HD 895
| Observation data Epoch J2000 Equinox J2000 |
|
|---|---|
| Constellation | Andromeda |
| Right ascension | 00h 13m 23.921s[1] |
| Declination | +26° 59′ 15.17″[1] |
| Apparent magnitude (V) | 6.27[2] |
| Characteristics | |
| Spectral type | F8V[2] |
| B−V color index | 0.63[2] |
| Astrometry | |
| Proper motion (μ) | RA: -18.40 ± 1.30[1] mas/yr Dec.: -32.50 ± 0.59[1] mas/yr |
| Parallax (π) | 7.61 ± 0.97[1] mas |
| Distance | approx. 430 ly (approx. 130 pc) |
| Absolute magnitude (MV) | 6.909 |
| Other designations | |
| Database references | |
| SIMBAD | data |
| Database references | |
| SIMBAD | data |
HD 895 is a triple star system[3] in the constellation Andromeda. Its apparent magnitude is 6.27. Located around 131 parsecs (430 ly) away, the primary is a F-type main-sequence star of spectral type F8V,[2] a star that is currently fusing its core hydrogen. While the secondary star cannot be separated from the primary except by spectroscopy, the tertiary can, and has been found to be a spectroscopic binary itself,[4] although with an apparent magnitude of 10.37,[5] it is too faint to be seen without a telescope.
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 binary or multiple star system–related article is a stub. You can help Wikipedia by expanding it. |
- ↑ 1.0 1.1 1.2 1.3 1.4 Lua error in package.lua at line 80: module 'strict' not found.Vizier catalog entry
- ↑ 2.0 2.1 2.2 2.3 2.4 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
