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Super Jupiter orbiting Beta Pictoris
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
Beta_Pictoris_b
Second brightest star in the southern constellation of Pictor
Beta Pictoris (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
Beta_Pictoris
Super Jupiter exoplanet orbiting Beta Pictoris
Beta Pictoris c (abbreviated as β Pic c) is the second exoplanet discovered orbiting the young star Beta Pictoris, located approximately 63 light-years
Beta_Pictoris_c
Moving group of stars
1086/337968. "Extrasolar Visions - Beta Pictoris b". Archived from the original on 2010-11-17. Retrieved 2010-03-26. "Beta Pictoris planet finally imaged?" (Press
Beta_Pictoris_moving_group
French astronomer
and modern image processing tools, Lagrange discovered the exoplanet Beta Pictoris b orbiting around the star, confirming her earlier predictions. In 2019
Anne-Marie_Lagrange
French Nanosatellite
nanosatellite, designed to measure the transit of Beta Pictoris b, an exoplanet which orbits the star Beta Pictoris. PicSat was designed and built by a team of
PicSat
Constellation in the southern celestial hemisphere
orbit of Saturn. Beta Pictoris b was discovered using direct imagery with the Very Large Telescope in late 2009, while Beta Pictoris c was discovered
Pictor
Star in the constellation Pictor
the proper motion anomaly. Beta Pictoris GQ Lupi List of exoplanets discovered between 2000–2009 - including AB Pictoris b List of exoplanets discovered
AB_Pictoris
Circumbinary planetary-mass object orbiting ROXs 42B
about 2,000 K or a radius of 2.55 ± 0.20 RJ for about 1950 K. Like Beta Pictoris b, ROXs 42Bb's atmosphere is likely very cloudy and dusty. The object
ROXs_42Bb
Beta Pictoris b's distance from its star is 9 AU. At such distances the rotation of Jovian planets is not slowed by tidal effects. Beta Pictoris b is
Exoplanet orbital and physical parameters
Exoplanet_orbital_and_physical_parameters
Stellar classification
stars. A-type star systems known to feature planets include HD 15082, Beta Pictoris and HR 8799. Examples of A-type main-sequence stars with circumstellar
A-type_main-sequence_star
VLT measures the spin of Beta Pictoris b". April 30, 2014. Landman, R.; Stolker, T.; et al. (February 2024). "β Pictoris b through the eyes of the upgraded
List_of_hottest_exoplanets
Disk of dust and debris in orbit around a star
explanation was confirmed with the 2008 discovery of the exoplanet Beta Pictoris b. Other exoplanet-hosting stars, including the first discovered by direct
Debris_disk
List of largest planets by size
1051/0004-6361/202039039. Lacour, S.; et al. (2021). "The mass of β Pictoris c from β Pictoris b orbital motion". Astronomy & Astrophysics. 654: L2. arXiv:2109
List_of_largest_exoplanets
Exoplanet in the constellation Crux
similar to other planetary-mass companions/exoplanets like beta Pictoris b or 1RXS J160929.1−210524 b, its projected separation from the star is much larger
HD_106906_b
Star in the constellation Pictor
AE Pictoris is an eclipsing binary star system in the southern constellation of Pictor. This dim, blue-white hued point of light is just barely visible
AE_Pictoris
Form of electromagnetic radiation
132E. doi:10.1002/andp.19053220607. English translation: Arons, A. B.; Peppard, M. B. (1965). "Einstein's proposal of the photon concept—a translation
Infrared
Extrasolar free-floating planet
sub-brown dwarf. It is approximately 80 light-years away and belongs to the Beta Pictoris moving group. The object was discovered in 2013 in images taken by the
PSO_J318.5−22
Study of the movement of stars
disks, such as TW Hydrae or directly imaged exoplanets, such as Beta Pictoris b or GU Psc b. A stellar stream is an association of stars orbiting a galaxy
Stellar_kinematics
European Space Agency scientific satellite
measure the mass of the exoplanet Beta Pictoris b and is sometimes used to study other long-period exoplanets, such as HR 5183 b. Pierre Lacroute (Observatory
Hipparcos
Variable star in the constellation Lepus
eye visibility under ideal conditions. AF Leporis is a member of the Beta Pictoris moving group, with an astronomically young age of about 24 million years
AF_Leporis
Telescope in the Atacama Desert, Chile
The telescope's scientific discoveries include direct imaging of Beta Pictoris b, the first extrasolar planet so imaged, tracking individual stars moving
Very_Large_Telescope
(15 September 2026). "Discovery of radio emission from the exoplanet β Pictoris b". arXiv:2609.16720 [astro-ph.EP]. Connerney, J. E. P.; Kotsiaros, S.;
List_of_exoplanet_extremes
et al. (2026-07-15). "Discovery of an Exterior Third Planet Orbiting β Pictoris". The Astrophysical Journal Letters. 1006 (1): L11. doi:10.3847/2041-8213/ae801b
List_of_exoplanet_firsts
Exoplanets confirmed or discovered from direct imaging
Rosa RJ, Vargas J, MacIntosh B, Bailey VP, et al. (2017). "1–2.4μm Near-IR Spectrum of the Giant Planet β Pictoris b Obtained with the Gemini Planet
List of directly imaged exoplanets
List_of_directly_imaged_exoplanets
Planet outside of the Solar System
The most massive exoplanet listed on the NASA Exoplanet Archive is HR 2562 b, about 30 times the mass of Jupiter. However, according to some definitions
Exoplanet
Star in the constellation Columba
close approach to the Beta Pictoris system. The estimated separation of the two stars at this time was around 1.9 ly (0.58 pc) and Beta Columbae may have
Beta_Columbae
Gaia spacecraft to Hipparcos data for the Beta Pictoris system was able to measure the mass of Beta Pictoris b, constraining it to 11±2 Jupiter masses.
Methods of detecting exoplanets
Methods_of_detecting_exoplanets
Lagrange X1982 Astrophysicist, French Academy of Sciences, discovered the exoplanet Beta Pictoris b Hong Wang X2010 Mathematician (2026 Fields Medal)
List of École polytechnique alumni
List_of_École_polytechnique_alumni
Star in the constellation Pavo
normally from the star's surface. As part of the Beta Pictoris moving group, HD 172555 is coeval with Beta Pictoris, approximately 20 million years old, and is
HD_172555
Comet outside the Solar System
other than the Sun. The first exocomets were detected in 1987 around Beta Pictoris, a very young A-type main-sequence star. There are now (as of February
Exocomet
rather than a planet. Similarly, a 2017 study showed 2MASS J21402931+1625183 b to actually have a mass of 69+8 −9 MJ, making it a high-mass brown dwarf or
List of exoplanets discovered between 2000–2009
List_of_exoplanets_discovered_between_2000–2009
Star in the constellation Microscopium
S2CID 34114530. Barrado y Navascués, David; et al. (August 1, 1999). "The age of beta Pictoris". The Astrophysical Journal. 520 (2): L123–L126. arXiv:astro-ph/9905242
AU_Microscopii
Star in the constellation Ophiuchus
1088/0004-637X/703/2/1188, S2CID 17938884 Smith, B. A.; Terrile, R. J. (1984), "A circumstellar disk around Beta Pictoris", Science, 226 (4681): 1421–1424, Bibcode:1984Sci
51_Ophiuchi
Star in the constellation Ursa Minor
Kochab /ˈkoʊkæb/, Bayer designation Beta Ursae Minoris (β Ursae Minoris, abbreviated β UMi, Beta UMi), is the brightest star in the bowl of the Little
Kochab
Star in the constellation Triangulum Australe
making it a debris disk candidate. This star may be a member of the Beta Pictoris moving group, an association of about 17 stars that share a common origin
Beta_Trianguli_Australis
Variable star in the constellation Pictor
Delta Pictoris, Latinized from δ Pictoris, is a binary star system in the southern constellation Pictor. It is visible to the naked with a combined apparent
Delta_Pictoris
Second brightest star in the Leo constellation
formed out of such a disk, Denebola and similar stars such as Vega and Beta Pictoris may be candidate locations for extrasolar planets. Kinematic studies
Denebola
Detecting planets located outside the Solar System
estimated at between 250 K and 430 K (between −20 °C and 160 °C). Beta Pictoris b: On June 10, for the first time astronomers have been able to directly
Discoveries_of_exoplanets
F-type main sequence star in the constellation Eridanus
P.; Barrado, D.; Montesinos, B.; Duchêne, G.; Bouy, H.; Pinte, C.; et al. (2014). "Gas and dust in the beta Pictoris moving group as seen by the Herschel
51_Eridani
Star in the constellation Telescopium
is approximately 158 light years from Earth and is a member of the Beta Pictoris Moving Group of stars that share a common motion through space. It forms
Eta_Telescopii
Research Astrophysicist at NASA's Goddard Space Flight Center
She is particularly known for her research on the debris disk around Beta Pictoris. Born in Kyoto, Japan, to an American potter and a Japanese Chemical
Aki_Roberge
Low mass binary brown dwarf
2MASS J02495639−0557352) is a young low-mass binary brown dwarf in the beta Pictoris moving group. It has one circumbinary planetary-mass companion, called
2MASS_J0249−0557
Planet not gravitationally bound to a star
911....7Z. doi:10.3847/1538-4357/abe3fa. ISSN 0004-637X. Langeveld, Adam B.; Scholz, Aleks; Mužić, Koraljka; Jayawardhana, Ray; Capela, Daniel; Albert
Rogue_planet
Star in the constellation Corona Australis
apparent visual magnitude of 4.929±0.025. The system is a member of the Beta Pictoris Moving Group. The pair orbit each other with a period of 450 years and
HD_165189_and_HD_165190
American professor and astrophysicist
the team that discovered and imaged the super-jupiter Beta Pictoris b around the star Beta Pictoris. In two papers published in 2018 and 2019, Apai, with
Daniel_Apai
Set of non-stellar objects in orbit around a star
planetary systems. The first exocomets were detected in 1987 around Beta Pictoris, a very young A-type main-sequence star. There are now a total of 11
Planetary_system
Astronomers have measured an exoplanet's length of day for the first time. Beta Pictoris b was found to have a day that lasts only eight hours. 1 May – Cancer
2014_in_science
Star in the southern zodiac constellation of Scorpius
extinction of 0.17 due to interstellar dust. It is a member of the Beta Pictoris moving group, a set of ~12 million year old stars that share a common
HD_146624
Large stellar association
has a similar size to the Beta Pictoris moving group (BPMG) and contains, like BPMG, more than 12 stars with spectral type B, A and F. The association
Tucana–Horologium_association
major discoveries in astronomy. First, several young stars, such as Beta Pictoris, were found to be surrounded by discs of cool dust, much as was predicted
History of Solar System formation and evolution hypotheses
History_of_Solar_System_formation_and_evolution_hypotheses
(1997). "β Pictoris revisited by Hipparcos. Star properties". Astronomy and Astrophysics. 320: L29–L32. Bibcode:1997A&A...320L..29C. "Beta Pictoris". SIMBAD
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
Astronomical theory about the Solar System
divided into two stages: a) accretion of a core of approximately 10 M🜨 and b) accretion of gas from the protoplanetary disk. Either method may also lead
Nebular_hypothesis
Star in the constellation Mensa
further away with a radial velocity of +16 km/s. It is a member of the Beta Pictoris moving group, a loose association of young stars moving through the
AO_Mensae
Type of circumstellar disk
Taurus members. 2MASS J0041353-562112 was discarded as it belongs to the Beta Pictoris moving group and does not show excess. There are different models to
Peter_Pan_disk
Brightest star in the constellation Lyra
Michelson, E. (1981). "The near ultraviolet stellar spectra of alpha Lyrae and beta Orionis". Monthly Notices of the Royal Astronomical Society. 197: 57–74.
Vega
Astronomer
Astrophysical Journal Letters., 673, L191 "Stabilization of the disk around Beta Pictoris by extremely carbon-rich gas," Roberge, A., Feldman, P. D., Weinberger
Alycia_J._Weinberger
Li, Alexis; Perrin, Marshall (2024-10-01). "MIRI MRS Observations of Beta Pictoris. II. The Spectroscopic Case for a Recent Giant Collision". The Astrophysical
List of extrasolar planetary collisions
List_of_extrasolar_planetary_collisions
F-type subgiant star in the constellation Cetus
at the rate of about 1 km/s. It has been proposed as a member of the Beta Pictoris moving group or the Tucana-Horologium association of co-moving stars;
HD_15115
Star in the constellation of Andromeda
likelihood (86%) that it is a member of the Beta Pictoris moving group. The star has one known exoplanet, Kappa Andromedae b. In traditional Arabic astronomy, the
Kappa_Andromedae
[citation needed] List of nearby stellar associations and moving groups β Pictoris moving group AB Doradus moving group Sheffler, Julia; Clark, Max; Soares-Furtado
Ursa_Major_moving_group
Supplement, 19: 281, Bibcode:1970ApJS...19..281B, doi:10.1086/190209. Frost, E. B. (December 1924), "Fourteen spectroscopic binaries", Astrophysical Journal
List of star systems within 150–200 light-years
List_of_star_systems_within_150–200_light-years
Greek American astronomer (born 1967)
discovered various forms of asymmetric structures in optical images of the Beta Pictoris disk. He was the lead scientist for the first optical images of debris
Paul_Kalas
Star in the constellation Pisces
second system, after Beta Pictoris that shows a large population of comets. The transit rate is about double compared to Beta Pictoris, with 0.40 exocomets
RZ_Piscium
Visible star that is nearly aligned with Earth's axis of rotation
Observer's Year: 366 Nights in the Universe. p. 283. Kaler, James B., "KOCHAB (Beta Ursae Minoris)", Stars, University of Illinois, retrieved 2018-04-28
Pole_star
Star in the constellation Circinus
Circini is a candidate member of a stellar kinematic group known as the Beta Pictoris moving group. This group shares a common origin and has an estimated
Alpha_Circini
et al. (15 July 2026). "Direct Imaging Discovery of Giant Exoplanet β Pictoris d: A Decade-long Game of Hide-and-seek". The Astrophysical Journal Letters
List of exoplanets discovered in 2026
List_of_exoplanets_discovered_in_2026
American artist
WAY TO FORGET, Maus Contemporary, Birmingham 2014: PULSE art fair, Beta Pictoris Gallery, Birmingham 2014: Launch, F18 gallery, New York City 2014: Put
Clayton_Colvin
Star cluster in the constellation of Taurus
distance of 132 pc based on stars in the AB Doradus, Tucana-Horologium and Beta Pictoris moving groups, which are all similar in age and composition to the Pleiades
Pleiades
Star in the constellation Telescopium
years from Earth in the constellation of Telescopium. It is part of the Beta Pictoris Moving Group. HD 181327 is surrounded by a thin debris disk which is
HD_181327
mercury–manganese star B A7V 4.21 Beta Reticuli 97 ± 2 Reticulum 03h 44m 11.97587s -64° 48′ 24.8610″ K0IV SB 3.84 Alpha Pictoris$ 97 ± 5 Pictor 06h 48m
List of star systems within 95–100 light-years
List_of_star_systems_within_95–100_light-years
Supplement, 19: 281, Bibcode:1970ApJS...19..281B, doi:10.1086/190209. Frost, E. B. (December 1924), "Fourteen spectroscopic binaries", Astrophysical Journal
List of star systems within 100–150 light-years
List_of_star_systems_within_100–150_light-years
Near-Earth asteroid
AD Leonis b Beta Pictoris c DS Tucanae b Gliese 251 c GJ 357 d Gliese 588 b c Gliese 687 c Gliese 555 b Gliese 754 b Gliese 784 b HR 5183 b Kepler-47d
2019_BE5
Binary star system in the constellation Cetus
variable, showing a similarity to the edge-on debris disk surrounding Beta Pictoris. The stellar classification of A2 IV/V matched an A-type star near the
HD_256
Star in the constellation Hercules
and thus is not a member of the system. "V* iot Her -- Variable Star of beta Cep type". SIMBAD. Centre de Données astronomiques de Strasbourg. Retrieved
Iota_Herculis
American artist
Fellowship in Rome, Italy in 2009. He is represented by Guido Maus, beta pictoris gallery / Maus Contemporary in Birmingham, AL.[clarification needed]
Leslie_Smith_III
Minor constellation in the southern celestial hemisphere
AT Microscopii are probably a wide triple system and members of the Beta Pictoris moving group. Nicknamed "Speedy Mic", BO Microscopii is a star with
Microscopium
Gas and dust surrounding a newly formed star
stars—most of which have ages in the range of ~10 million years (e.g. Beta Pictoris, 51 Ophiuchi) to billions of years (e.g. Tau Ceti). These systems are
Protoplanetary_disk
Substellar object
Vertical Cloud Structure of a Young Low-mass Brown Dwarf, an Analog to the β-Pictoris b Directly Imaged Exoplanet, through Keck I/MOSFIRE Spectrophotometric Variability"
Brown_dwarf
Star in the constellation of Draco
was considered the pole star until about 1800 BC, when the much brighter Beta Ursae Minoris (Kochab) began to approach the pole as well. Having gradually
Thuban
magnitude derived from adding the magnitudes of Mizar A (2.220 ±0.003) and Mizar B (3.88) as per the formula: 2.01 ≈ − 2.5 log 10 ( 10 − 0.4 ⋅ 2.220 + 10 −
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Mineral of magnesium iron silicate
olivine has also been detected in the planetesimal belt around the star Beta Pictoris. Minerals in the olivine group crystallize in the orthorhombic system
Olivine
Protoplanetary disk in the Taurus molecular cloud
List of resolved circumstellar disks Examples of other edge-on disks: Beta Pictoris (debris disks) AU Microscopii (debris disks) HD 106906 (debris disk)
HH_30
Natural object in space that releases gas
common in the Milky Way. The first exocomet system detected was around Beta Pictoris, a very young A-type main-sequence star, in 1987. A total of 11 such
Comet
Poisonous gas consisting of carbon and oxygen
the information about the molecular clouds in which most stars form. Beta Pictoris, the second brightest star in the constellation Pictor, shows an excess
Carbon_monoxide
Family of comets
families resembling the Kreutz group have been detected around the star Beta Pictoris. Until recently, a very bright member of the Kreutz sungrazers could
Kreutz_sungrazer
Stark, Christopher C.; et al. (2009). "51 Ophiuchus: A Possible Beta Pictoris Analog Measured with the Keck Interferometer Nuller". Astrophysical
List of exoplanets and planetary debris around giant stars
List_of_exoplanets_and_planetary_debris_around_giant_stars
Mensa 86.23 ± 0.05 8.07±0.01 K0 V b c d 219 Beta Pictoris Pictor 63.4 ± 0.1 3.861 A6V 221 Orion 66.23 ± 0.02 9.70 K7V/M0V b c d 222 Chi¹ Orionis Orion 28
List of Gliese and GJ objects (1-1000)
List_of_Gliese_and_GJ_objects_(1-1000)
Intergovernmental observatory in Chile
Archived from the original on 20 May 2020. Retrieved 4 May 2011. "Beta Pictoris planet finally imaged?". ESO. 21 November 2008. Archived from the original
European_Southern_Observatory
Interplanetary introduction of species
planetary systems such as Fomalhaut (25 ly (light-years) away) and Beta Pictoris (63.4 ly), both of which show accretion discs and signs of comets and
Directed_panspermia
Continuous band of stars that appears on plots of stellar color versus brightness
difficult to detect. Other classes of unstable main-sequence stars, like Beta Cephei variables, are unrelated to this instability strip. The total amount
Main_sequence
Alien civilizations in the TV show Babylon 5
Their homeworld is Abbai 4 called SsumsshaA, which orbits the star Beta Pictoris in Sector 16. A peaceful, matriarchal society, the Abbai were the central
Civilizations_in_Babylon_5
launch of PicSat in January 2018, a nano-satellite that surveys the Beta Pictoris star for exoplanets. The French space agency was also responsible for
French_space_programme
Constellation in the southern celestial hemisphere
to have brown dwarf companions. A member of the 12-million-year-old Beta Pictoris moving group of stars that share a common proper motion through space
Telescopium
Olofsson, Göran; Liseau, René (2021-02-01). "The far reaches of the β Pictoris debris disk". Astronomy and Astrophysics. 646: A132. arXiv:2101.06281.
List of resolved circumstellar disks
List_of_resolved_circumstellar_disks
Nearest OB association to Earth
group, ~8 million-year-old TW Hydrae association, ~12 million-year-old Beta Pictoris moving group, and possibly the ~30–50 million-year-old IC 2602 open
Scorpius–Centaurus association
Scorpius–Centaurus_association
Loose star cluster
Association (Pleiades moving group) Hyades Stream IC 2391 supercluster Beta Pictoris moving group Castor moving group AB Doradus moving group Zeta Herculis
Stellar_association
Accumulation of matter around a star
(e.g. Gomez's Hamburger or Flying Saucer). Other edge-on disks (e.g. Beta Pictoris or AU Microscopii) and face-on disks (e.g. IM Lupi or AB Aurigae) require
Circumstellar_disc
NASA-funded citizen science project
companion 2MASS J05581644–4501559 B and the brown dwarf UCAC3 52–1038 B, which is on a wide 7100 AU orbit. UCAC3 52–1038 B was later found to be a mildly
Backyard_Worlds
Hypothesis of the formation of the Moon
the nearby (29 pc distant) young (~12 My old) star HD 172555 in the Beta Pictoris moving group. A belt of warm dust in a zone between 0.25AU and 2AU from
Giant-impact_hypothesis
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