Difference between revisions of "HIP 30104"
m |
|||
| Line 1: | Line 1: | ||
| − | {{ | + | {{Needs WikiMagic|This page is a Wikipedia or SolStation data dump with little or no relation – or, worse yet, with contradictions – to the situation in Fenspace.}}{{Starbox |
|name=HIP 30104 | |name=HIP 30104 | ||
|image= | |image= | ||
| Line 12: | Line 12: | ||
|planets= | |planets= | ||
}} | }} | ||
| − | |||
'''HIP 30104''' is located about 83.8 light-years from Sol. It lies in the southwest corner of the constellation Puppis, the Stern of the legendary ship Argo Navis. | '''HIP 30104''' is located about 83.8 light-years from Sol. It lies in the southwest corner of the constellation Puppis, the Stern of the legendary ship Argo Navis. | ||
Revision as of 19:35, 21 February 2016
 There's something missing here…This page is a Wikipedia or SolStation data dump with little or no relation – or, worse yet, with contradictions – to the situation in Fenspace. You can help FenWiki by expanding this page. |
| HIP 30104 | |
| Stellar characteristics | |
|---|---|
| Constellation | Puppis |
| Right ascension (Epoch J2000) | 06h 20m 06.10s |
| Declination (Epoch J2000) | -48° 44' 27.90" |
| Spectral type | G3-4 V |
| Distance from Sol | 83.8 ly |
| Other designations | HR 2290, Hip 30104, HD 44594, CD-48 2259, CP(D)-48 833, SAO 217861, FK5 2486, LTT 2525. |
HIP 30104 is located about 83.8 light-years from Sol. It lies in the southwest corner of the constellation Puppis, the Stern of the legendary ship Argo Navis.
HIP 30104 is a yellow-orange main sequence dwarf star of spectral and luminosity type G3-4 V. Similar to Sol[1][2][3][4], this possible "Solar twin" may have roughly the same mass, the same diameter[5][6], and 1.25 times its luminosity. It appears to be almost 1.55 times as enriched than Sol in elements heavier than hydrogen ("metals") based on its abundance of iron[7]. With low chromospheric activity, the star appears to be much older than Sol's 4.6 billion years[8][9].
An Earth-type planet with liquid water on its surface would require a stable orbit centered around 1.1 AU from HIP 30104 -- just over the orbital distance of Earth in the Solar System. Assuming that the star has about one Solar-mass, such a planet would have an orbital period lasting close to 1.2 Earth years or around 430 days.
(Data from SolStation.com)
Notes
- ↑ (Giusa Cayrel de Strobel, 1996)
- ↑ (Cayrel de Strobel and Bentolila, 1989)
- ↑ (Hardorp et al, 1982)
- ↑ (Cayrel de Strobel, 1981)
- ↑ (Pasinetti-Fracassini et al, 2001)
- ↑ (Wesselink et al, 1972)
- ↑ (B.J. Taylor, 2003)
- ↑ (Guinan et al, 1999)
- ↑ (Fernley et al, 1996)
