HIP 70849

HIP 70849 is a 10th magnitude K-type main sequence star located approximately 78 light years away in the constellation Lupus. This star, which resembles a brighter red dwarf, is smaller, cooler, dimmer, and less massive than our Sun. In 2009, a gas giant planet/brown dwarf was found in orbit around it.

HIP 70849
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Lupus
Right ascension 14h 29m 18.563s[1]
Declination −46° 27 49.74[1]
Apparent magnitude (V) 10.4
Characteristics
Spectral type K7V
Apparent magnitude (B) 11.6
Apparent magnitude (J) 7.639
Apparent magnitude (H) 7.006
Apparent magnitude (K) 6.790
B−V color index 1.2
Astrometry
Proper motion (μ) RA: −47.12 ± 2.15[1] mas/yr
Dec.: −203.52 ± 1.93[1] mas/yr
Parallax (π)42.42 ± 2.09[1] mas
Distance77 ± 4 ly
(24 ± 1 pc)
Absolute magnitude (MV)8.5
Details
Mass0.62 M
Radius0.67 ± 0.04 R
Luminosity0.097 ± 0.012 L
Surface gravity (log g)4.34 cgs
Temperature3950 ± 100 K
Other designations
CD−45°9206, Gliese 550.3, LTT 5717, NLTT 37446, NSV 6678, PPM 760399
Database references
SIMBADdata
Exoplanet Archivedata
Extrasolar Planets
Encyclopaedia
data

There is also a potential T4.5 brown dwarf companion orbiting ~9000AU from HIP 70849.[2]

Planetary system

HIP 70849 b is an extrasolar planet orbiting the star. It has more than five times the mass of Jupiter and takes more than 3000 days to orbit at a semimajor axis of more than 3.5 AU.[3]

The HIP 70849 planetary system[3]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b >5 MJ >3.5 >3000 ?

See also

  • List of extrasolar planets

References


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