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Gamma Cygni

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Also known as Sadr, 37 Cygni, γ Cygni, HIP 100453, HIC 100453, 37 Cyg, γ Cyg, HD 194093

star in the northern constellation Cygnus

In the Vinony graph

Vinony's link graph records 330 inbound references to Gamma Cygni, and connects out to year, apparent magnitude and star system.

It is catalogued under topics including Bayer objects, Brightest stars and Bright Star Catalogue objects.

Vinony links it to 32 Wikipedia language editions.

Key facts

Constellation
Cygnus
Right ascension
20 22 13.70184
Declination
+40 ° 15 ′ 24.0450 ″
Spectral type
F8 Iab
U b color index
+0.54
B v color index
+0.67
Variable type
suspected

via Wikipedia infobox

Wikidata facts

Constellation
Cygnus
Distance from Earth
560
Variable-star type
Cepheid variable
Show 17 more facts
catalog code
UBV M 24788
spectral class
F8p
stellar rotational velocity
20
apparent magnitude
2.113725
right ascension
305.55710787667
declination
40.25667361143
effective temperature
6000
parallax
1.78
radial velocity
-5.906
epoch
J2000.0
metallicity
-0.04
surface gravity
3.55
luminosity
33023
absolute magnitude
-4.54
right ascension component of proper motion
-2
declination component of proper motion
1
age estimated by a dating method
12
Sources (3)

via Wikidata · CC0

~4 min read

Encyclopedic overview

Gamma Cygni is a star in the northern constellation of Cygnus, forming the intersection of an asterism of five stars called the Northern Cross. It is officially named Sadr /ˈsædər/; Gamma Cygni is its Bayer designation, which that is Latinized from γ Cygni, and abbreviated Gamma Cyg or γ Cyg. Based upon parallax measurements obtained during the Hipparcos mission, it is approximately 1,800 light-years (560 parsecs) from the Sun.

It forms the primary or 'A' component of a multiple star system designated WDS J20222+4015 (the secondary or 'BCD' component is WDS J20222+4015BCD, a close triplet of stars 41" away from γ Cygni).

Excerpted from Wikipedia’s “Gamma Cygni” article, available under the CC BY-SA 4.0 licence.

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