The motion of Beta Pictoris b. The orbital plane is viewed side-on; the planet is not moving towards the star.
Discovery
Discovered by
Lagrange et al.
Discovery site
Very Large Telescope
Discovery date
November 18, 2008
Detection method
Direct imaging
Orbital characteristics[1]
Semi-major axis
10.018+0.082 −0.076 AU
Eccentricity
0.106+0.007 −0.006
Orbital period (sidereal)
23.593+0.248 −0.209 yr
Inclination
89.009°±0.012°
Longitude of ascending node
31.774°+0.008° −0.009°
Time of periastron
2448022.339+15.635 −24.710
Argument of periastron
21.835°+4.099° −4.044°
Semi-amplitude
78.791+15.672 −14.126 m/s
Star
Beta Pictoris
Physical characteristics
Mean radius
1.46±0.01[2][note 1]RJ
Mass
11.729+2.337 −2.135[1]MJ
Synodic rotation period
8.7±0.8 h[3]
Equatorial rotation velocity
19.9±1.0 km/s[3]
Temperature
1,724 K (1,451 °C; 2,644 °F) ±15 K (15 °C; 27 °F)[2][note 1]
Beta Pictoris b (abbreviated as β Pic b) is an exoplanet orbiting the young debris disk A-type main sequence star Beta Pictoris located approximately 63 light-years (19.4 parsecs, or 6×1014 km) away from Earth in the constellation of Pictor. It has a mass around 13 Jupiter masses and a radius around 46% larger than Jupiter's. It orbits at 9 AU from Beta Pictoris, which is about 3.5 times farther than the orbit of Beta Pictoris c.[4] It orbits close to the plane of the debris disk orbiting the star, with a low eccentricity and a period of 20–21 years.
^ abCite error: The named reference Feng2022 was invoked but never defined (see the help page).
^ abCite error: The named reference Chilcote2017 was invoked but never defined (see the help page).
^ abCite error: The named reference Landman2024 was invoked but never defined (see the help page).
^Lagrange, A.-M.; Meunier, Pascal Rubini; Keppler, Miriam; Galland, Franck; et al. (August 19, 2019). "Evidence for an additional planet in the β Pictoris system". Nature Astronomy. 3 (12): 1135–1142. Bibcode:2019NatAs...3.1135L. doi:10.1038/s41550-019-0857-1. S2CID 202126059. Retrieved August 20, 2019.
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BetaPictoris (abbreviated β Pictoris or β Pic) is the second brightest star in the constellation Pictor. It is located 63.4 light-years (19.4 pc) from...
BetaPictoris c (abbreviated as β Pic c) is the second exoplanet discovered orbiting the young star BetaPictoris, located approximately 63 light-years...
nanosatellite, designed to measure the transit of BetaPictorisb, an exoplanet which orbits the star BetaPictoris. PicSat was designed and built by a team of...
1086/337968. "Extrasolar Visions - BetaPictorisb". Archived from the original on 2010-11-17. Retrieved 2010-03-26. "BetaPictoris planet finally imaged?" (Press...
about 2,000 K or a radius of 2.55 ± 0.20 RJ for about 1950 K. Like BetaPictorisb, ROXs 42Bb's atmosphere is likely very cloudy and dusty. List of largest...
132E. doi:10.1002/andp.19053220607. English translation: Arons, A. B.; Peppard, M. B. (1965). "Einstein's proposal of the photon concept—a translation...
PSR B1257+12 b), which is about twice the mass of the Moon. The most massive exoplanet listed on the NASA Exoplanet Archive is HR 2562 b, about 30 times...
similar to other planetary-mass companions/exoplanets like betaPictorisb or 1RXS J160929.1−210524 b, its projected separation from the star is much larger...
1051/0004-6361/202345877. Wang; et al. (2016). "The Orbit and Transit Prospects for β Pictorisb Constrained with One Milliarcsecond Astrometry". The Astronomical Journal...
explanation was confirmed with the 2008 discovery of the exoplanet BetaPictorisb. Other exoplanet-hosting stars, including the first discovered by direct...
(2017-04-01). "1 to 2.4 micron Near-IR spectrum of the Giant Planet $\beta$ Pictorisb obtained with the Gemini Planet Imager". The Astronomical Journal....
Dillon, Daren (2017-03-28). "1–2.4μm Near-IR Spectrum of the Giant PlanetβPictorisb Obtained with the Gemini Planet Imager". The Astronomical Journal. 153...
Kiefer, Flavien (2019-08-19). "Evidence for an additional planet in the β Pictoris system". Nature Astronomy. 3 (12): 1135–1142. Bibcode:2019NatAs...3.1135L...
brightest star is Alpha Pictoris, a white main-sequence star around 97 light-years away from Earth. Pictor also hosts RR Pictoris, a cataclysmic variable...
Gaia spacecraft to Hipparcos data for the BetaPictoris system was able to measure the mass of BetaPictorisb, constraining it to 11±2 Jupiter masses....
The telescope's scientific discoveries include direct imaging of BetaPictorisb, the first extrasolar planet so imaged, tracking individual stars moving...
measure the mass of the exoplanet BetaPictorisb and is sometimes used to study other long-period exoplanets, such as HR 5183 b. Pierre Lacroute (Observatory...
estimated at between 250 K and 430 K (between −20 °C and 160 °C). BetaPictorisb: On June 10, for the first time astronomers have been able to directly...
disks, such as TW Hydrae or directly imaged exoplanets, such as BetaPictorisb or GU Psc b. A stellar stream is an association of stars orbiting a galaxy...
other than the Sun. The first exocomets were detected in 1987 around BetaPictoris, a very young A-type main-sequence star. There are now (as of February...
resulting from the presence of starspots. AF Leporis is a member of the BetaPictoris moving group, with an astronomically young age of about 24 million years...
close approach to the BetaPictoris system. The estimated separation of the two stars at this time was around 1.9 ly (0.58 pc) and Beta Columbae may have...
AB Pictoris (abbreviated AB Pic, also catalogued as HD 44627) is a K-type main-sequence star, located 163.5 light-years away in the southern constellation...
formed out of such a disk, Denebola and similar stars such as Vega and BetaPictoris may be candidate locations for extrasolar planets. Kinematic studies...
1088/0004-637X/703/2/1188, S2CID 17938884 Smith, B. A.; Terrile, R. J. (1984), "A circumstellar disk around BetaPictoris", Science, 226 (4681): 1421–1424, Bibcode:1984Sci...