27 Cancri
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Cancer |
| Right ascension | Template:RA[2] |
| Declination | Template:DEC[2] |
| Apparent magnitude (V) | +5.56[3] |
| Characteristics | |
| Evolutionary stage | Asymptotic giant branch[4] |
| Spectral type | M3 IIIa[5] |
| B−V Template:Engvar | Script error: No such module "val".[3] |
| Variable type | SRb[4] |
| Astrometry | |
| Radial velocity (Rv) | Script error: No such module "val".[6] km/s |
| Proper motion (μ) | RA: −19.760[2] mas/yr Dec.: −104.664[2] mas/yr |
| Parallax (π) | 3.3094±0.3176 mas[2] |
| Distance | Template:Rnd ± Template:Rnd ly (Template:Rnd ± Template:Rnd pc) |
| Absolute magnitude (MV) | −1.62[3] |
| Details | |
| Radius | 119[2] Template:Solar radius |
| Luminosity | Script error: No such module "val".[7] Template:Solar luminosity |
| Surface gravity (log g) | 1.00[7] cgs |
| Temperature | 3,574[7] K |
| Metallicity [Fe/H] | 0.00[7] dex |
| Metallicity [Fe/H] | {{{metal_fe2}}} dex |
| Other designations | |
| Template:Odlist[8] | |
| Database references | |
| SIMBAD | data |
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27 Cancri is a single[9] star in the zodiac constellation of Cancer, located around 990 light-years away from the Sun.[2] It is visible to the naked eye as a faint, red-hued star with a typical apparent visual magnitude of around +5.56.[3] The star is moving closer to the Earth with a heliocentric radial velocity of −8.3 km/s.[6] It is a member of the Arcturus stream, a group of stars with high proper motion and metal-poor properties thought to be the remnants of a small galaxy consumed by the Milky Way.[10]
The variability of the brightness of 27 Cancri was announced by Joel Stebbins and Charles Morse Huffer in 1928, based on observations made at Washburn Observatory.[11] It was given its variable star designation, BP Cancri, in 1977.[12]
This is an aging red giant with a stellar classification of M3 IIIa,[5] currently on the asymptotic giant branch.[4] It is classified as a semiregular variable star of type SRb and its brightness varies from magnitude +5.41 to +5.75 with a period of 40 days.[13] The star is radiating around 2,455[7] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 3,574 K.[7]
References
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- ↑ a b c d e f g Template:Cite Gaia DR2
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- ↑ Template:Cite simbad
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- ↑ Script error: No such module "citation/CS1".
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- Pages with script errors
- Pages with broken file links
- M-type giants
- Semiregular variable stars
- Asymptotic-giant-branch stars
- Arcturus moving group
- Cancer (constellation)
- Durchmusterung objects
- Flamsteed objects
- Henry Draper Catalogue objects
- Hipparcos objects
- Bright Star Catalogue objects
- Objects with variable star designations