Durchmusterung objects

variable star in the constellation Triangulum Australe

star in the constellation Hercules

star

binary star in the constellation Aquarius

star in the constellation Centaurus

star in the constellation Monoceros

star in the constellation Coma Berenices

variable star in the constellation Lupus

WASP-15, also named Nyamien, is a magnitude 11 star located about 935 light-years away in the constellation Centaurus. The star, which is more massive, larger, hotter, and more luminous than the Sun, is also less metal-rich than the Sun. WASP-15 has one known planet in its orbit, WASP-15b; the planet is a hot Jupiter with an anomalously high radius, a phenomenon which may be explained by the presence of an internal heat source. The star was first observed by the SuperWASP program in 2006; future measurements in 2007 and 2008, as well as follow-up observations and analysis, eventually led to th

star in the constellation Cancer

spectroscopic binary star system in the constellation Taurus

star system in the constellation Cetus

variable star in the constellation Auriga

star in the constellation Lynx

star in the constellation Ursa Major

star in the constellation Pavo

star in the constellation Aquarius

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.

star in the constellation Cancer

star

star

star in the constellation Vela

star in the constellation Aquarius

star in the constellation Capricornus

M-type giant star in the constellation Andromeda

star in the constellation Piscis Austrinus

variable star in the constellation Orion

star in the constellation Centaurus

star in the constellation Centaurus

WASP-8 is a binary star system away. The star system is much younger than the Sun at 300 million to 1.2 billion years age, and is heavily enriched in heavy elements, having nearly twice the concentration of iron compared to the Sun.

star in the constellation Piscis Austrinus

star in the constellation Aquarius

binary star system in the constellation Andromeda

star in the constellation Cetus

binary star system in the constellation Coma Berenices

star in the constellation Triangulum Australe

star in the constellation Andromeda

star in the constellation Equuleus

star in the constellation Aries

star in the constellation Piscis Austrinus

star

star

star in the constellation Aries

star in the constellation Grus

star in the constellation Aquarius

star in the constellation Centaurus

star in the constellation Auriga

star in the constellation Andromeda

star in the constellation Columba

star in the constellation Ursa Major

star in the constellation Aquarius

star

star in the constellation Aquila

star in the constellation Boötes

star in the constellation Canes Venatici

multiple star

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binary star system in the constellation Auriga

WASP-121, also known as CD-38 3220 and formally named Dilmun, is a magnitude 10.4 star located approximately away in the constellation Puppis. WASP-121 has a mass and radius similar to the Sun's. It hosts one known exoplanet. Due to the star's strongly titled rotational axis with a stellar inclination angle of 8.1°, the planet's orbit is almost polar.

star in the constellation Aquila