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'''ADS 16402''' is a [[binary star|binary]] [[star system]], composed of two sun-like [[star]]s. The two stars are separated by 1500 [[astronomical unit|AU]]s. The star system is estimated at being 3.6 billion years old. ''ADS 16402B'' (aka |
'''ADS 16402''' is a [[binary star|binary]] [[star system]], composed of two sun-like [[star]]s. The two stars are separated by 1500 [[astronomical unit|AU]]s. The star system is estimated at being 3.6 billion years old. ''ADS 16402B'' (aka HAT-P-1) is orbited by the enormous bloated gas planet [[HAT-P-1b]]. |
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==References== |
==References== |
Revision as of 22:49, 27 July 2008
Observation data Epoch J2000.0 Equinox J2000.0 | |
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Constellation | Lacerta |
Right ascension | 22h 57m 47s |
Declination | +38° 40' 30" |
Apparent magnitude (V) | 10.0 |
Distance | 450 ly (140 pc) |
Spectral type | F8 |
Other designations | |
BD+37°4734s, SAO 72884 |
ADS 16402 is a binary star system, composed of two sun-like stars. The two stars are separated by 1500 AUs. The star system is estimated at being 3.6 billion years old. ADS 16402B (aka HAT-P-1) is orbited by the enormous bloated gas planet HAT-P-1b.
References
- exoplanet.eu Star : HAT-P-1
- simbad Object query : ADS 16402 B