Gamma Phoenicis
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) |
|
|---|---|
| Constellation | Phoenix |
| Right ascension | 01h 28m 21.93s[1] |
| Declination | −43° 19′ 05.7″[1] |
| Apparent magnitude (V) | 3.41[2] |
| Spectral type | M0III[3] |
Gamma Phoenicis is a star system in the constellation Phoenix. Located around 71.63 parsecs (233.6 ly) distant,[1] it is an red giant of spectral type M0III,[3] a star that has used up its core hydrogen and has expanded. A spectroscopic binary, the two components orbit each other in 193.75 days, producing eclipses that cause the apparent magnitude to drop to 3.49 from its baseline of 3.39.[4] The primary, with a spectral type of M0III,[3] is also a slow irregular variable, showing small intrinsic variations.[4]
References
<templatestyles src="Reflist/styles.css" />
Cite error: Invalid <references> tag; parameter "group" is allowed only.
<references />, or <references group="..." /><templatestyles src="Asbox/styles.css"></templatestyles>
 |
This giant-star-related article is a stub. You can help Wikipedia by expanding it. |
<templatestyles src="Asbox/styles.css"></templatestyles>
 |
This variable star–related article is a stub. You can help Wikipedia by expanding it. |
