HD 60532

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HD 60532
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Puppis
Right ascension 07h 34m 03.18084s[1]
Declination –22° 17′ 45.8398″[1]
Apparent magnitude (V) 4.450[2]
Characteristics
Spectral type F6 IV-V[3]
U−B color index +0.07[4]
B−V color index +0.51[4]
Astrometry
Radial velocity (Rv) 60.7[2] km/s
Proper motion (μ) RA: –39.87[1] mas/yr
Dec.: 46.84[1] mas/yr
Parallax (π) 38.91 ± 0.27[1] mas
Distance 83.8 ± 0.6 ly
(25.7 ± 0.2 pc)
Absolute magnitude (MV) 2.40[2]
Details
Mass 1.44+0.03
−0.1
[5] M
Radius 2.52 R
Luminosity 8.596 L
Surface gravity (log g) 4.09[6] cgs
Temperature 6,095[5] K
Metallicity [Fe/H] –0.42[5] dex
Rotational velocity (v sin i) 8[5] km/s
Age 2.7 ± 0.1[5] Gyr
Other designations
108 G. Puppis,[7][8] BD–21° 2007, GC 10134, HIP 36795, HR 2906, Gliese 279, SAO 174009
Database references
SIMBAD data
Exoplanet Archive data
ARICNS data
Extrasolar Planets
Encyclopaedia
data

HD 60532 is a white (F-type) main sequence star located approximately 84 light-years away in the constellation of Puppis, taking its primary name from its Henry Draper Catalogue designation. It is calculated to be 1.44 times more massive than the Sun. The star is only 59% as old as our Sun (2.7 Gyr) and has metallicity of only 38% that of our Sun. In 2008, two extrasolar planets were discovered in orbit around it.

Planetary system

In September 2008, two Jupiter-like planets were found orbiting the star.[5] The orbital periods of these two planets appear to be in 3:1 resonance.[9]

The HD 60532 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 3.15 MJ 0.77 201.83 ± 0.14 0.278 ± 0.006
c 7.46 MJ 1.58 607.06 ± 2.1 0.038 ± 0.008

See also

References

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  5. 5.0 5.1 5.2 5.3 5.4 5.5 Lua error in package.lua at line 80: module 'strict' not found.web preprint
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External links

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Coordinates: Sky map 07h 34m 03.1805s, −22° 17′ 45.841″

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