Английская Википедия:EZ Aquarii
Шаблон:Short description Шаблон:Sky Шаблон:Starbox begin Шаблон:Starbox image Шаблон:Starbox observe Шаблон:Starbox character Шаблон:Starbox astrometry Шаблон:Starbox visbin Шаблон:Starbox detail Шаблон:Starbox detail Шаблон:Starbox catalog Шаблон:Starbox reference Шаблон:Starbox image Шаблон:Starbox end
EZ Aquarii is a triple star system Шаблон:Convert from the Sun in the constellation Aquarius within the Milky Way. It is also known as Luyten 789-6, Gliese 866 and LHS 68. It is a variable star showing flares as well as smaller brightness changes due to rotation. The aggregate mass of the system is 0.3262±0.0018 solar masses.[1] All three seem to have masses close to the hydrogen burning mass limit.[2]
The configuration of the inner binary pair may permit a circumbinary planet to orbit near their habitable zone, however no exoplanets have yet been observed.[3] EZ Aquarii is approaching the Solar System and, in about 32,300 years, will be at its minimal distance of about Шаблон:Convert from the Sun.[4] The ChView simulation shows that currently its nearest neighbouring star is Lacaille 9352 at about Шаблон:Convert from EZ Aquarii. Шаблон:TOC limit
System
All three components are M-type red dwarfs. The pair EZ Aquarii AC form a spectroscopic binary with a 3.8-day orbit and a 0.03 AU separation. This pair share an orbit with EZ Aquarii B that has an 823-day period.[6] The A and B components of Luyten 789-6 together emit X-rays.[7]
EZ Aquarii A
This star is a red dwarf of type M5V[8] which has a mass of Шаблон:Val solar masses.[1] It has a parallax of Шаблон:Val.[9] Its period in days around EZ Aquarii C is Шаблон:Val with an eccentricity of 0 which together make up the primary of the system.[9] It has an absolute magnitude at wavelengths centered at 5500 Angstroms of 15.33 making it the brightest of the three.[8] Some alternate designations for it are EZ Aqr, GL 866A, L 789-6 A and LHS 68.
EZ Aquarii B
There is less known about this star compared to A. Its type is likely a type MV[8] with a mass of Шаблон:Val solar masses.[1] It orbits the AC system with a period of Шаблон:Val at an eccentricity of Шаблон:Val.[9] It has an absolute magnitude of 15.58, making it dimmer than A but brighter than C.[8] Some alternate designations for it are GL 866B and L 789-6 B.
EZ Aquarii C
Like the other two, this star is likely a type MV[8] with a mass of Шаблон:Val solar masses.[1] It orbits A in a period of Шаблон:Val with a nearly circular orbit.[9] It is the dimmest of the three with an absolute magnitude of 17.37.[8] An alternate designation for it is GL 866C.
Other details
The high proper motion of EZ Aquarii may have been discovered by Willem Jacob Luyten with his automated photographic plate scanner.[10]
See also
References
External links
- Image EZ Aquarii
- Solstation provides an orbital animation as well as a visualization of the habitable zone around EZ Aquarii B.
Шаблон:Nearest systems Шаблон:Stars of Aquarius
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