Difference between revisions of "Delta Trianguli"

From FenWiki
Jump to: navigation, search
(created as stub)
 
m
 
(3 intermediate revisions by the same user not shown)
Line 1: Line 1:
{{stub}}
+
{{stub}}{{Starbox
{{Starbox
+
 
|name=Delta Trianguli A/B
 
|name=Delta Trianguli A/B
 
|image=
 
|image=
Line 12: Line 11:
 
|other designations=8 Trianguli, δ Tri, δ Trianguli, ADS 1739, BD+33°395, CCDM J02170+3414, GC 2733, GCTP 464.00, Gliese 92, HD 13974, HIP 10644 HR 660, LFT 198, LHS 154, LTT 10770, SAO 55420
 
|other designations=8 Trianguli, δ Tri, δ Trianguli, ADS 1739, BD+33°395, CCDM J02170+3414, GC 2733, GCTP 464.00, Gliese 92, HD 13974, HIP 10644 HR 660, LFT 198, LHS 154, LTT 10770, SAO 55420
 
}}
 
}}
 
 
'''Delta Trianguli''' is a binary system made up of a yellow G-type star (similar to, but heavier than, Sol) with a companion believed to be an orange K-type star, both in the main sequence. They are in close orbit around their center of mass, averaging a separation of only 0.11 AU.
 
'''Delta Trianguli''' is a binary system made up of a yellow G-type star (similar to, but heavier than, Sol) with a companion believed to be an orange K-type star, both in the main sequence. They are in close orbit around their center of mass, averaging a separation of only 0.11 AU.
  
  
 
{{interstellar}}
 
{{interstellar}}
[[Category:Places in Fenspace]]
 
[[Category:Interstellar]]
 

Latest revision as of 00:58, 19 May 2016

Fenwiki stub.pngThis Fenspace article is a stub. You can help FenWiki by expanding it.
Places in Fenspace
Delta Trianguli A/B
Stellar characteristics
ConstellationTriangulum
Right ascension (Epoch J2000)02h 17m 03.2s
Declination (Epoch J2000)+34° 13' 27"
Spectral typeG0.5Ve / K4V(?)
Distance from Sol35.3 ± 0.3 ly
Other designations8 Trianguli, δ Tri, δ Trianguli, ADS 1739, BD+33°395, CCDM J02170+3414, GC 2733, GCTP 464.00, Gliese 92, HD 13974, HIP 10644 HR 660, LFT 198, LHS 154, LTT 10770, SAO 55420
This box: view  talk  edit


Delta Trianguli is a binary system made up of a yellow G-type star (similar to, but heavier than, Sol) with a companion believed to be an orange K-type star, both in the main sequence. They are in close orbit around their center of mass, averaging a separation of only 0.11 AU.