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27 relations: Apparent magnitude, Cambridge, Massachusetts, Constellation, Cygnus (constellation), Earth, Exoplanet, Field of view, Gliese 436 b, HAT-P-11, HAT-P-7b, HATNet Project, Hot Neptune, Kepler (spacecraft), Methods of detecting exoplanets, Molecule, MSN, NASA, Saturn, Solar System, Star, Stellar classification, Transit (astronomy), True mass, University of St Andrews, Water vapor, 51 Pegasi, 51 Pegasi b.
Apparent magnitude
The apparent magnitude of a celestial object is a number that is a measure of its brightness as seen by an observer on Earth.
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Cambridge, Massachusetts
Cambridge is a city in Middlesex County, Massachusetts, and part of the Boston metropolitan area.
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Constellation
A constellation is a group of stars that are considered to form imaginary outlines or meaningful patterns on the celestial sphere, typically representing animals, mythological people or gods, mythological creatures, or manufactured devices.
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Cygnus (constellation)
Cygnus is a northern constellation lying on the plane of the Milky Way, deriving its name from the Latinized Greek word for swan.
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Earth
Earth is the third planet from the Sun and the only astronomical object known to harbor life.
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Exoplanet
An exoplanet or extrasolar planet is a planet outside our solar system.
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Field of view
The field of view is the extent of the observable world that is seen at any given moment.
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Gliese 436 b
Gliese 436 b (sometimes called GJ 436 b) is a Neptune-sized exoplanet orbiting the red dwarf Gliese 436.
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HAT-P-11
HAT-P-11, also designated GSC 03561-02092, is an orange dwarf metal rich star about 124 light-years away in the constellation Cygnus.
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HAT-P-7b
No description.
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HATNet Project
The Hungarian Automated Telescope Network (HATNet) project is a network of six small fully automated "HAT" telescopes.
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Hot Neptune
A hot Neptune or Hoptune is a type of giant planet with a mass similar to that of Uranus or Neptune orbiting close to its star, normally within less than 1 AU.
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Kepler (spacecraft)
Kepler is a space observatory launched by NASA to discover Earth-size planets orbiting other stars.
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Methods of detecting exoplanets
Any planet is an extremely faint light source compared to its parent star.
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Molecule
A molecule is an electrically neutral group of two or more atoms held together by chemical bonds.
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MSN
MSN (stylized as msn) is a web portal and related collection of Internet services and apps for Windows and mobile devices, provided by Microsoft and launched on August 24, 1995, the same release date as Windows 95.
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NASA
The National Aeronautics and Space Administration (NASA) is an independent agency of the executive branch of the United States federal government responsible for the civilian space program, as well as aeronautics and aerospace research.
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Saturn
Saturn is the sixth planet from the Sun and the second-largest in the Solar System, after Jupiter.
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Solar System
The Solar SystemCapitalization of the name varies.
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Star
A star is type of astronomical object consisting of a luminous spheroid of plasma held together by its own gravity.
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Stellar classification
In astronomy, stellar classification is the classification of stars based on their spectral characteristics.
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Transit (astronomy)
In astronomy, a transit or astronomical transit is the phenomenon of at least one celestial body appearing to move across the face of another celestial body, hiding a small part of it, as seen by an observer at some particular vantage point.
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True mass
The term true mass is synonymous with the term mass, but is used in astronomy to differentiate the measured mass of a planet from the lower limit of mass usually obtained from radial velocity techniques.
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University of St Andrews
The University of St Andrews (informally known as St Andrews University or simply St Andrews; abbreviated as St And, from the Latin Sancti Andreae, in post-nominals) is a British public research university in St Andrews, Fife, Scotland.
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Water vapor
No description.
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51 Pegasi
51 Pegasi (abbreviated 51 Peg), also named Helvetios, is a Sun-like star located from Earth in the constellation of Pegasus.
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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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References
[1] https://en.wikipedia.org/wiki/HAT-P-11b
