Lambda Cancri
Template:Location mark Location of Piautos (circled) | |
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Cancer |
| Right ascension | Template:RA[1] |
| Declination | Template:DEC[1] |
| Apparent magnitude (V) | +5.93[2] |
| Characteristics | |
| Spectral type | B9.5 V[3][2] |
| Astrometry | |
| Radial velocity (Rv) | Template:Val[4] km/s |
| Proper motion (μ) | RA: −20.29[1] mas/yr Dec.: −18.81[1] mas/yr |
| Parallax (π) | 5.9490±0.1482 mas[5] |
| Distance | Template:Rnd ± Template:Rnd ly (Template:Rnd ± Template:Rnd pc) |
| Absolute magnitude (MV) | +0.19[6] |
| Details[2] | |
| λ Cnc A | |
| Mass | Template:Val Template:Solar mass |
| Luminosity | 78[7] Template:Solar luminosity |
| Surface gravity (log g) | Template:Val cgs |
| Temperature | Template:Val K |
| Rotational velocity (v sin i) | 188[8] km/s |
| Age | Template:Val Myr |
| λ Cnc B | |
| Mass | 0.8 Template:Solar mass |
| Temperature | Template:Val K |
| Metallicity [Fe/H] | −0.5 dex |
| Rotational velocity (v sin i) | 10 km/s |
| Other designations | |
| Piautos, Template:Odlist[9] | |
| Database references | |
| SIMBAD | data |
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Lambda Cancri (λ Cancri, abbreviated Lambda Cnc, λ Cnc) is a blue-white-hued spectroscopic binary star[2] in the zodiac constellation of Cancer. With a combined apparent visual magnitude of +5.93, it is faintly visible to the naked eye.[2] Based upon parallax measurements obtained during the Gaia mission, it is about 550 light-years distant from the Sun.[5]
The two components are designated Lambda Cancri A (formally named Piautos Template:IPAc-en)[10] and B.
Nomenclature
λ Cancri (Latinised to Lambda Cancri) is the binary's Bayer designation. The designations of the two components as Lambda Cancri A and B derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU).[11]
The system occurs in the lunar station that was given the name πιαυτος piautos in a Coptic manuscript list of lunar stations, nearly all of which were in "debased" Greek. Walter Crum was of the opinion that Piautos is formed from the Greek word autos "self" and the Coptic determiner pi- "that", which is automatically tacked onto Greek nouns. The combination would (in Greek) mean "the same, the very one". Given that the Greeks are not known to have used lunar stations, the origin of the names is unknown.[12]
In 2016, the IAU organized a Working Group on Star Names (WGSN)[13] to catalog and standardize proper names for stars. The WGSN approved the name Piautos for Lambda Cancri on 1 June 2018 and it is now so included in the List of IAU-approved Star Names.[10] The WGSN had previously stated that where a component letter (from e.g. Washington Double Star Catalog) is not explicitly listed, that the name should be understood to be attributed to the brightest component by visual brightness[14] (Lambda Cancri A in this case).
In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Beacon Fire, refers to an asterism consisting of Lambda Cancri and Psi, Phi1 and 15 Cancri.[15] Consequently, Lambda Cancri itself is known as Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx).[16] From this Chinese name, the name Kwan Wei meaning "the bright fire" was given.[17]
Properties
The primary, Lambda Cancri A, is a B-type main-sequence star with a stellar classification of B9.5 V.[3] It has 2.1[2] times the mass of the Sun and radiates 78[7] times the Sun's luminosity from its photosphere at an effective temperature of roughly Template:Val.[2] Its close companion, Lambda Cancri B, has 80% of the mass of the Sun.[2]
References
- ↑ a b c d Cite error: Invalid
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- ↑ Script error: No such module "citation/CS1".
- ↑ See station 10 in footnote 12 in Stefan Weinstock, "Lunar Mansions and Early Calendars", Journal of Hellenic Studies, Volume 69, November 1949, pp. 48-69.
- ↑ Script error: No such module "citation/CS1".
- ↑ Script error: No such module "citation/CS1".
- ↑ Template:In lang 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, Template:ISBN.
- ↑ Template:In lang AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 27 日 Template:Webarchive
- ↑ Cite error: Invalid
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