Astronomy:HD 330075

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Short description: Star in the constellation Norma
HD 330075
Observation data
Equinox J2000.0]] (ICRS)
Constellation Norma[1]
Right ascension  15h 49m 37.69382s[2]
Declination −49° 57′ 48.6771″[2]
Apparent magnitude (V) 9.36[1]
Characteristics
Evolutionary stage main sequence[3]
Spectral type G5[4]
B−V color index 0.935±0.005[1]
Astrometry
Radial velocity (Rv)61.67±0.24[2] km/s
Proper motion (μ) RA: −232.760[2] mas/yr
Dec.: −92.540[2] mas/yr
Parallax (π)22.0467 ± 0.0443[2] mas
Distance147.9 ± 0.3 ly
(45.36 ± 0.09 pc)
Absolute magnitude (MV)5.89[1]
Details
Mass0.86±0.02[5] M
Radius0.85+0.02
−0.03
[2] R
Luminosity0.393±0.001[2] L
Surface gravity (log g)4.68±0.09[5] cgs
Temperature4,967+88
−65
[2] K
Metallicity [Fe/H]0.18±0.04[5] dex
Age5.30±4.22[5] Gyr
Other designations
CD−49°10033, Gaia DR2 5982775854377691136, HD 330075, HIP 77517, SAO 226248, PPM 321068, LTT 6312, NLTT 41237, 2MASS J15493770-4957486[6]
Database references
SIMBADdata
Extrasolar Planets
Encyclopaedia
data

HD 330075 is a star in the southern constellation of Norma. It has a yellow hue and an apparent visual magnitude of 9.36,[1] which makes it too faint to be seen with the naked eye – it is visible only with telescope or powerful binoculars. Parallax measurements provide a distance estimate of 148 light years from the Sun, and it is drifting further away with a radial velocity of 62 km/s.[2] The star is estimated to have come as close as 111.5 light-years some 409 million years ago.[1]

This object appears to be a slightly evolved dwarf with a spectral class of G5. That is, it is nearing the end of its main sequence lifetimes and is becoming a subgiant star. The star has very low chromospheric activity and is around five billion years old.[4] It is smaller than the Sun with 86%[5] of the Sun's mass and 85%[2] of the solar radius. As a consequence, it is radiating just 39% of the luminosity of the Sun from its photosphere at an effective temperature of 4,967 K.[2] It has a super-solar metallicity, which means the abundance of elements other than hydrogen and helium appears much higher than in the Sun.[5]

Planetary system

In 2004, the discovery of a hot Jupiter planet orbiting close to the star was announced. This is the first planet discovered by the then-new HARPS spectrograph.[4]

The HD 330075 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ≥ 0.76 MJ 0.043 3.369±0.004 0

See also

  • List of stars with extrasolar planets

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode2012AstL...38..331A  XHIP record for this object at VizieR.
  2. 2.00 2.01 2.02 2.03 2.04 2.05 2.06 2.07 2.08 2.09 2.10 2.11 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode2018A&A...616A...1G.  Gaia DR2 record for this source at VizieR.
  3. Hamer, Jacob H.; Schlaufman, Kevin C. (2019). "Hot Jupiters Are Destroyed by Tides While Their Host Stars Are on the Main Sequence". The Astronomical Journal 158 (5): 190. doi:10.3847/1538-3881/ab3c56. Bibcode2019AJ....158..190H. 
  4. 4.0 4.1 4.2 Pepe, F. et al. (2004). "The HARPS search for southern extra-solar planets I. HD 330075 b: A new "hot Jupiter"". Astronomy and Astrophysics 423 (1): 385–389. doi:10.1051/0004-6361:20040389. Bibcode2004A&A...423..385P. http://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=/articles/aa/full/2004/31/aa0389-04/aa0389-04.html. 
  5. 5.0 5.1 5.2 5.3 5.4 5.5 Maldonado, J. et al. (May 2018). "Chemical fingerprints of hot Jupiter planet formation". Astronomy & Astrophysics 612: 18. doi:10.1051/0004-6361/201732001. A93. Bibcode2018A&A...612A..93M. 
  6. "HD 330075". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HD+330075. 

Coordinates: Sky map 15h 49m 37.6913s, −49° 57′ 48.692″