46 relations: Apparent magnitude, Astronomical unit, Coplanarity, Cygnus (constellation), Day, Degree (angle), Density, Earth, Earth mass, Earth radius, Gliese 581, HD 10180, Helium, Hydrogen, Kelvin, Kepler (spacecraft), Kepler Input Catalog, Kepler object of interest, Kepler-11b, Kepler-11c, Kepler-11d, Kepler-11e, Kepler-11f, Kepler-11g, List of multiplanetary systems, Mass, Mercury (planet), Methods of detecting exoplanets, NASA, Neptune, Orbital eccentricity, Orbital inclination, Orbital period, Orbital resonance, Planet, Planetary migration, Protoplanetary disk, Radius, Scientific American, Semi-major and semi-minor axes, Solar analog, Solar System, Steam, Sun, Transit (astronomy), 55 Cancri.
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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Astronomical unit
The astronomical unit (symbol: au, ua, or AU) is a unit of length, roughly the distance from Earth to the Sun.
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Coplanarity
In geometry, a set of points in space are coplanar if there exists a geometric plane that contains them all.
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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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Day
A day, a unit of time, is approximately the period of time during which the Earth completes one rotation with respect to the Sun (solar day).
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Degree (angle)
A degree (in full, a degree of arc, arc degree, or arcdegree), usually denoted by ° (the degree symbol), is a measurement of a plane angle, defined so that a full rotation is 360 degrees.
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Density
The density, or more precisely, the volumetric mass density, of a substance is its mass per unit volume.
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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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Earth mass
Earth mass (where ⊕ is the standard astronomical symbol for planet Earth) is the unit of mass equal to that of Earth.
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Earth radius
Earth radius is the approximate distance from Earth's center to its surface, about.
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Gliese 581
Gliese 581 is a star of spectral type M3V (a red dwarf) at the center of the Gliese 581 planetary system, about 20 light years away from Earth in the Libra constellation.
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HD 10180
HD 10180 is a Sun-like star in the southern constellation Hydrus that is notable for its large planetary system.
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Helium
Helium (from lit) is a chemical element with symbol He and atomic number 2.
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Hydrogen
Hydrogen is a chemical element with symbol H and atomic number 1.
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Kelvin
The Kelvin scale is an absolute thermodynamic temperature scale using as its null point absolute zero, the temperature at which all thermal motion ceases in the classical description of thermodynamics.
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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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Kepler Input Catalog
The Kepler Input Catalog (or KIC) is a publicly searchable database of roughly 13.2 million targets used for the Kepler Spectral Classification Program (SCP) and Kepler.
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Kepler object of interest
A Kepler object of interest (KOI) is a star observed by the Kepler spacecraft that is suspected of hosting one or more transiting planets.
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Kepler-11b
Kepler-11b is an exoplanet discovered around the star Kepler-11 by the Kepler spacecraft, a NASA-led mission to discover Earth-like planets.
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Kepler-11c
Kepler-11c is an exoplanet discovered in the orbit of the Sun-like star Kepler-11 by the Kepler spacecraft, a NASA telescope aiming to discover Earth-like planets.
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Kepler-11d
Kepler-11d is an exoplanet discovered in the orbit of the sun-like star Kepler-11.
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Kepler-11e
Kepler-11e is an exoplanet (extrasolar planet) discovered in the orbit of the sunlike star Kepler-11.
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Kepler-11f
Kepler-11f is an exoplanet (extrasolar planet) discovered in the orbit of the sun-like star Kepler-11 by NASA's Kepler spacecraft, which searches for planets that transit (cross in front of) their host stars.
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Kepler-11g
Kepler-11g is an exoplanet discovered in the orbit of the sunlike star Kepler-11 by the Kepler spacecraft, a NASA satellite tasked with searching for terrestrial planets.
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List of multiplanetary systems
From the total of stars known to have exoplanets (as of), there are a total of known multiplanetary systems, or stars with at least two confirmed planets, beyond the Solar System.
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Mass
Mass is both a property of a physical body and a measure of its resistance to acceleration (a change in its state of motion) when a net force is applied.
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Mercury (planet)
Mercury is the smallest and innermost planet in the Solar System.
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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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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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Neptune
Neptune is the eighth and farthest known planet from the Sun in the Solar System.
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Orbital eccentricity
The orbital eccentricity of an astronomical object is a parameter that determines the amount by which its orbit around another body deviates from a perfect circle.
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Orbital inclination
Orbital inclination measures the tilt of an object's orbit around a celestial body.
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Orbital period
The orbital period is the time a given astronomical object takes to complete one orbit around another object, and applies in astronomy usually to planets or asteroids orbiting the Sun, moons orbiting planets, exoplanets orbiting other stars, or binary stars.
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Orbital resonance
In celestial mechanics, an orbital resonance occurs when orbiting bodies exert a regular, periodic gravitational influence on each other, usually because their orbital periods are related by a ratio of small integers.
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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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Planetary migration
Planetary migration occurs when a planet or other stellar satellite interacts with a disk of gas or planetesimals, resulting in the alteration of the satellite's orbital parameters, especially its semi-major axis.
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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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Radius
In classical geometry, a radius of a circle or sphere is any of the line segments from its center to its perimeter, and in more modern usage, it is also their length.
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Scientific American
Scientific American (informally abbreviated SciAm) is an American popular science magazine.
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Semi-major and semi-minor axes
In geometry, the major axis of an ellipse is its longest diameter: a line segment that runs through the center and both foci, with ends at the widest points of the perimeter.
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Solar analog
Solar-type star, solar analogs (also analogues), and solar twins are stars that are particularly similar to the Sun.
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Solar System
The Solar SystemCapitalization of the name varies.
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Steam
Steam is water in the gas phase, which is formed when water boils.
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Sun
The Sun is the star at the center of the Solar System.
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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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55 Cancri
55 Cancri (abbreviated 55 Cnc) is a binary star approximately 41 light-years away from the Sun in the constellation of Cancer.
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References
[1] https://en.wikipedia.org/wiki/Kepler-11