RR Caeli

RR Caeli

A white light light curve for RR Caeli, adapted from Maxted et al. (2007)[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Caelum
Right ascension 04h 21m 05.563s[2]
Declination −48° 39′ 07.06″[2]
Apparent magnitude (V) 14.40[3]
Characteristics
Evolutionary stage White dwarf + red dwarf
Spectral type DA7.8 + M4[4]
U−B color index −0.42 [3]
B−V color index 0.52[3]
Variable type Algol[5]
Astrometry
Proper motion (μ) RA: 30.030[2] mas/yr
Dec.: −533.886[2] mas/yr
Parallax (π)47.2 ± 0.02 mas[2]
Distance69.10 ± 0.03 ly
(21.186 ± 0.009 pc)
Orbit[4]
Period (P)7.289 h
Semi-major axis (a)1.46 R
Eccentricity (e)0
Inclination (i)87.9°
Semi-amplitude (K1)
(primary)
48 km/s
Semi-amplitude (K2)
(secondary)
196 km/s
Details[1]
White dwarf
Mass0.453±0.002[6] M
Radius0.01568±0.00009[4] R
Luminosity (bolometric)0.0007 ± 0.00015[note 1] L
Surface gravity (log g)(7.67–7.72) ± 0.06 cgs
Temperature7540 ± 175 K
Red dwarf
Mass0.168±0.001[6] M
Radius(0.203–0.215) ± 0.015 R
Luminosity (bolometric)0.0038 ± 0.0013[note 1] L
Surface gravity (log g)(5.04–5.09) ± 0.04 cgs
Temperature3100 ± 113 K
Other designations
RR Caeli, LFT 349, WD 0419-487, GJ 2034, 2MASS J04210556-4839070, GSC 08072-01454, Gaia DR3 4788741548375134336[7]
Database references
SIMBADdata
Exoplanet Archivedata
ARICNSdata

RR Caeli is an eclipsing binary star system, located 69 light-years from Earth in the constellation Caelum. It is made up of a red dwarf star and a white dwarf, which complete an orbit around each other every seven hours. There is evidence of two circumbinary planets orbiting even further away.

  1. ^ a b Cite error: The named reference Maxted was invoked but never defined (see the help page).
  2. ^ a b c d e Cite error: The named reference dr3 was invoked but never defined (see the help page).
  3. ^ a b c Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. Bibcode:1986EgUBV........0M.
  4. ^ a b c Cite error: The named reference Parsons2017 was invoked but never defined (see the help page).
  5. ^ Samus', N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (2017). "General catalogue of variable stars: Version GCVS 5.1". Astronomy Reports. 61 (1): 80. Bibcode:2017ARep...61...80S. doi:10.1134/S1063772917010085. S2CID 125853869.
  6. ^ a b Cite error: The named reference Rattanamala2021 was invoked but never defined (see the help page).
  7. ^ "V* RR Caeli – Eclipsing binary of Algol type (detached)". SIMBAD. Retrieved 18 February 2013.


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