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HD 44385

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HD 44385
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Camelopardalis
Right ascension  06h 33m 04.00s[1]
Declination +78° 58′ 46.30″[1]
Apparent magnitude (V) 6.60 ± 0.01[2]
Characteristics
Evolutionary stage red giant
Spectral type K2II-III[1] or K0
Astrometry
Radial velocity (Rv)15.28 ± 0.14[1] km/s
Proper motion (μ) RA: -4.328 ± 0.033[1] mas/yr
Dec.: -17.300 ± 0.038[1] mas/yr
Parallax (π)4.5278 ± 0.0254[1] mas
Distance720 ± 4 ly
(221 ± 1 pc)
Details[3]
Mass1.8 ± 0.2 M
Radius18.2 ± 1.2 R
Luminosity233.2 L
Surface gravity (log g)1.80 cgs
Temperature4499 K
Metallicity [Fe/H]0.10 ± 0.07 dex
Rotational velocity (v sin i)2.6 ± 0.5 km/s
Age1.8 ± 0.4 Gyr
Other designations
BD+79 202, HD 44385, HIP 31231, GSC 04533-00372
Database references
SIMBADdata

HD 44385 is a star in the circumpolar constellation Camelopardalis. With an apparent magnitude of 6.60, it's below maximum naked eye visibility.

Properties[edit]

Distance[edit]

This star has a radial velocity of 15.28, which means it's drifting away from the Solar System. HD 44385 is currently 720 light years from earth based on parallax.

Properties[edit]

According to the paper, this star has a classification of K0. It has 1.8 times the mass of the Sun, but has expanded to 18.2 times the latter's girth. It radiates at 233.2 times the luminosity of the Sun, and has a similar metallicity to it. HD 44385 has an effective temperature of 4499 K, which gives it an orange hue of a K-type star.

Planetary System[edit]

In 2018, SENS discovered an extrasolar planet orbiting the giant star. Not much is known about this planet, and was discovered via Doppler spectroscopy.

The HD 44385 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b (uncofirmed) 5.9 ± 1.1 MJ 1.4 ± 0.1 473.5 ± 4.9 0.20 ± 0.20

Notes[edit]

1.^ Self-calculated based on temperature and luminosity.

References[edit]

  1. 1.0 1.1 1.2 1.3 1.4 Gaia Collaboration (2018-04-01). "VizieR Online Data Catalog: Gaia DR2 (Gaia Collaboration, 2018)". VizieR Online Data Catalog. 1345. Bibcode:2018yCat.1345....0G.
  2. Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000-03-01). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode:2000A&A...355L..27H. ISSN 0004-6361.
  3. Jeong, Gwanghui; Han, Inwoo; Park, Myeong-Gu; Hatzes, Artie P.; Bang, Tae-Yang; Gu, Shenghong; Bai, Jinming; Lee, Byeong-Cheol (2018-08-01). "A Search for Exoplanets around Northern Circumpolar Stars. IV. Six Planet Candidates to the K Giants, HD 44385, HD 97619, HD 106574, HD 118904, HD 164428, and HD 202432". The Astronomical Journal. 156 (2): 64. arXiv:1808.01109. Bibcode:2018AJ....156...64J. doi:10.3847/1538-3881/aacbc1. ISSN 0004-6256. Unknown parameter |s2cid= ignored (help)


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