Triple star systems

star

Star in the constellation Draco

star in the constellation Pegasus

star in the constellation Eridanus

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star in the constellation Andromeda

Star in the constellation Draco

probable triple star system in the constellation of Lupus

star in the constellation Serpens

star in the constellation Circinus

star system in the constellation Indus

ternary star system in the constellation Cepheus

star system in the constellation Vulpecula

star in the constellation Coma Berenices

WASP-3 is a triple star system located about away from the Sun in the constellation Lyra. The system has an apparent magnitude of 10. The brightest and most massive star of this system is WASP-3A, an F-type main sequence star which has one known transiting hot Jupiter exoplanet, WASP-3b. Since the planet transits the star, the star is classified as a planetary transit variable and has received the variable star designation V838 Lyrae.

multiple star system in the constellation Ophiuchus

star system in the constellation Cetus

Rotating variable star in the constellation Carina

star in the constellation Aquarius

star system in the constellation Gemini

star in the constellation Telescopus

star in the constellation Aquarius

star in the constellation Draco

star in the constellation Hydra

star in the constellation Cassiopeia

star in the constellation Aries

binary star

high proper-motion star in the constellation Coma Berenices

Star

multiple star system in the constellation Hydra

triple star system in the constellation Centaurus

star system in the constellation Auriga

star in the constellation Orion

HAT-P-8 is a magnitude 10 star located 700 light-years away in Pegasus. It is a F-type star about 28% more massive than the Sun. Two red dwarf companions have been detected around HAT-P-8. The first has a spectral type of M5V and has a mass of . The second is even less massive, at , and its spectral type is M6V.

Star in the constellation Norma

star system in the constellation Hydra

variable star in the constellation Musca

star in the constellation Norma

star system in the constellation Eridanus

star in the constellation Orion

star

Multiple star and astrophysical X-ray source in the constellation Aquarius

double star in the constellation Capricornus

star in the constellation Grus

2M1510 (full designation: 2MASS J15104761–2818234) is a triple or possibly quadruple system of gravitationally bound brown dwarfs, consisting of the eclipsing binary 2M1510AB and the wide companion 2M1510C. 2M1510AB was found to be an eclipsing binary in the first light data of the SPECULOOS telescopes. It is only the second eclipsing binary brown dwarf found so far (as of March 2020), the other is 2M0535-05. The system verified theoretical models for how brown dwarfs cool. The system is located 120 light-years away from Earth in the constellation Libra.

star in the constellation Gemini

star in the constellation Ursa Major

star system in the constellation Orion

star in the constellation Andromeda

star system in the constellation Corona Boeralis

star in the constellation Aquarius

triple star system in the constellation Aries

multiple star system in the constellation Cepheus

star in the constellation Boötes

star in the constellation Lupus

star in the constellation Lyra

star system in the constellation Equuleus

star in the constellation Pisces

triple star system in the constellation Phoenix

red dwarf star in the constellation Corvus