HD 38283

Star in the constellation Mensa From Wikipedia, the free encyclopedia

HD 38283, or Bubup, is a star in the southern circumpolar constellation Mensa. With a magnitude of 6.70, it's invisible to the naked eye but can be seen with binoculars. Bubup is located relatively close at a distance of 124 light-years but is recceding with a heliocentric radial velocity of 61.5 km/s.[1]

Right ascension05h 37m 02.0168s[1]
Declination−73° 41 57.645[1]
Quick facts Observation data Epoch J2000.0 Equinox J2000.0, Constellation ...
HD 38283 / Bubup
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Mensa
Right ascension 05h 37m 02.0168s[1]
Declination −73° 41 57.645[1]
Apparent magnitude (V) 6.70[2]
Characteristics
Evolutionary stage subgiant[1]
Spectral type F9.5 V[3]
B−V color index 0.540[4]
Astrometry
Radial velocity (Rv)61.50±0.13[1] km/s
Proper motion (μ) RA: 138.794 mas/yr[1]
Dec.: −108.499 mas/yr[1]
Parallax (π)26.2854±0.0170 mas[1]
Distance124.08 ± 0.08 ly
(38.04 ± 0.02 pc)
Absolute magnitude (MV)3.82[4]
Details[5]
Mass1.37 ± 0.07 M
Radius1.49 ± 0.0 R
Luminosity2.35[4] L
Surface gravity (log g)4.23 ± 0.02 cgs
Temperature5,981 ± 12 K
Metallicity [Fe/H]−0.18 dex
Rotational velocity (v sin i)3.8[6] km/s
Age7.43[6] Gyr
Other designations
Bubup, CD−73°253, HD 38283, HIP 26380, SAO 256213, 2MASS J05370199-7341574[7]
Database references
SIMBADdata
Exoplanet Archivedata
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Nomenclature

HD 38283 was given the name "Bubup", the Boonwurrung word for "child", by the IAU, chosen by representatives of Australia for the 2019 NameExoWorlds contest.[8]

Properties

HD 38283/Bubup has a stellar classification of F9.5 V,[3] indicating that it is an ordinary late F-type main-sequence star just shy of being a G-type main-sequence star. At present it has 137% the mass of the Sun[5] and 149% the radius of the Sun.[5] It shines at about double the luminosity of the Sun from its photosphere at an effective temperature of 5981 K,[5] which gives it a yellow glow. Unlike most planetary hosts, HD 38283/Bubup is metal-deficient with an iron abundance 66% that of the Sun[5] and is older than the latter with an age of about 7 billion years.[6] Currently, it spins leisurely with a projected rotational velocity of about 4 km/s.[6]

A survey in 2015 has ruled out the existence of any stellar companions at projected distances above 11 AU.[9]

Planetary system

On April 11, 2011, a Saturnian planet, HD 38283 b (Yanyan), was discovered in an Earth-like 363-day orbit.[4] HD 38283 b/Yanyan itself turns out to be unable to host habitable exomoons, both because of its significant eccentricity (for the single eccentric planet solution), and because of the overluminosity of its host star compared to the Sun.[4]

More information Companion (in order from star), Mass ...
The HD 38283 planetary system[10]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ≥0.289±0.034 MJ 1.020±0.002 361.0±1.1 0.474±0.136
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See also

References

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