HD 1273
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Phoenix |
| Right ascension | 00h 16m 53.89 s |
| Declination | −52° 39′ 04.2″ |
| Apparent magnitude (V) | 6.852 |
| Characteristics | |
| Spectral type | G2V |
HD 1273 is a G2V spectroscopic binary star located 75.1 light years away, in the constellation of Phoenix.[1][2] In 1972, Cathpole proposed an astrometric orbit to explain the discrepancy between the trigonometric and spectroscopic parallax of HD 1273.[3]
The star also receives the names of Gl 13, Hip 1349 and CD-53 36 A.[4][5] As of December 2020, no exoplanets have been discovered around this Sun-like star.[6] With an apparent magnitude of 6.852, the star is visible to the naked eye according to the Astronomical Magnitude Scale.[7]
References[edit]
- ↑ "G stars within 100 light-years". www.solstation.com. Retrieved 2020-12-16.
- ↑ "HD 1273 - Star - WIKISKY". server7.wikisky.org. Retrieved 2020-12-16.
- ↑ Catchpole, R. M. (1972-08-01). "A possible astrometric spectroscopic binary". The Observatory. 92: 125–127. Bibcode:1972Obs....92..125C. ISSN 0029-7704.
- ↑ Bopp, Bernard W.; Evans, David S.; Laing, J. D.; Deeming, T. J. (1970-04-01). "Orbital Elements of Six Spectroscopic Binary Stars". Monthly Notices of the Royal Astronomical Society. 147 (4): 355–366. Bibcode:1970MNRAS.147..355B. doi:10.1093/mnras/147.4.355. ISSN 0035-8711.
- ↑ "HD 1273". sim-basic. Retrieved 2020-12-16. Unknown parameter
|url-status=ignored (help) - ↑ "Exoplanet Catalog | Discovery". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 2020-12-16.
- ↑ "The astronomical magnitude scale". www.icq.eps.harvard.edu. Retrieved 2020-12-27.
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