HD 330075
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Norma |
Right ascension | 15h 49m 37.6913s[1] |
Declination | –49° 57′ 48.692″[1] |
Apparent magnitude (V) | 9.36[1] |
Characteristics | |
Spectral type | G5[1] |
Apparent magnitude (B) | ~10.3[1] |
Apparent magnitude (V) | 9.36[1] |
Astrometry | |
Proper motion (μ) | RA: -235.58 ±1.41 [1] mas/yr Dec.: -94.14 ±1.18[1] mas/yr |
Parallax (π) | 19.92[1] ± 1.49[1] mas |
Distance | 163.7 ly (50.2 pc) |
Details | |
Mass | 0.95 M☉ |
Temperature | 6295 K |
Metallicity | 0.03 Fe/H |
Age | 6.21 billion years |
Other designations | |
NLTT 41237, CPD-49 8621, HIP 77517, PPM 321068, CD-49 10033, LTT 6312, SAO 226248,
CPC 0 14030, HIC 77517, PLX 3572[1] | |
Database references | |
SIMBAD | data |
Extrasolar Planets Encyclopaedia | data |
HD 330075 is a 9th magnitude star approximately 164 light-years away in the southern constellation of Norma. Like our Sun, it is a yellow dwarf (spectral type G5). However, it is slightly cooler and less luminous. Due to its distance, it is rather dim and visible only with telescope or powerful binoculars.[1]
Planetary system
In 2004, the discovery of a hot Jupiter planet orbiting the star was announced. This is the first planet discovered by the HARPS spectrograph.[2]
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
References
- 1 2 3 4 5 6 7 8 9 10 11 12 "SIMBAD query result: NLTT 41237 -- High proper-motion Star". SIMBAD. Centre de Données astronomiques de Strasbourg. Retrieved 2009-05-22.
- ↑ 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. arXiv:astro-ph/0405252. Bibcode:2004A&A...423..385P. doi:10.1051/0004-6361:20040389.
External links
- "HD 330075". Exoplanets. Retrieved 2009-05-22.
Coordinates: 15h 49m 37.6913s, −49° 57′ 48.692″
This article is issued from Wikipedia - version of the 3/31/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.