Langbahn Team – Weltmeisterschaft

ADS 16402: Difference between revisions

Content deleted Content added
Albambot (talk | contribs)
m robot Adding: ko:ADS 16402
Mike s (talk | contribs)
m remove link that redirects to this page
Line 12: Line 12:
<!-- Aitken Double Star 16402 -->
<!-- Aitken Double Star 16402 -->


'''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]].
'''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]].


==References==
==References==

Revision as of 22:49, 27 July 2008

ADS 16402
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Lacerta
Right ascension 22h 57m 47s
Declination +38° 40' 30"
Apparent magnitude (V) 10.0
Distance450 ly
(140 pc)
Spectral typeF8
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