Andromeda (constellation)

star in the constellation Andromeda

variable star in the constellation Andromeda

star in the constellation Andromeda

variable star in the constellation Andromeda

star in the constellation Andromeda

star in the constellation Andromeda

star in the constellation Andromeda

star

binary star in the constellation Andromeda

star in the constellation Andromeda

star in the constellation Andromeda

galaxy cluster

HAT-P-6b is a transiting extrasolar planet discovered by Noyes et al. on October 15, 2007. It is located approximately 910 light-years away in the constellation of Andromeda, orbiting the star HAT-P-6. This hot Jupiter planet orbits with a semi-major axis of about 0.05 AU, and takes 92 hours, 28 minutes, 17 seconds to orbit the star. It has true mass of 5.7% greater than Jupiter and a radius 33% greater than Jupiter, corresponding to a density of 0.583 g/cm3, which is less than water.

binary star in the constellation Andromeda

star in the constellation Andromeda

star in the constellation Andromeda

group of galaxies

star in the constellation Andromeda

star in the constellation Andromeda

star in the constellation Andromeda

star in the constellation Andromeda

M-type giant star in the constellation Andromeda

star in the constellation Andromeda

dwarf spheroidal galaxy

binary star system in the constellation Andromeda

HAT-P-6, also named Sterrennacht is a star in the constellation Andromeda, located approximately 895 light years or 274 parsecs away from the Earth. It is an F-type star, implying that it is hotter and more massive than the Sun. The apparent magnitude of the star is +10.54, which means that it can only be visible through the telescope. The absolute magnitude of +3.36 is brighter than the Sun's +4.83, meaning that the star itself is brighter than the Sun. A search for a binary companion star using adaptive optics at the MMT Observatory turned out negative.

star in the constellation Andromeda

galaxy in constellation Andromeda

star in the constellation Andromeda

star in the constellation Andromeda

star in the constellation Andromeda

star in the constellation Andromeda

star in the constellation Andromeda

binary star system in the constellation Andromeda

satellite galaxy of the Andromeda galaxy

star in the constellation Andromeda

star in the constellation Andromeda

M31-RV is a possible red cataclysmic variable star located in the Andromeda Galaxy (M31) that experienced an outburst in 1988, which was similar to the outburst V838 Monocerotis experienced in 2002. At peak brightness, M31-RV was the most luminous red supergiant in the Local Group. Such objects have been called luminous red novae or intermediate-luminosity red transients. During the outburst, both V838 Mon and M31-RV reached a maximum absolute visual magnitude of -9.8.

star in the constellation Andromeda

star in the constellation Andromeda

galaxy in constellation Andromeda

variable star in the constellation Andromeda

extrasolar planet

star in the constellation Andromeda

star in the constellation Andromeda

binary star system in the constellation Andromeda

star in the constellation Andromeda

star in the constellation Andromeda

star in the constellation Andromeda

star in the constellation Andromeda

former constellation

star in the constellation Andromeda

variable star in the constellation Andromeda

star in the constellation Andromeda

star in the constellation Andromeda

galaxy in constellation Andromeda

variable star in the constellation Andromeda

star in the constellation Andromeda

variable star in the constellation Andromeda

star in the constellation Andromeda