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Beta Pictoris moving group information


β Pic Moving Group
Observation data
Distance115 ly (35 pc)
Physical characteristics
Estimated age20–26 Ma[1]
Associations
See also: Open cluster, List of open clusters

The Beta Pictoris Moving Group is a young moving group of stars located relatively near Earth. A moving group, in astronomy, is a group of stars that share a common motion through space as well as a common origin. This moving group is named for Beta Pictoris.

The Beta Pictoris Moving Group is an important object for astronomical study as it is the closest youthful group of stars to the Earth.[2] The star Beta Pictoris is known to have a large disk of gas and dust, possibly a protoplanetary disk. There is also evidence of a young gas giant planet around the star.[3][4] A free-floating planet has also been found in the moving group, PSO J318.5-22.[5] It has recently been estimated, as of 17 October 2023, that more than a third of the single Sun-like stars in the group have planets with more than four times the mass of Jupiter, and virtually all of the single Sun-like stars, 99%, possess at least one gas giant in orbit around them.[6] The age and distance of the group makes it a candidate for directly imaging extrasolar planets.

  1. ^ Cite error: The named reference Mamajek2014 was invoked but never defined (see the help page).
  2. ^ Zuckerman, B.; et al. (2001). "The β Pictoris Moving Group". The Astrophysical Journal. 562 (1): L87–L90. Bibcode:2001ApJ...562L..87Z. doi:10.1086/337968.
  3. ^ "Extrasolar Visions - Beta Pictoris b". Archived from the original on 2010-11-17. Retrieved 2010-03-26.
  4. ^ "Beta Pictoris planet finally imaged?" (Press release). ESO. 2008-11-21. Archived from the original on 2009-02-08. Retrieved 2008-11-22.
  5. ^ "A Strange Lonely Planet Found Without a Star". Science Daily. 2013-10-09.
  6. ^ Gratton, Raffaele; Mesa, Dino; Bonavita, Mariangela; et al. (2023-10-17). "Jupiter-like planets might be common in a low-density environment". Nature Communications. 14 (1). Springer Science and Business Media LLC. arXiv:2310.11190. doi:10.1038/s41467-023-41665-0. ISSN 2041-1723.

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Beta Pictoris moving group

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The Beta Pictoris Moving Group is a young moving group of stars located relatively near Earth. A moving group, in astronomy, is a group of stars that...

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Beta Pictoris

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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...

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Rogue planet

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J111010.01+011613.1: A New Planetary-mass T Dwarf Member of the AB Doradus Moving Group". Astrophysical Journal Letters. 808 (1): L20. arXiv:1506.04195. Bibcode:2015ApJ...

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Beta Pictoris c

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Beta Pictoris c (abbreviated as β Pic c) is the second exoplanet discovered orbiting the young star Beta Pictoris, located approximately 63 light-years...

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Stellar kinematics

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kinematic groups include: Local Association (Pleiades moving group) AB Doradus moving group Alpha Persei moving cluster Beta Pictoris moving group Castor...

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Microscopium

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Microscopii are probably a wide triple system and members of the Beta Pictoris moving group. Nicknamed "Speedy Mic", BO Microscopii is a star with an extremely...

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Ursa Major moving group

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Ursa Major group.[citation needed] List of nearby stellar associations and moving groups β Pictoris moving group AB Doradus moving group King, Jeremy...

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AF Leporis

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from the presence of starspots. AF Leporis is a member of the Beta Pictoris moving group, with an astronomically young age of about 24 million years. It...

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Telescopium

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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, Eta...

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AU Microscopii

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hued glow of an M-type star. AU Microscopii is a member of the β Pictoris moving group. AU Microscopii may be gravitationally bound to the binary star...

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Pictor

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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...

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Beta Trianguli Australis

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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 and...

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Kappa Andromedae

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and there is a high likelihood (86%) that it is a member of the Beta Pictoris moving group. The star has one known companion exoplanet, Kappa Andromedae...

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PicSat

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measurement of Beta Pictoris' brightness. A fast-moving piezoelectric actuator was added to PicSat to keep the optical fiber tracked upon Beta Pictoris, since...

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Eta Telescopii

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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 a...

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51 Eridani

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main-sequence star of spectral type F0V, 51 Eridani is a member of the Beta Pictoris moving group and hence thought to be around 23 million years old. Somewhat...

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Stellar association

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that group.) Other young moving groups include: Local Association (Pleiades moving group) Hyades Stream IC 2391 supercluster Beta Pictoris moving group Castor...

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YZ Canis Minoris

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at a distance of 10.2 ly. YZ CMi is a potential member of the Beta Pictoris moving group. This is a red dwarf star, or M-type main-sequence star, with...

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Alpha Circini

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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 age...

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HD 15115

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has been proposed as a member of the Beta Pictoris moving group or the Tucana-Horologium association of co-moving stars; there is some ambiguity as to...

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Beta Columbae

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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...

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Backyard Worlds

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objects, leaving moving objects intact. The aim is to identify points of light that move between the flip book frames, including slower-moving "dipoles". Citizen...

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Pleiades

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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...

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AO Mensae

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velocity of +16 km/s. It is a member of the Beta Pictoris moving group, a loose association of young stars moving through the galaxy. This is an orange-hued...

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HD 172555

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would be emitted normally from the star's surface. As part of the Beta Pictoris moving group, HD 172555 is coeval with that more famous system, approximately...

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