13 Boötis

13 Boötis

File:CFBooLightCurve.png A light curve for CF Boötis, plotted from Hipparcos data
Observation data Epoch J2000      Equinox J2000
Constellation	Boötes
Right ascension	Template:RA
Declination	Template:DEC
Apparent magnitude (V)	5.29 to 5.38
Characteristics
Evolutionary stage	AGB
Spectral type	M1.5III
U−B Template:Engvar	+1.92
B−V Template:Engvar
Variable type	Lb
Astrometry
Radial velocity (Rv)	km/s
Proper motion (μ)	RA: −58.584 mas/yr Dec.: 59.801 mas/yr
Parallax (π)	4.6635±0.1756 mas
Distance	Template:Rnd ± Template:Rnd ly (Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)	−0.87
Details
Mass	0.8-2.6 Template:Solar mass
Radius	Template:Solar radius
Luminosity	Template:Solar luminosity
Temperature	K
Metallicity [Fe/H]	{{{metal_fe2}}} dex
Other designations
Template:Odlist
Database references
SIMBAD	data

13 Boötis is a solitary variable star in the northern constellation of Boötes, and is positioned near the western constellation border with Ursa Major. In 1977 it was given the variable star designation CF Boötis, often abbreviated CF Boo, while 13 Boötis is the star's Flamsteed designation. This star has a reddish hue and is faintly visible to the naked eye with an apparent visual magnitude that fluctuates around 5.26. It is located at a distance of approximately 700 light years from the Sun based on parallax, but is drifting closer with a radial velocity of −14 km/s.

The variability of the brightness of 13 Boötis was announced by Joel Stebbins and Charles Morse Huffer in 1928, based on observations made at Washburn Observatory. This is an aging red giant star on the asymptotic giant branch with a stellar classification of M1.5III, which is interpreted by stellar evolutionary models to mean it has exhausted the supply of hydrogen at its core then cooled and expanded off the main sequence. It is classified as a slow irregular variable of the Lb type, and its brightness has been observed to vary from +5.29 down to +5.38. The star has ~74 times the girth of the Sun and is radiating 1,114 times the Sun's luminosity from its swollen photosphere at an effective temperature of 3,889 K.

There is a magnitude 11.05 visual companion located at an angular separation of from the brighter star, along a position angle of 270°. This was first reported by William Herschel in 1783.

Possible planetary system

In 1991, Duquennoy & Mayor reported the possible presence of a low-mass object (of likely substellar nature) orbiting the red giant 13 Bootis. They set a minimum mass of 30 times that of Jupiter (likely a brown dwarf) and estimated an orbital period of 1.35 years. So far there has been no confirmation about the presence a substellar object.

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External links

• HR 5300
• CCDM J14082+4927
• Image 13 Boötis
• [1]
• [2]