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HR 4796

HR 4796
Dust ring around HR 4796A (eso1417a).jpg
A dust ring encircles HR 4796's primary star
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Centaurus
Right ascension 12h 36m 01.03100s
Declination −39° 52′ 10.2270″
Apparent magnitude (V) 5.80
Characteristics
Spectral type A0 V_+ M2.5 V
B−V color index +0.01
Astrometry
Radial velocity (Rv) 9.4 km/s
Proper motion (μ) RA: –56.66 mas/yr
Dec.: –24.99 mas/yr
Parallax (π) 13.74 ± 0.33mas
Distance 237 ± 6 ly
(73 ± 2 pc)
Absolute magnitude (MV) 1.61±0.11
Details
Component A
Mass 2.18 ± 0.10 M
Radius 1.68 R
Luminosity 23 L
Surface gravity (log g) 4.43 cgs
Temperature 9,378 K
Metallicity [Fe/H] –0.03 dex
Rotational velocity (v sin i) 152 km/s
Age 8 ± 2 Myr
Component B
Mass 0.3 M
Other designations
2MASS J12360103-3952102, CCDM J12360-3952, CD-39°7717, CPD-39°5622, GC 17164, HD 109573, HIP 61498, HR 4796, SAO 203621.
Database references
SIMBAD data

HR 4796 is a binary star system in the southern constellation of Centaurus. Parallax measurements put it at a distance of 237 light-years (73 parsecs) from the Earth. The two components of this system have an angular separation of 7.7 arcseconds, which, at their estimated distance, is equivalent to a projected separation of about 560 Astronomical Units (AU), or 560 times the separation of the Earth from the Sun. The star and its ring resemble an eye, and it is sometimes known by the nickname "Sauron's Eye".

This is a young system with an estimated age of about 8 million years. The primary member A has a stellar classification of A0 V, while its smaller companion B is a red dwarf with a classification of M2.5 V. The luminosity class of 'V' indicates that both stars belong to the main sequence and are generating energy through the thermonuclear fusion of hydrogen at their cores. The primary is emitting this energy from its outer envelope at an effective temperature of about 9,378 K, which gives it the white hue characteristic of A-type stars. It has a radius about 168% of the radius of the Sun and 218% of the Sun's mass. By comparison, the secondary has only 30% of a solar mass. The abundance of elements other than hydrogen or helium, what astronomers term the star's metallicity, is similar to the proportion in the Sun.


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