CT Chamaeleontis

CT Chamaeleontis
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Chamaeleon
Right ascension 11h 04m 09.131s[1]
Declination −76° 27 19.30[1]
Apparent magnitude (V) 12.31 to 12.43[2]
Characteristics
Spectral type K7[1]
B−V color index −0.9[1]
V−R color index 0.8[1]
Variable type INB[2]
Astrometry
Radial velocity (Rv)15.1 ± 0.5[1] km/s
Proper motion (μ) RA: −21.3 ± 4.6[3] mas/yr
Dec.: 6.3 ± 4.5[3] mas/yr
Distance540 ± 100 ly
(165 ± 30[3] pc)
Details
Age0 to 4 × 106 [3] years
Other designations
CT Cha.
Database references
SIMBADdata
CT Chamaeleontis b

A size comparison between the colossal planet CT Chamaeleontis b and Jupiter.
Position (relative to CT Chamaleontis)
Epoch of observation2006–2007
Angular distance2.670 [3]
Position angle300.7° [3]
Observed separation
(projected)
~440 AU [3]
Characteristics
Spectral type M8–L0[3]
Details
Mass0.016 ± 0.006[3] M
Radius0.23+0.08
0.06
[3] R
Luminosity0.002[3] L
Surface gravity (log g)3.5[3] cgs
Temperature2600 ± 250[3] K
Age0 to 4 × 106 [3] years
Other designations
CT Cha b.
Database references
SIMBADdata

CT Chamaeleontis (CT Cha) is a T Tauri star in the constellation of Chamaeleon.[1] It has an apparent visual magnitude which varies between 12.31 and 12.43.[2]

In 2006 and 2007, a faint companion was observed 2.7 arcseconds away from CT Chamaeleontis, using the Very Large Telescope at the European Southern Observatory. Since the object shares common proper motion with CT Chamaleontis, it is believed to be physically close to the star, with a projected separation of approximately 440 astronomical units. It is estimated to have a mass of approximately 17 Jupiter masses and is probably a brown dwarf or a planet.[3] The companion has been designated CT Chamaeleontis b.[4]

References

  1. 1 2 3 4 5 6 7 V* CT Cha -- T Tau-type Star, database entry, SIMBAD. Accessed on line October 1, 2008.
  2. 1 2 3 CT Cha, database entry, The combined table of GCVS Vols I-III and NL 67-78 with improved coordinates, General Catalogue of Variable Stars, Sternberg Astronomical Institute, Moscow, Russia. Accessed on line October 1, 2008.
  3. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 Direct evidence of a sub-stellar companion around CT Cha, T. O. B. Schmidt et al., accepted for publication in Astronomy and Astrophysics, Bibcode: 2008arXiv0809.2812S, arXiv:0809.2812.
  4. NAME CT Cha b -- Extra-solar Planet Candidate, database entry, SIMBAD. Accessed on line October 1, 2008.


This article is issued from Wikipedia - version of the 7/4/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.