HD 103774

HD 103774 is a young yellow-white main-sequence star of apparent magnitude 7.12 that is 181 ± 5 light-years distant from Earth. It is 1.335 ± 0.03 times as massive and 3.5 ± 0.3 as luminous as the Sun.[2]

HD 103774
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Corvus
Right ascension  11h 56m 56s
Declination −12° 6 28
Apparent magnitude (V) 7.12 ± 0.01
Characteristics
Spectral type F6 V[1]
Astrometry
Parallax (π)18.03 ± 0.52 mas
Distance181 ± 5 ly
(55 ± 2 pc)
Details
Mass1.335 ± 0.03 M
Radius? R
Luminosity3.5± 0.3 L
Surface gravity (log g)4.26 ± 0.13 cgs
Temperature6489 ± 77 K
Metallicity0.28 ± 0.06
Age1.05 ± 0.64 × 109 years
Other designations
HIP 58263, SAO 157002, BD-11°3211
Database references
SIMBADdata
Exoplanet Archivedata
Extrasolar Planets
Encyclopaedia
data

Planetary system

From 2003 to 2012, the star was under observation from HARPS.

In 2012, a hot Saturn-mass[3] planet was deduced by radial velocity. This result was published in January 2013.

Also probable is a dust field, with grains of 12 micrometres.

The HD 103774 planetary system[4][2]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b >0.367 ± 0.022 MJ 0.07 ± 0.001 5.8881 ± 0.0005 0.09 ± 0.04
gollark: IIRC the Old Testament actually contains recordings of commands by god to kill specific groups.
gollark: Not all religions say "be peaceful and not mean to each other", though?
gollark: I mean, if you believe Religion 1 and believe that everyone who believes Religion 2 will go to hell and suffer forever, then you obviously don't want Religion 2 to spread.
gollark: They're pretty rational if you actually believe your religion is true, though.
gollark: Looking at religious conflicts probably doesn't require knowing about all the deep details of the religions involved, because people do tribalism and probably do not meaningfully care about the actual underlying point.

References

  1. Houk, N.; Swift, C. (1999), "Michigan catalogue of two-dimensional spectral types for the HD Stars", Michigan Spectral Survey, Ann Arbor, Michigan: Department of Astronomy, University of Michigan, 5, Bibcode:1999MSS...C05....0H.
  2. Lo Curto, G.; Mayor, M.; Benz, W.; Bouchy, F.; Hébrard, G.; Lovis, C.; Moutou, C.; Naef, D.; Pepe, F.; Queloz, D.; Santos, N. C.; Segransan, D.; Udry, S. (2013). "The HARPS search for southern extrasolar planets: XXXVI. New multi-planet systems in the HARPS volume limited sample: a super-Earth and a Neptune in the habitable zone". Astronomy & Astrophysics. 551: 7. arXiv:1301.2741. Bibcode:2013A&A...551A..59L. doi:10.1051/0004-6361/201220415. A59.
  3. The preprint listed this as "roughly the mass of Neptune" but it is much more massive than that.
  4. "hd_103774_b".


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