Sidus Ludoviciana: Difference between revisions
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'''Sidus Ludoviciana''' {{IPAc-en|'|s|ai|d|@|s|_|,|lj|uː|d|ou|,|v|I|s|i|'|ei|n|@}}{{cn}} is an 8th-magnitude [[giant star]] in the [[Asterism (astronomy)|asterism]] of the [[Big Dipper]] in the constellation [[Ursa Major]], halfway between [[Mizar and Alcor|Mizar]] and [[Mizar and Alcor|Alcor]]. It was discovered on 2 December 1722 by [[Johann Georg Liebknecht]], who mistook it for a planet and named it after [[Louis V, Landgrave of Hesse-Darmstadt]]. A line-of-sight companion with Mizar and Alcor (with a spectral type similar to the latter), it is roughly |
'''Sidus Ludoviciana''' {{IPAc-en|'|s|ai|d|@|s|_|,|lj|uː|d|ou|,|v|I|s|i|'|ei|n|@}}{{cn}} is an 8th-magnitude [[giant star]] in the [[Asterism (astronomy)|asterism]] of the [[Big Dipper]] in the constellation [[Ursa Major]], halfway between [[Mizar and Alcor|Mizar]] and [[Mizar and Alcor|Alcor]]. It was discovered on 2 December 1722 by [[Johann Georg Liebknecht]], who mistook it for a planet and named it after [[Louis V, Landgrave of Hesse-Darmstadt]]. A line-of-sight companion with Mizar and Alcor (with a spectral type similar to the latter), it is roughly four times more distant. It has the spectral type A8/F0 III.<ref name=grenier/> |
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The star is six times more luminous than the [[Sun]], 1.6 times its radius, and has an [[effective temperature|surface temperature]] of {{val|7,167|fmt=commas|ul=K}}. It has exhausted its core hydrogen and evolved away from the [[main sequence]]. |
The star is six times more luminous than the [[Sun]], 1.6 times its radius, and has an [[effective temperature|surface temperature]] of {{val|7,167|fmt=commas|ul=K}}. It has exhausted its core hydrogen and evolved away from the [[main sequence]]. |
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Revision as of 10:57, 22 September 2019
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Ursa Major |
| Right ascension | 13h 24m 51.8516s[1] |
| Declination | +54° 53′ 50.839″[1] |
| Apparent magnitude (V) | +7.58[2] |
| Characteristics | |
| Spectral type | A8/F0III[3] |
| Astrometry | |
| Radial velocity (Rv) | −4.9[3] km/s |
| Proper motion (μ) | RA: −19.910[1] mas/yr Dec.: −5.202[1] mas/yr |
| Parallax (π) | 10.8536 ± 0.0280 mas[1] |
| Distance | 300.5 ± 0.8 ly (92.1 ± 0.2 pc) |
| Details | |
| Radius | 1.61[1] R☉ |
| Luminosity | 6.159[1] L☉ |
| Temperature | 7,167[1] K |
| Other designations | |
| Database references | |
| SIMBAD | data |
Sidus Ludoviciana /ˈsaɪdəs ˌljuːdoʊˌvɪsiˈeɪnə/[citation needed] is an 8th-magnitude giant star in the asterism of the Big Dipper in the constellation Ursa Major, halfway between Mizar and Alcor. It was discovered on 2 December 1722 by Johann Georg Liebknecht, who mistook it for a planet and named it after Louis V, Landgrave of Hesse-Darmstadt. A line-of-sight companion with Mizar and Alcor (with a spectral type similar to the latter), it is roughly four times more distant. It has the spectral type A8/F0 III.[3]
The star is six times more luminous than the Sun, 1.6 times its radius, and has an surface temperature of 7,167 K. It has exhausted its core hydrogen and evolved away from the main sequence.
References
- ^ a b c d e f g h Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27. Bibcode:2000A&A...355L..27H.
- ^ a b c Grenier, S.; Baylac, M.-O.; Rolland, L.; Burnage, R.; Arenou, F.; Briot, D.; Delmas, F.; Duflot, M.; Genty, V.; Gómez, A. E.; Halbwachs, J.-L.; Marouard, M.; Oblak, E.; Sellier, A. (1999). "Radial velocities. Measurements of 2800 B2-F5 stars for HIPPARCOS" (PDF). Astronomy and Astrophysics Supplement. 137 (3): 451. Bibcode:1999A&AS..137..451G. doi:10.1051/aas:1999489.
