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HD 149382: Difference between revisions

Coordinates: Sky map 23h 41m 51.5299s, −05° 59′ 08.726″
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'''HD 149382''' is a [[B-type]] [[subdwarf star]] approximately 242 [[light-year]]s away from [[Sun]] in the [[constellation]] of [[Ophiuchus (constellation)|Ophiuchus]]. In 2009, a [[substellar]] companion (even a [[superjovian]] [[extrasolar planet|planet]]) was announced orbiting the star.<ref name="Geier et al."> {{cite journal | url=http://fr.arxiv.org/abs/0908.1025| author=Geier et al.| title=Discovery of a close substellar companion to the hot subdwarf star HD 149382 - The decisive influence of substellar objects on late stellar evolution|journal=[[The Astrophysical Journal Letters]]|volume=702|issue=1| pages=96-99 | year=2009 | bibcode=2009ApJ...702L..96G}}</ref>. This star has nearly half the mass of ''SOL'', and is 241 light years away from earth.
'''HD 149382''' is a [[B-type]] [[subdwarf star]] approximately 242 [[light-year]]s away from [[Sun]] in the [[constellation]] of [[Ophiuchus (constellation)|Ophiuchus]]. In 2009, a [[substellar]] companion (even a [[superjovian]] [[extrasolar planet|planet]]) was announced orbiting the star.<ref name="Geier et al."> {{cite journal | url=http://fr.arxiv.org/abs/0908.1025| author=Geier et al.| title=Discovery of a close substellar companion to the hot subdwarf star HD 149382 - The decisive influence of substellar objects on late stellar evolution|journal=[[The Astrophysical Journal Letters]]|volume=702|issue=1| pages=96–99 | year=2009 | bibcode=2009ApJ...702L..96G}}</ref>. This star has nearly half the mass of ''SOL'', and is 241 light years away from earth.


{{OrbitboxPlanet begin|name=HD 149382}}
{{OrbitboxPlanet begin|name=HD 149382}}

Revision as of 14:59, 14 April 2010

HD 149382

Brown dwarf HD 149382 b.
Observation data
Epoch J2000      Equinox J2000
Constellation Ophiuchus
Right ascension 16h 34m 23.3338s
Declination –04° 00′ 52.015″
Apparent magnitude (V) 8.9
Characteristics
Spectral type B5VI
Astrometry
Distance241.2 ly
(74±8 pc)
Details
Mass0.47 M
Radius0.24 R
Luminosity82 L
Temperature35,500 K
Other designations
ALS 9317, HD 149382, HIP 81145, SAO 141250
Database references
SIMBADdata

HD 149382 is a B-type subdwarf star approximately 242 light-years away from Sun in the constellation of Ophiuchus. In 2009, a substellar companion (even a superjovian planet) was announced orbiting the star.[1]. This star has nearly half the mass of SOL, and is 241 light years away from earth.

The HD 149382 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b >8-23 MJ 0.02343 2.391 0 39±13°

See also

References

  1. ^ Geier; et al. (2009). "Discovery of a close substellar companion to the hot subdwarf star HD 149382 - The decisive influence of substellar objects on late stellar evolution". The Astrophysical Journal Letters. 702 (1): 96–99. Bibcode:2009ApJ...702L..96G. {{cite journal}}: Explicit use of et al. in: |author= (help)