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47 relations: Astronomy & Astrophysics, Beta Pictoris b, Brown dwarf, Cha 110913-773444, CT Chamaeleontis, Exoplanet, Geometric albedo, GQ Lupi b, HAT-P-32b, HAT-P-33b, HD 100546, HD 209458 b, Hot Jupiter, HR 2562 b, Jupiter, Jupiter radius, KELT-9b, Kepler-12b, Kepler-13, Kepler-39b, Kepler-7b, List of galaxies, List of gravitationally rounded objects of the Solar System, List of largest cosmic structures, List of largest nebulae, List of largest stars, Main sequence, NASA Exoplanet Archive, OTS 44, Planet, Protoplanetary disk, PSO J318.5-22, Rogue planet, ROXs 42Bb, Solar System, Sub-brown dwarf, Sun, TrES-2b, TrES-4b, WASP-121b, WASP-12b, WASP-17b, WASP-79b, XO-6b, Year, 1RXS J160929.1−210524, 51 Pegasi b.
Astronomy & Astrophysics
Astronomy & Astrophysics is a peer-reviewed scientific journal covering theoretical, observational, and instrumental astronomy and astrophysics.
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Beta Pictoris b
Beta Pictoris b (also abbreviated as β Pic b) is an exoplanet orbiting the young debris disk A-type main sequence star Beta Pictoris located approximately 63 light-years (19.4 parsecs, or nearly km) away from Earth in the constellation of Pictor.
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Brown dwarf
Brown dwarfs are substellar objects that occupy the mass range between the heaviest gas giant planets and the lightest stars, having masses between approximately 13 to 75–80 times that of Jupiter, or approximately to about.
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Cha 110913-773444
Cha 110913-773444 (sometimes abbreviated Cha 110913) is an astronomical object surrounded by what appears to be a protoplanetary disk.
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CT Chamaeleontis
CT Chamaeleontis (CT Cha) is a T Tauri star in the constellation of Chamaeleon.
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Exoplanet
An exoplanet or extrasolar planet is a planet outside our solar system.
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Geometric albedo
In astronomy, the geometric albedo of a celestial body is the ratio of its actual brightness as seen from the light source (i.e. at zero phase angle) to that of an idealized flat, fully reflecting, diffusively scattering (Lambertian) disk with the same cross-section.
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GQ Lupi b
GQ Lupi b is a possible extrasolar planet or brown dwarf orbiting the star GQ Lupi.
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HAT-P-32b
HAT-P-32b is a planet in the orbit of the G-type or F-type star HAT-P-32, which is approximately 860 light years away from Earth.
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HAT-P-33b
HAT-P-33b is a planet in the orbit of HAT-P-33, which lies 1,400 light years away from Earth.
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HD 100546
HD 100546, also known as KR Muscae, is a star 320 light-years from Earth.
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HD 209458 b
HD 209458 b, also given the nickname Osiris,http://exoplanets.co/exoplanets-tutorial/extrasolar-planet-hd-209458-b.html is an exoplanet that orbits the solar analog HD 209458 in the constellation Pegasus, some 159 light-years from the Solar System.
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Hot Jupiter
Hot Jupiters are a class of gas giant exoplanets that are inferred to be physically similar to Jupiter but that have very short orbital period (P The close proximity to their stars and high surface-atmosphere temperatures resulted in the moniker "hot Jupiters". Hot Jupiters are the easiest extrasolar planets to detect via the radial-velocity method, because the oscillations they induce in their parent stars' motion are relatively large and rapid compared to those of other known types of planets. One of the best-known hot Jupiters is 51 Pegasi b. Discovered in 1995, it was the first extrasolar planet found orbiting a Sun-like star. 51 Pegasi b has an orbital period of about 4 days.
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HR 2562 b
HR 2526b is a substellar companion of debris disk host star HR 2562.
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Jupiter
Jupiter is the fifth planet from the Sun and the largest in the Solar System.
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Jupiter radius
Jupiter radius or Jovian radius is the distance equal to the radius of planet Jupiter.
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KELT-9b
KELT-9b is the hottest gas giant exoplanet known, with a dayside temperature of between 4,050 and 4,600 K, which makes it hotter than M-type stars, and many K-type stars.
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Kepler-12b
Kepler-12b is a Hot Jupiter that orbits G-type star Kepler-12 some 900 parsecs away.
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Kepler-13
Kepler-13 or KOI-13 is a stellar triple star system consisting of Kepler-13A, around which an orbiting hot Jupiter exoplanet was discovered with the Kepler spacecraft in 2011, and Kepler-13B a common proper motion companion star which has an additional star orbiting it.
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Kepler-39b
Kepler-39b (formerly known as KOI-423b), is a confirmed extrasolar object (either a Jovian planet or brown dwarf because of its mass) discovered orbiting the F-type star Kepler-39.
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Kepler-7b
Kepler-7b is one of the first five exoplanets to be confirmed by NASA's Kepler spacecraft, and was confirmed in the first 33.5 days of Kepler's science operations.
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List of galaxies
The following is a list of notable galaxies.
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List of gravitationally rounded objects of the Solar System
This is a list of gravitationally rounded objects of the Solar System, which are objects that have a rounded, ellipsoidal shape due to the forces of their own gravity (hydrostatic equilibrium).
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List of largest cosmic structures
This is a list of the largest cosmic structures so far discovered.
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List of largest nebulae
Below is a list of the largest nebulae so far discovered, ordered by size.
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List of largest stars
Below is an ordered list of the largest stars currently known by radius.
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Main sequence
In astronomy, the main sequence is a continuous and distinctive band of stars that appear on plots of stellar color versus brightness.
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NASA Exoplanet Archive
The NASA Exoplanet Archive is an online astronomical exoplanet catalog and data service that collects and serves public data that support the search for and characterization of extra-solar planets (exoplanets) and their host stars.
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OTS 44
OTS 44 is a free-floating planetary-mass object or brown dwarf located at in the constellation Chamaeleon.
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Planet
A planet is an astronomical body orbiting a star or stellar remnant that is massive enough to be rounded by its own gravity, is not massive enough to cause thermonuclear fusion, and has cleared its neighbouring region of planetesimals.
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Protoplanetary disk
A protoplanetary disk is a rotating circumstellar disk of dense gas and dust surrounding a young newly formed star, a T Tauri star, or Herbig Ae/Be star.
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PSO J318.5-22
PSO J318.5-22 is a rogue planet, an extrasolar object of planetary mass that does not appear to have a host star.
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Rogue planet
A rogue planet (also termed an interstellar planet, nomad planet, free-floating planet, orphan planet, wandering planet, starless planet, or sunless planet) is a planetary-mass object that orbits a galactic center directly.
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ROXs 42Bb
ROXs 42Bb is a directly imaged planetary-mass companion to the binary M star ROXs 42B, a likely member of the Rho Ophiuchi cloud complex.
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Solar System
The Solar SystemCapitalization of the name varies.
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Sub-brown dwarf
A sub-brown dwarf or planetary-mass brown dwarf is an astronomical object that formed in the same manner as stars and brown dwarfs (i.e. through the collapse of a gas cloud) but that has a mass below the limiting mass for thermonuclear fusion of deuterium (about). Some researchers call them free-floating planets whereas others call them planetary-mass brown dwarfs.
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Sun
The Sun is the star at the center of the Solar System.
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TrES-2b
TrES-2b (TrES-2 or Kepler-1b) is an extrasolar planet orbiting the star GSC 03549-02811 located 750 light years away from the Solar System.
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TrES-4b
TrES-4b is an extrasolar planet, and one of the largest exoplanets ever found, after WASP-12b, WASP-17b, CT Chamaeleontis b (though the latter may be a brown dwarf) and GQ Lupi b. It was discovered in 2006, and announced in 2007, by the Trans-Atlantic Exoplanet Survey, using the transit method.
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WASP-121b
WASP-121b is an extrasolar planet orbiting the star WASP-121.
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WASP-12b
WASP-12b is an extrasolar planet orbiting the star WASP-12, discovered by the SuperWASP planetary transit survey.
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WASP-17b
WASP-17b is an exoplanet in the constellation Scorpius that is orbiting the star WASP-17.
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WASP-79b
WASP-79b is an extrasolar planet orbiting the star CD-30 1812.
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XO-6b
XO-6b is a transiting exoplanet orbiting the star XO-6 around 760 Light Years (230 Parsecs) away from Earth.
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Year
A year is the orbital period of the Earth moving in its orbit around the Sun.
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1RXS J160929.1−210524
1RXS J160929.1-210524 (also known as GSC 6213-1358 or PZ99 J160930.3-210459) is a pre-main-sequence star nearly 470 light-years away in the constellation of Scorpius.
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51 Pegasi b
51 Pegasi b (abbreviated 51 Peg b), unofficially dubbed Bellerophon, later named Dimidium, is an extrasolar planet approximately 50 light-years away in the constellation of Pegasus.
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Redirects here:
List of largest known exoplanets, List of largest planets.
References
[1] https://en.wikipedia.org/wiki/List_of_largest_exoplanets
