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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
Constellation in the southern celestial hemisphere
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
Pictor
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
Brightest star in the southern constellation of Pictor
Alpha Pictoris (α Pic, α Pictoris) is the brightest star in the southern constellation of Pictor. It has an apparent visual magnitude of 3.27, which is
Alpha_Pictoris
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
Star in the constellation Octans
apparent magnitude of 5.5, but is slightly variable and is classified as a Delta Scuti variable. σ Octantis (Latinised to Sigma Octantis) is the star's Bayer
Sigma_Octantis
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 have
Denebola
Brightest star in the constellation Lyra
{\displaystyle {\begin{smallmatrix}\mu ={\sqrt {{\mu _{\delta }}^{2}+{\mu _{\alpha }}^{2}\cdot \cos ^{2}\delta }}\ =\ 327.78\ {\text{mas/y}}\end{smallmatrix}}}
Vega
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
Star cluster in the constellation of Taurus
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
Visible star that is nearly aligned with Earth's axis of rotation
never close enough to be taken as marking the pole, while third-magnitude Delta Cygni will be a more helpful pole star, at a distance of 3° from celestial
Pole_star
[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
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 planets
Directed_panspermia
Chinese From the Chinese name 亢 Kàng ('the neck'). /ˈkæŋ/ Kapteyn's Star† VZ Pictoris Pictor eponymous Named after the Dutch astronomer Jacobus Kapteyn. Karaka
List_of_proper_names_of_stars
00.92254s −18° 40′ 42.0313″ F2 V 6.72 50 parsecs (about 163.08 ly) AB Pictoris (HD 44627) 163.5 ± 0.1 Pictor 06h 19m 12.913s −58° 03′ 15.53″ K1V(e) 9
List of star systems within 150–200 light-years
List_of_star_systems_within_150–200_light-years
97 ± 2 Reticulum 03h 44m 11.97587s -64° 48′ 24.8610″ K0IV SB 3.84 Alpha Pictoris$ 97 ± 5 Pictor 06h 48m 11.45512s -61° 56′ 29.0008″ A8 Vn kA6 3.27# HD 52265
List of star systems within 95–100 light-years
List_of_star_systems_within_95–100_light-years
Extraterrestrial view of outer space
different from viewing space from orbit. Mercury has a southern pole star, α Pictoris, a magnitude 3.2 star. It is fainter than Earth's Polaris (α Ursae Minoris)
Extraterrestrial_sky
Cephei 115.3 ± 0.4 Cepheus 22h 49m 40.817s +66° 12′ 01.46″ K0III Zeta Pictoris 116.5 ± 1.0 Pictor 05h 19m 22.13501s −50° 36′ 21.4817″ F6 IV +5.43 HD 20781
List of star systems within 100–150 light-years
List_of_star_systems_within_100–150_light-years
Star 3.29 Iota Draconis (Edasich) Star Suspected variable star 3.30 Alpha Pictoris Star 3.30 Beta Phoenicis Binary star system 3.30 Xi Puppis Triple star
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Northern pole-star; brightest star in Ursa Minor
Polaris is part of the asterism Gouchen (勾陈, "Curved Array"), along with Delta, Epsilon and Zeta Ursae Minoris, and two other stars in Cepheus. In Inuit
Polaris
European Space Agency scientific satellite
Hipparcos-Gaia data was used to measure the mass of the exoplanet Beta Pictoris b and is sometimes used to study other long-period exoplanets, such as
Hipparcos
(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
Constellation in the southern celestial hemisphere
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
systems within 65–70 light-years List of nearest stars and brown dwarfs "Delta Equulei". University of Illinois Astronomy department. Archived from the
List of star systems within 60–65 light-years
List_of_star_systems_within_60–65_light-years
208 K3 V 185 HD 32450 Lepus 28.0 ± 0.4 8.317 (8.66 / 10.60) K7V 187 Eta¹ Pictoris Pictor 85.0 ± 0.4 5.37 F5 V 188 104 Tauri Taurus 50.3 ± 0.3 4.92 G4V 189
List of Gliese and GJ objects (1-1000)
List_of_Gliese_and_GJ_objects_(1-1000)
Nearest OB association to Earth
~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 cluster
Scorpius–Centaurus association
Scorpius–Centaurus_association
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
Brown_dwarf
Study of the movement of stars
protoplanetary 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
Star in the constellation Canis Minor
passage 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
YZ_Canis_Minoris
Continuous band of stars that appears on plots of stellar color versus brightness
instability strip intersecting the upper part of the main sequence are called Delta Scuti variables. Main-sequence stars in this region experience only small
Main_sequence
(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
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