843:
4838:
4833:
4828:
4823:
4818:
4813:
4808:
4803:
4798:
4793:
4787:
4785:
4779:
4778:
4776:
4775:
4770:
4765:
4760:
4755:
4750:
4745:
4740:
4735:
4730:
4725:
4720:
4715:
4710:
4705:
4700:
4695:
4690:
4682:
4677:
4672:
4667:
4662:
4660:α (Rasalhague)
4656:
4654:
4645:
4639:
4638:
4636:
4635:
4630:
4625:
4619:
4616:
4615:
4610:
4608:
4607:
4600:
4593:
4585:
4576:
4575:
4572:
4571:
4568:
4567:
4565:
4564:
4557:WISE 0855−0714
4553:
4551:
4544:
4529:
4528:
4525:
4524:
4521:
4520:
4518:
4517:
4514:
4503:
4501:
4492:
4482:
4481:
4478:
4477:
4474:
4473:
4471:
4470:
4460:
4457:
4447:
4444:
4434:
4431:
4421:
4414:Barnard's Star
4410:
4408:
4398:
4397:
4395:
4394:
4376:
4369:
4366:
4365:
4364:
4351:
4340:
4333:
4331:
4325:
4324:
4322:
4321:
4318:
4307:
4305:
4296:
4284:
4283:
4280:
4279:
4276:
4275:
4272:
4266:
4250:
4249:
4240:
4238:
4237:
4230:
4223:
4215:
4206:
4205:
4192:
4182:
4172:
4159:
4157:. Sol Station.
4149:
4148:External links
4146:
4143:
4142:
4099:
4065:
4017:
3984:
3924:
3911:10.1086/499497
3866:
3855:on 13 May 2008
3836:
3809:
3756:
3730:
3687:
3674:10.1086/300975
3628:
3615:10.1086/379137
3573:
3547:
3500:
3474:
3449:
3412:
3377:
3346:
3340:10.1086/111436
3325:(6): 421–425.
3305:
3299:10.1086/111480
3262:
3257:10.1086/110852
3243:(8): 757–759.
3227:
3221:10.1086/110799
3184:
3179:10.1086/109001
3147:
3107:
3083:
3016:
2985:
2956:
2927:
2890:(3): 220–222.
2872:
2814:
2784:
2771:10.1086/300420
2727:
2711:"Naming Stars"
2702:
2672:
2602:
2492:
2472:10.1086/499497
2428:
2423:10.1086/104156
2397:Barnard, E. E.
2388:
2354:
2328:
2321:
2303:
2276:
2255:
2225:
2188:
2153:
2090:
2084:10.1086/383289
2042:
1972:
1945:
1912:
1899:10.1086/118302
1875:(2): 806–822.
1852:
1790:
1708:
1707:
1705:
1702:
1699:
1698:
1680:
1677:
1674:
1671:
1668:
1665:
1662:
1659:
1654:
1650:
1646:
1643:
1640:
1637:
1634:
1631:
1628:
1625:
1622:
1621:
1600:
1582:
1581:
1579:
1576:
1575:
1574:
1568:
1559:
1551:
1548:
1532:Robert Freitas
1521:speed of light
1509:nuclear fusion
1494:Main article:
1491:
1488:
1454:
1451:
1435:Alpha Centauri
1409:
1406:
1397:stellar flares
1392:
1389:
1337:
1334:
1332:
1331:Stellar flares
1329:
1323:
1320:
1315:
1312:
1263:
1260:
1248:habitable zone
1243:
1240:
1232:
1229:
1220:work with the
1205:
1202:
1194:habitable zone
1188:
1185:
1144:
1141:
1109:
1106:
1094:
1091:
1046:
1043:
1041:
1038:
992:
989:
983:
980:
934:−110 km/s
872:
869:
865:Barnard's Star
852:
849:
836:
833:
781:, an American
748:Alpha Centauri
716:Barnard's Star
711:
710:
700:
694:
693:
686:
685:
679:
678:
677:
676:
673:
672:
667:
661:
660:
655:
647:
646:
642:
641:
638:Velox Barnardi
580:V2500 Ophiuchi
574:
571:
570:
564:
563:
560:
559:
553:
545:
544:
532:
524:
523:
510:
502:
501:
497:
494:
490:
485:
480:
479:
475:
472:
464:
458:
457:
453:
450:
439:
431:
430:
426:
423:
409:
401:
400:
397:
396:
392:
391:
388:
387:
384:
379:
371:
370:
358:
350:
349:
343:
334:
333:
308:
299:
298:
288:
283:
275:
274:
271:
270:
264:
263:
258:
252:
251:
248:
241:
240:
237:
230:
229:
226:
219:
218:
215:
208:
207:
204:
197:
196:
193:
186:
185:
182:
175:
174:
171:
164:
163:
160:
153:
152:
149:
142:
141:
138:
131:
130:
127:
121:
120:
116:
115:
112:
103:
102:
99:
93:
92:
90:17 57 48.49847
87:
79:
78:
73:
67:
66:
48:
47:
38:
26:
24:
14:
13:
10:
9:
6:
4:
3:
2:
6658:
6647:
6644:
6642:
6639:
6637:
6634:
6632:
6629:
6627:
6624:
6622:
6619:
6617:
6614:
6612:
6609:
6607:
6604:
6602:
6599:
6597:
6594:
6592:
6589:
6587:
6584:
6582:
6581:2MASS objects
6579:
6578:
6576:
6566:
6556:
6554:
6544:
6542:
6537:
6532:
6530:
6520:
6516:
6505:
6495:
6485:
6482:
6481:
6479:
6477:
6473:
6469:
6459:
6456:
6455:
6453:
6451:
6447:
6443:
6433:
6430:
6429:
6427:
6423:
6417:
6414:
6412:
6409:
6407:
6404:
6402:
6399:
6398:
6396:
6392:
6389:
6387:
6383:
6373:
6370:
6368:
6365:
6363:
6360:
6358:
6355:
6353:
6350:
6348:
6345:
6343:
6340:
6339:
6337:
6333:
6327:
6324:
6322:
6319:
6318:
6316:
6312:
6309:
6307:
6303:
6293:
6290:
6288:
6285:
6283:
6280:
6278:
6275:
6273:
6270:
6268:
6265:
6263:
6260:
6258:
6255:
6253:
6250:
6248:
6245:
6244:
6242:
6238:
6232:
6229:
6227:
6224:
6222:
6219:
6217:
6214:
6212:
6209:
6207:
6204:
6202:
6199:
6197:
6194:
6192:
6189:
6187:
6184:
6182:
6179:
6177:
6174:
6172:
6169:
6168:
6166:
6164:
6160:
6157:
6155:
6149:
6139:
6136:
6134:
6131:
6129:
6126:
6124:
6121:
6119:
6116:
6114:
6111:
6109:
6106:
6105:
6103:
6101:
6097:
6093:
6083:
6082:XTE J1739-285
6080:
6078:
6075:
6073:
6070:
6068:
6065:
6063:
6060:
6058:
6055:
6053:
6050:
6048:
6045:
6043:
6040:
6038:
6035:
6033:
6030:
6028:
6025:
6023:
6020:
6018:
6015:
6013:
6010:
6008:
6005:
6003:
6000:
5998:
5995:
5993:
5990:
5988:
5985:
5983:
5980:
5978:
5975:
5973:
5970:
5968:
5965:
5963:
5960:
5958:
5955:
5953:
5950:
5948:
5945:
5943:
5940:
5938:
5935:
5933:
5930:
5928:
5925:
5923:
5920:
5919:
5917:
5913:
5907:
5904:
5902:
5899:
5897:
5894:
5892:
5889:
5887:
5884:
5882:
5879:
5877:
5874:
5872:
5869:
5867:
5864:
5862:
5859:
5857:
5854:
5852:
5849:
5847:
5844:
5842:
5839:
5837:
5834:
5832:
5829:
5827:
5824:
5822:
5819:
5817:
5814:
5813:
5811:
5809:
5805:
5799:
5796:
5794:
5791:
5789:
5786:
5784:
5781:
5779:
5776:
5774:
5771:
5769:
5766:
5764:
5761:
5759:
5756:
5754:
5751:
5749:
5746:
5744:
5741:
5739:
5736:
5734:
5731:
5729:
5726:
5724:
5721:
5719:
5716:
5714:
5711:
5709:
5706:
5704:
5701:
5699:
5696:
5694:
5691:
5689:
5686:
5684:
5681:
5679:
5676:
5674:
5671:
5669:
5666:
5664:
5661:
5659:
5656:
5654:
5651:
5649:
5646:
5644:
5641:
5639:
5636:
5634:
5631:
5629:
5626:
5624:
5621:
5619:
5616:
5614:
5611:
5609:
5606:
5604:
5601:
5599:
5596:
5594:
5591:
5589:
5586:
5584:
5581:
5579:
5576:
5574:
5571:
5569:
5566:
5564:
5561:
5559:
5556:
5554:
5551:
5549:
5546:
5544:
5541:
5539:
5536:
5534:
5531:
5529:
5526:
5524:
5521:
5519:
5516:
5514:
5511:
5509:
5506:
5504:
5501:
5499:
5496:
5494:
5491:
5489:
5486:
5484:
5481:
5479:
5476:
5474:
5471:
5469:
5466:
5464:
5461:
5459:
5456:
5454:
5451:
5449:
5446:
5444:
5441:
5439:
5436:
5434:
5431:
5429:
5426:
5424:
5421:
5419:
5416:
5414:
5411:
5409:
5406:
5404:
5401:
5399:
5396:
5394:
5391:
5389:
5386:
5384:
5381:
5379:
5376:
5374:
5371:
5369:
5366:
5364:
5361:
5359:
5356:
5354:
5351:
5349:
5346:
5344:
5341:
5339:
5336:
5335:
5333:
5331:
5327:
5321:
5318:
5316:
5313:
5311:
5308:
5306:
5303:
5301:
5298:
5296:
5293:
5291:
5288:
5286:
5283:
5281:
5278:
5276:
5273:
5271:
5268:
5266:
5263:
5261:
5258:
5256:
5253:
5251:
5248:
5246:
5243:
5241:
5238:
5236:
5233:
5231:
5228:
5226:
5223:
5221:
5218:
5216:
5213:
5211:
5208:
5206:
5203:
5201:
5198:
5196:
5193:
5191:
5188:
5186:
5183:
5181:
5178:
5176:
5173:
5171:
5168:
5166:
5163:
5161:
5158:
5156:
5153:
5151:
5148:
5146:
5143:
5141:
5138:
5136:
5133:
5131:
5128:
5126:
5123:
5121:
5118:
5116:
5113:
5111:
5108:
5106:
5103:
5101:
5098:
5096:
5093:
5091:
5088:
5086:
5083:
5081:
5078:
5076:
5073:
5071:
5068:
5066:
5063:
5061:
5058:
5056:
5053:
5051:
5048:
5046:
5043:
5041:
5038:
5036:
5033:
5031:
5028:
5026:
5023:
5021:
5018:
5016:
5013:
5011:
5008:
5006:
5003:
5001:
4998:
4997:
4995:
4993:
4989:
4983:
4982:
4978:
4976:
4973:
4971:
4968:
4966:
4963:
4961:
4958:
4956:
4953:
4951:
4948:
4946:
4943:
4941:
4938:
4936:
4933:
4931:
4928:
4926:
4923:
4921:
4918:
4916:
4913:
4911:
4908:
4906:
4903:
4901:
4899:
4894:
4892:
4889:
4887:
4884:
4882:
4879:
4877:
4874:
4872:
4869:
4867:
4864:
4862:
4859:
4857:
4854:
4852:
4849:
4847:
4844:
4842:
4839:
4837:
4834:
4832:
4829:
4827:
4824:
4822:
4819:
4817:
4814:
4812:
4809:
4807:
4804:
4802:
4799:
4797:
4794:
4792:
4789:
4788:
4786:
4784:
4780:
4774:
4771:
4769:
4766:
4764:
4761:
4759:
4756:
4754:
4751:
4749:
4746:
4744:
4741:
4739:
4736:
4734:
4731:
4729:
4726:
4724:
4721:
4719:
4716:
4714:
4711:
4709:
4706:
4704:
4701:
4699:
4696:
4694:
4691:
4689:
4688:
4683:
4681:
4678:
4676:
4675:δ (Yed Prior)
4673:
4671:
4668:
4666:
4663:
4661:
4658:
4657:
4655:
4653:
4649:
4646:
4644:
4640:
4634:
4631:
4629:
4626:
4624:
4621:
4620:
4617:
4613:
4606:
4601:
4599:
4594:
4592:
4587:
4586:
4583:
4558:
4555:
4554:
4552:
4548:
4545:
4543:
4542:rogue planets
4538:
4534:
4530:
4515:
4508:
4505:
4504:
4502:
4500:
4496:
4493:
4491:
4487:
4483:
4464:
4461:
4458:
4451:
4448:
4445:
4438:
4437:Lalande 21185
4435:
4432:
4425:
4422:
4415:
4412:
4411:
4409:
4407:
4399:
4393:
4389:
4385:
4381:
4377:
4374:
4370:
4367:
4358:
4355:
4354:
4352:
4349:
4341:
4338:
4335:
4334:
4332:
4330:
4326:
4319:
4312:
4309:
4308:
4306:
4304:
4300:
4297:
4295:
4292:Main-sequence
4289:
4285:
4270:
4267:
4264:
4255:
4251:
4247:
4244:
4236:
4231:
4229:
4224:
4222:
4217:
4216:
4213:
4209:
4202:
4198:
4193:
4188:
4183:
4178:
4173:
4169:
4165:
4160:
4156:
4152:
4151:
4147:
4131:
4127:
4123:
4119:
4118:
4113:
4106:
4104:
4100:
4087:
4083:
4079:
4072:
4070:
4066:
4053:
4049:
4045:
4041:
4037:
4036:
4031:
4024:
4022:
4018:
4005:
4001:
4000:
3995:
3988:
3985:
3980:
3976:
3971:
3966:
3962:
3958:
3953:
3948:
3944:
3940:
3936:
3928:
3925:
3920:
3916:
3912:
3908:
3904:
3900:
3895:
3890:
3886:
3882:
3881:
3873:
3871:
3867:
3854:
3850:
3846:
3840:
3837:
3824:
3820:
3813:
3810:
3805:
3801:
3797:
3793:
3789:
3785:
3780:
3775:
3771:
3767:
3760:
3757:
3745:
3741:
3734:
3731:
3726:
3722:
3718:
3714:
3710:
3706:
3702:
3698:
3691:
3688:
3683:
3679:
3675:
3671:
3667:
3663:
3658:
3653:
3649:
3645:
3644:
3635:
3633:
3629:
3624:
3620:
3616:
3612:
3608:
3604:
3599:
3594:
3590:
3586:
3585:
3577:
3574:
3562:
3558:
3551:
3548:
3542:
3537:
3533:
3529:
3524:
3519:
3515:
3511:
3504:
3501:
3488:
3484:
3478:
3475:
3463:
3459:
3453:
3450:
3434:
3430:
3423:
3416:
3413:
3408:
3404:
3400:
3396:
3392:
3388:
3381:
3378:
3364:
3360:
3353:
3351:
3347:
3341:
3336:
3332:
3328:
3324:
3320:
3316:
3309:
3306:
3300:
3295:
3291:
3287:
3283:
3279:
3278:
3273:
3266:
3263:
3258:
3254:
3250:
3246:
3242:
3238:
3231:
3228:
3222:
3217:
3213:
3209:
3205:
3201:
3200:
3195:
3188:
3185:
3180:
3176:
3172:
3168:
3164:
3160:
3159:
3151:
3148:
3143:
3137:
3121:
3117:
3111:
3108:
3103:
3099:
3098:
3093:
3087:
3084:
3079:
3075:
3071:
3067:
3062:
3057:
3053:
3049:
3044:
3039:
3035:
3031:
3027:
3020:
3017:
3004:
3000:
2994:
2992:
2990:
2986:
2981:
2977:
2973:
2969:
2968:
2960:
2957:
2952:
2948:
2944:
2940:
2939:
2931:
2928:
2923:
2919:
2915:
2911:
2907:
2903:
2898:
2893:
2889:
2885:
2884:
2876:
2873:
2868:
2864:
2860:
2856:
2852:
2848:
2843:
2838:
2834:
2830:
2823:
2821:
2819:
2815:
2802:
2798:
2791:
2789:
2785:
2780:
2776:
2772:
2768:
2764:
2760:
2755:
2750:
2746:
2742:
2734:
2732:
2728:
2716:
2712:
2706:
2703:
2690:
2686:
2682:
2676:
2673:
2668:
2664:
2660:
2656:
2651:
2646:
2642:
2638:
2633:
2628:
2624:
2620:
2616:
2609:
2607:
2603:
2595:
2591:
2587:
2583:
2579:
2575:
2571:
2567:
2563:
2559:
2555:
2551:
2547:
2543:
2539:
2534:
2529:
2525:
2521:
2517:
2516:
2508:
2501:
2499:
2497:
2493:
2481:
2477:
2473:
2469:
2465:
2461:
2456:
2451:
2447:
2443:
2439:
2432:
2429:
2424:
2420:
2416:
2412:
2408:
2404:
2403:
2398:
2392:
2389:
2376:
2372:
2368:
2361:
2359:
2355:
2342:
2338:
2332:
2329:
2324:
2318:
2314:
2307:
2304:
2299:
2295:
2291:
2287:
2280:
2277:
2272:
2268:
2267:
2259:
2256:
2251:
2247:
2243:
2239:
2235:
2229:
2226:
2221:
2217:
2213:
2209:
2205:
2202:(in German).
2201:
2200:
2192:
2189:
2184:
2180:
2176:
2172:
2171:
2162:
2160:
2158:
2154:
2149:
2145:
2140:
2135:
2131:
2127:
2122:
2117:
2113:
2109:
2105:
2101:
2094:
2091:
2085:
2080:
2076:
2072:
2068:
2064:
2063:
2058:
2051:
2049:
2047:
2043:
2038:
2034:
2029:
2024:
2020:
2016:
2011:
2006:
2002:
1998:
1994:
1987:
1985:
1983:
1981:
1979:
1977:
1973:
1968:
1964:
1960:
1956:
1949:
1946:
1941:
1937:
1933:
1929:
1921:
1919:
1917:
1913:
1908:
1904:
1900:
1896:
1892:
1888:
1883:
1878:
1874:
1870:
1869:
1861:
1859:
1857:
1853:
1847:
1842:
1838:
1834:
1830:
1826:
1825:
1820:
1813:
1811:
1809:
1807:
1805:
1803:
1801:
1799:
1797:
1795:
1791:
1787:
1783:
1777:
1773:
1768:
1763:
1759:
1755:
1750:
1745:
1741:
1737:
1733:
1731:
1722:
1720:
1718:
1716:
1714:
1710:
1703:
1678:
1675:
1669:
1666:
1660:
1657:
1652:
1648:
1638:
1635:
1632:
1629:
1626:
1623:
1610:
1604:
1601:
1597:
1593:
1587:
1584:
1577:
1572:
1569:
1563:
1560:
1557:
1554:
1553:
1549:
1547:
1545:
1541:
1537:
1533:
1528:
1526:
1522:
1518:
1514:
1510:
1505:
1503:
1497:
1489:
1484:
1480:
1476:
1472:
1468:
1464:
1459:
1452:
1450:
1448:
1444:
1436:
1432:
1428:
1419:
1414:
1407:
1405:
1402:
1401:stellar flare
1398:
1390:
1388:
1386:
1385:stellar winds
1382:
1378:
1374:
1369:
1366:
1363:
1359:
1354:
1347:
1343:
1342:stellar flare
1335:
1330:
1328:
1318:
1307:
1305:
1301:
1297:
1293:
1289:
1284:
1281:
1277:
1273:
1268:
1266:
1257:
1253:
1249:
1223:
1219:
1214:
1212:
1203:
1201:
1199:
1195:
1191:
1182:
1174:
1169:
1166:
1162:
1154:
1149:
1140:
1138:
1134:
1129:
1126:
1117:
1113:
1084:
1080:
1076:
1072:
1068:
1064:
1060:
1059:proper motion
1056:
1052:
1044:
1039:
1037:
1034:
1030:
1026:
1022:
1018:
1013:
1011:
1007:
1003:
999:
995:
986:
977:
972:
969:
962:
961:nearest stars
957:
953:
950:0.2 km/s
943:
939:
930:
919:
915:
913:
909:
905:
901:
900:stellar flare
897:
893:
888:
886:
882:
878:
877:spectral type
870:
868:
866:
862:
858:
855:In 2016, the
850:
848:
845:
840:and orbit at
839:
830:
826:
822:
817:
815:
814:stellar flare
811:
807:
803:
798:
796:
792:
788:
787:proper motion
784:
780:
775:
773:
769:
765:
761:
757:
753:
749:
745:
741:
737:
733:
729:
725:
724:constellation
721:
717:
704:
683:
674:
671:
668:
666:
663:
662:
659:
656:
654:
653:
649:
648:
643:
639:
635:
631:
627:
623:
619:
613:
609: 15309,
608:
604:
600:
597: 87937,
596:
592:
586:
581:
577:
572:
569:
565:
561:
558:
554:
552:
551:
547:
546:
542:
533:
531:
530:
526:
525:
522:
511:
509:
508:
504:
503:
500:
491:
489:
482:
481:
478:
470:0.00006
465:
463:
460:
459:
456:
440:
438:
437:
433:
432:
429:
410:
408:
407:
403:
402:
398:
393:
389:
385:
383:
377:
373:
372:
368:
363:
359:
357:
356:
352:
351:
348:
344:
342:
340:
336:
335:
332:
328:
320:
316:
309:
307:
305:
304:Proper motion
301:
300:
289:
287:
281:
277:
276:
272:
269:
265:
262:
259:
257:
254:
253:
249:
247:
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133:
132:
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126:
123:
122:
117:
113:
109:
105:
104:
100:
98:
95:
94:
88:
85:
81:
80:
77:
74:
72:
71:Constellation
69:
68:
65:
62:
58:
55:
49:
42:
36:
30:
19:
6372:Snake Nebula
6133:ν Ophiuchi b
6047:PSR B1929+10
5982:GRS 1739-278
5304:
4979:
4897:
4686:
4670:γ (Muliphen)
4665:β (Cebalrai)
4490:Brown dwarfs
4413:
4405:(red dwarfs)
4348:Solar System
4207:
4167:
4133:. Retrieved
4121:
4115:
4090:. Retrieved
4081:
4056:. Retrieved
4052:the original
4039:
4033:
4008:. Retrieved
3997:
3987:
3942:
3938:
3927:
3884:
3878:
3859:12 September
3857:. Retrieved
3853:the original
3839:
3827:. Retrieved
3823:the original
3812:
3769:
3765:
3759:
3747:. Retrieved
3743:
3733:
3703:(1): 91–98.
3700:
3696:
3690:
3647:
3641:
3588:
3582:
3576:
3564:. Retrieved
3560:
3550:
3513:
3503:
3491:. Retrieved
3477:
3465:. Retrieved
3461:
3452:
3440:. Retrieved
3433:the original
3428:
3415:
3390:
3386:
3380:
3367:. Retrieved
3322:
3318:
3308:
3281:
3275:
3265:
3240:
3236:
3230:
3203:
3197:
3187:
3162:
3156:
3150:
3124:. Retrieved
3119:
3110:
3095:
3086:
3033:
3029:
3019:
3007:. Retrieved
2971:
2965:
2959:
2942:
2936:
2930:
2887:
2881:
2875:
2832:
2828:
2805:. Retrieved
2800:
2744:
2740:
2718:. Retrieved
2705:
2693:. Retrieved
2675:
2622:
2618:
2519:
2513:
2483:. Retrieved
2445:
2441:
2431:
2406:
2400:
2391:
2379:. Retrieved
2375:the original
2370:
2345:. Retrieved
2341:the original
2331:
2312:
2306:
2289:
2285:
2279:
2273:: 170. 1969.
2270:
2264:
2258:
2244:(377): 207.
2241:
2237:
2228:
2203:
2197:
2191:
2174:
2168:
2111:
2107:
2093:
2066:
2060:
2000:
1996:
1958:
1954:
1948:
1931:
1927:
1872:
1866:
1828:
1822:
1739:
1735:
1729:
1603:
1595:
1591:
1586:
1529:
1506:
1499:
1423:
1394:
1370:
1355:
1339:
1308:
1285:
1269:
1255:
1251:
1215:
1207:
1183:of 3.2
1181:minimum mass
1170:
1158:
1137:double stars
1133:Wulff Heintz
1130:
1122:
1048:
1014:
976:solar masses
973:
966:
931:
924:
889:
874:
864:
859:organized a
854:
818:
799:
776:
756:stellar mass
722:star in the
715:
714:
664:
650:
601: 1385,
548:
527:
505:
492:0.0004
483:
461:
434:
404:
374:
353:
337:
302:
278:
29:
6606:Flare stars
6565:Outer space
6553:Spaceflight
6357:Pipe Nebula
6287:Messier 107
6252:Melotte 186
6042:PG 1627-017
6032:MXB 1659-29
4124:: 251–264.
3566:19 November
3493:14 November
3467:15 November
3284:(10): 769.
2974:: 523–531.
2720:16 December
2526:: 365–368.
2266:Spaceflight
1831:(4): 1949.
1479:declination
1475:hours angle
1408:Environment
1302:'s similar
1165:super-Earth
1153:super-Earth
1017:metallicity
871:Description
829:super-Earth
764:unaided eye
734:(1.83
732:light-years
718:is a small
593: 699,
507:Temperature
261:BY Draconis
246:color index
235:color index
224:color index
213:color index
97:Declination
6575:Categories
6342:Dark Horse
6282:Messier 62
6277:Messier 19
6272:Messier 14
6267:Messier 12
6262:Messier 10
6100:Exoplanets
6037:Oph-IRS 48
6002:Hen 3-1341
5997:H 1705-250
5967:Gliese 673
5957:Elias 2-27
4713:λ (Marfik)
4513:0.0011 ly)
4469:0.0009 ly)
4443:0.0007 ly)
4430:0.0013 ly)
4420:0.0004 ly)
4363:0.0022 ly)
4317:0.0054 ly)
4042:(2): 101.
3952:2009.01259
3945:(5): 237.
3887:(1): 227.
3829:26 January
3772:(2): 131.
3523:2207.13524
3393:(2): 141.
3206:(2): 238.
3165:(7): 515.
3126:26 January
3043:1810.13252
2747:(1): 429.
2632:2105.07005
2558:2299/21132
2533:1811.05955
2485:5 February
2121:2201.11288
2010:2106.07656
1961:: B/gcvs.
1749:2208.00211
1704:References
1609:extinction
1483:concentric
1365:convection
1340:In 1998 a
1075:micrometre
1055:astrometry
1029:halo stars
904:flare star
825:gas giants
806:astrometry
791:arcseconds
783:astronomer
605: 57,
555:≈ 10
297: km/s
268:Astrometry
203: (K)
192: (H)
181: (J)
170: (I)
159: (R)
148: (B)
137: (U)
6641:Ophiuchus
6529:Astronomy
6292:Palomar 6
6257:Messier 9
6062:VVV BD001
6022:LS IV-1 2
5927:BD-9 4395
4783:Flamsteed
4693:η (Sabik)
4563:0.041 ly)
4507:Luhman 16
4456:0.012 ly)
4135:1 October
4092:10 August
4058:15 August
3979:225282584
3779:1208.2273
3725:120060893
3369:10 August
3078:204200655
3070:0004-6361
3009:10 August
2922:118374161
2897:1003.2160
2807:10 August
2667:234741985
2659:0004-6256
2590:256769911
2574:716177853
2566:0028-0836
2206:(4): 77.
2148:246294876
2114:(1): 11.
2037:235435757
2003:(1): 23.
1776:244398875
1667:−
1658:
1639:⋅
1556:Kepler-42
1513:deuterium
1443:Monoceros
1439:5 57 48.5
1310:0.7
1173:snow line
1033:disk star
938:blueshift
892:Milky Way
881:telescope
842:0.4
728:Ophiuchus
720:red dwarf
703:Ophiuchus
630:Vyssotsky
624:140-024,
620:4098.00,
587:+04°3561a
110: (V)
76:Ophiuchus
6504:Category
6386:Galaxies
6154:clusters
6113:CoRoT-6b
6077:Wolf 635
5962:Gaia BH1
5947:CoRoT-26
5942:CoRoT-25
4992:Variable
4463:Ross 154
4424:Wolf 359
4382:?; Bc?;
4201:BBC News
4086:Archived
4010:25 April
4004:Archived
3919:17926580
3804:29053334
3749:11 April
3682:18099356
3623:17353771
3363:Archived
3136:cite web
3036:: A180.
3003:Archived
2867:16738100
2779:15880053
2689:Archived
2594:Archived
2582:30429552
2522:(7731).
2480:17926580
1907:16863021
1550:See also
1517:helium-3
1427:Ross 154
1211:M dwarfs
984:☉
887:is 9.5.
789:as 10.3
768:infrared
539:15
529:Rotation
498:☉
476:☉
454:☉
427:☉
378: (M
355:Distance
339:Parallax
6515:Portals
6306:Nebulae
6247:IC 4665
6052:TOI-677
5972:GJ 1207
5952:DoAr 21
5937:CoRoT-6
4896:45 (d,
4509:(6.5029
4465:(9.7063
4439:(8.3044
4426:(7.8558
4416:(5.9629
4359:(4.3441
4313:(8.7094
4261:member
4259:Primary
4126:Bibcode
4044:Bibcode
3957:Bibcode
3899:Bibcode
3784:Bibcode
3705:Bibcode
3662:Bibcode
3603:Bibcode
3528:Bibcode
3462:eso.org
3395:Bibcode
3327:Bibcode
3286:Bibcode
3245:Bibcode
3208:Bibcode
3167:Bibcode
3048:Bibcode
2976:Bibcode
2947:Bibcode
2945:: 1–9.
2902:Bibcode
2847:Bibcode
2759:Bibcode
2637:Bibcode
2538:Bibcode
2460:Bibcode
2411:Bibcode
2381:12 July
2294:Bibcode
2246:Bibcode
2208:Bibcode
2179:Bibcode
2177:: 442.
2126:Bibcode
2071:Bibcode
2015:Bibcode
1963:Bibcode
1936:Bibcode
1887:Bibcode
1833:Bibcode
1754:Bibcode
1544:Jupiter
1431:parsecs
1063:Jupiter
466:0.00340
417:−0.0035
415:+0.0036
395:Details
291:−110.47
151:11.240
140:12.497
64:J2000.0
61:Equinox
57:J2000.0
6432:NeVe 1
5992:GX 9+9
5987:GX 1+4
5922:AS 239
5906:171028
5901:170469
5896:167162
5891:164509
5886:160346
5881:160042
5876:157172
5871:156992
5866:154088
5856:150493
5851:150433
5846:150381
5841:150052
5836:149382
5826:148531
5816:148390
4981:24 Sco
4955:70 (p)
4920:53 (f)
4910:51 (c)
4891:44 (b)
4559:(7.430
4550:Y-type
4499:L-type
4452:(8.724
4402:M-type
4339:(0 ly)
4329:G-type
4303:A-type
3977:
3917:
3802:
3723:
3680:
3621:
3442:2 June
3097:VizieR
3076:
3068:
2920:
2865:
2777:
2695:22 May
2665:
2657:
2588:
2580:
2572:
2564:
2515:Nature
2478:
2319:
2146:
2035:
1905:
1786:VizieR
1774:
1742:: A1.
1447:Pollux
1362:plasma
1350:
1304:Darwin
1239:
1228:
1177:
1105:
1099:
1090:
1021:helium
1002:kelvin
927:
883:; its
851:Naming
754:. Its
665:ARICNS
652:SIMBAD
519:
448:
436:Radius
421:
412:0.1610
250:1.557
239:1.213
228:1.713
217:1.257
206:4.524
173:6.741
162:8.298
129:M4.0V
114:9.511
6541:Stars
6425:Other
6335:Other
6240:Other
6017:K2-32
5915:Other
5320:V2542
5315:V2540
5310:V2502
5300:V2487
5295:V2400
5290:V2393
5285:V2388
5280:V2368
5275:V2324
5270:V2307
5265:V2306
5260:V2301
5255:V2295
5250:V2293
5245:V2292
5240:V2291
5235:V2247
5230:V2214
5225:V2213
5220:V2129
5215:V2126
5210:V2118
5205:V2114
5200:V2113
5195:V2112
5190:V2105
5185:V2076
5180:V2052
5175:V2051
5170:V1054
5165:V1010
4898:θ Tel
4687:(Han)
4652:Bayer
4643:Stars
4294:stars
3975:S2CID
3947:arXiv
3915:S2CID
3889:arXiv
3800:S2CID
3774:arXiv
3721:S2CID
3678:S2CID
3652:arXiv
3619:S2CID
3593:arXiv
3518:arXiv
3436:(PDF)
3425:(PDF)
3074:S2CID
3038:arXiv
2918:S2CID
2892:arXiv
2863:S2CID
2837:arXiv
2775:S2CID
2749:arXiv
2663:S2CID
2627:arXiv
2597:(PDF)
2586:S2CID
2528:arXiv
2510:(PDF)
2476:S2CID
2450:arXiv
2371:Stars
2347:5 May
2292:: 1.
2144:S2CID
2116:arXiv
2039:. 40.
2033:S2CID
2005:arXiv
1903:S2CID
1877:arXiv
1780:
1772:S2CID
1744:arXiv
1661:1.834
1578:Notes
1463:radar
1373:X-ray
946:142.6
772:light
634:Latin
632:799,
626:Karmn
612:2MASS
513:3,223
446:0.001
442:0.187
386:13.21
323:Dec.:
195:4.83
184:5.24
54:Epoch
6416:6570
6411:6509
6406:6384
6401:6240
6326:6572
6321:6309
6231:6633
6226:6426
6221:6401
6216:6366
6211:6356
6206:6355
6201:6342
6196:6325
6191:6316
6186:6304
6181:6293
6176:6287
6171:6284
6152:Star
5798:7010
5793:6987
5788:6985
5783:6976
5778:6925
5773:6902
5768:6883
5763:6857
5758:6851
5753:6800
5748:6797
5743:6784
5738:6719
5733:6706
5728:6696
5723:6690
5718:6689
5713:6686
5708:6670
5703:6667
5698:6659
5693:6650
5688:6639
5683:6633
5678:6601
5673:6593
5668:6590
5663:6578
5658:6577
5653:6575
5648:6534
5643:6532
5638:6524
5633:6521
5628:6520
5623:6516
5618:6512
5613:6507
5608:6504
5603:6497
5598:6494
5593:6490
5588:6489
5583:6476
5578:6474
5573:6473
5568:6472
5563:6465
5558:6441
5553:6439
5548:6435
5543:6433
5538:6428
5533:6413
5528:6404
5523:6390
5518:6387
5513:6375
5508:6372
5503:6367
5498:6365
5493:6361
5488:6359
5483:6358
5478:6354
5473:6353
5468:6350
5463:6340
5458:6329
5453:6308
5448:6302
5443:6296
5438:6294
5433:6284
5428:6269
5423:6248
5418:6235
5413:6202
5408:6201
5403:6193
5398:6190
5393:6189
5388:6179
5383:6144
5378:6140
5373:6137
5368:6136
5363:6124
5358:6096
5353:6067
5348:6041
5343:5990
5338:5989
5160:V986
5155:V849
5150:V841
5145:V839
5140:V716
5135:V567
5130:V566
5125:V508
5120:V502
5115:V453
5110:V451
5105:V445
5100:V442
5095:V438
5090:V426
5085:V380
4540:and
4344:rest
4263:type
4137:2008
4094:2006
4060:2006
4012:2014
3999:NASA
3861:2011
3831:2014
3751:2018
3568:2018
3495:2018
3469:2018
3444:2010
3371:2006
3142:link
3128:2014
3066:ISSN
3011:2006
2809:2006
2722:2017
2697:2016
2655:ISSN
2578:PMID
2570:OCLC
2562:ISSN
2487:2022
2383:2018
2349:2013
2317:ISBN
1932:2246
1730:Gaia
1679:1.15
1630:4.83
1594:sin
1515:and
1391:2019
1375:and
1336:1998
1292:NASA
1276:Keck
1274:and
1272:Lick
1254:sin
670:data
658:data
618:GCTP
406:Mass
295:0.13
244:R−I
233:V−R
222:B−V
211:U−B
6394:NGC
6314:NGC
6163:NGC
6123:26b
6118:25b
4390:?,
4346:of
4337:Sun
3965:doi
3943:160
3907:doi
3885:118
3792:doi
3770:764
3713:doi
3701:223
3670:doi
3648:118
3611:doi
3589:126
3536:doi
3403:doi
3335:doi
3294:doi
3253:doi
3216:doi
3175:doi
3056:doi
3034:620
2910:doi
2855:doi
2833:403
2767:doi
2745:116
2645:doi
2623:162
2554:hdl
2546:doi
2520:563
2468:doi
2446:118
2419:doi
2216:doi
2204:230
2134:doi
2112:927
2079:doi
2067:127
2023:doi
2001:918
1895:doi
1873:113
1841:doi
1829:403
1784:at
1762:doi
1740:674
1649:log
1473:in
1418:Sun
1300:ESA
1294:'s
1237:0.8
1103:0.8
1088:1.6
1069:at
896:Sun
744:Sun
726:of
607:LTT
603:LHS
599:LFT
595:HIP
557:Gyr
550:Age
535:145
347:mas
341:(π)
327:mas
315:mas
311:RA:
306:(μ)
6577::
5808:HD
5330:HR
5080:KK
5075:IX
5070:BF
5065:XX
5060:WZ
5055:UU
5050:TW
5045:TT
5040:SW
5035:ST
5030:RZ
5025:RV
5020:RS
4975:74
4970:73
4965:72
4960:71
4950:68
4945:67
4940:66
4935:61
4930:58
4925:54
4915:52
4905:50
4886:43
4881:41
4876:38
4871:37
4861:31
4856:30
4851:29
4846:28
4841:26
4836:24
4831:23
4826:21
4821:20
4816:19
4811:18
4806:16
4801:15
4796:14
4791:12
4685:ζ
4392:Cd
4388:Cc
4386:,
4384:Cb
4380:Ab
4166:.
4122:33
4120:.
4114:.
4102:^
4084:.
4080:.
4068:^
4038:.
4032:.
4020:^
4002:.
3996:.
3973:.
3963:.
3955:.
3941:.
3937:.
3913:.
3905:.
3897:.
3883:.
3869:^
3847:.
3798:.
3790:.
3782:.
3768:.
3742:.
3719:.
3711:.
3699:.
3676:.
3668:.
3660:.
3646:.
3631:^
3617:.
3609:.
3601:.
3587:.
3559:.
3534:.
3526:.
3512:.
3485:.
3460:.
3427:.
3401:.
3391:26
3389:.
3349:^
3333:.
3323:78
3321:.
3317:.
3292:.
3282:78
3280:.
3274:.
3251:.
3241:74
3239:.
3214:.
3204:74
3202:.
3196:.
3173:.
3163:68
3161:.
3138:}}
3134:{{
3118:.
3100:.
3094:.
3072:.
3064:.
3054:.
3046:.
3032:.
3028:.
2988:^
2972:47
2970:.
2943:35
2941:.
2916:.
2908:.
2900:.
2888:36
2886:.
2861:.
2853:.
2845:.
2831:.
2817:^
2799:.
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