Faster access than browser!Similarities between Kepler (spacecraft) and Methods of detecting exoplanets
Kepler (spacecraft) and Methods of detecting exoplanets have 48 things in common (in Unionpedia): Asteroid, Astronomical unit, Binary star, CHEOPS, Circumbinary planet, Circumstellar habitable zone, CoRoT, Cygnus (constellation), Doppler spectroscopy, Exoplanet, Gaia (spacecraft), HATNet Project, Herschel Space Observatory, High Accuracy Radial Velocity Planet Searcher, Hubble Space Telescope, Jet Propulsion Laboratory, Johannes Kepler, Jupiter, Kepler-16b, Kepler-70b, Kepler-70c, List of exoplanets, Main sequence, Methods of detecting exoplanets, Monthly Notices of the Royal Astronomical Society, Moon, NASA, Neptune, Occultation, PDF, ..., Photometry (astronomy), Planetary phase, PLATO (spacecraft), Proceedings of SPIE, Radial velocity, Red dwarf, Science (journal), Solar analog, Solar System, Space Interferometry Mission, Star, Sun, Supernova, The Astrophysical Journal, Transit (astronomy), Transiting Exoplanet Survey Satellite, White dwarf, Wide Angle Search for Planets. Expand index (18 more) »
Asteroid
Asteroids are minor planets, especially those of the inner Solar System.
Asteroid and Kepler (spacecraft) · Asteroid and Methods of detecting exoplanets ·
Astronomical unit
The astronomical unit (symbol: au, ua, or AU) is a unit of length, roughly the distance from Earth to the Sun.
Astronomical unit and Kepler (spacecraft) · Astronomical unit and Methods of detecting exoplanets ·
Binary star
A binary star is a star system consisting of two stars orbiting around their common barycenter.
Binary star and Kepler (spacecraft) · Binary star and Methods of detecting exoplanets ·
CHEOPS
CHEOPS (CHaracterising ExOPlanets Satellite) is a planned European space telescope for the study of the formation of extrasolar planets.
CHEOPS and Kepler (spacecraft) · CHEOPS and Methods of detecting exoplanets ·
Circumbinary planet
A circumbinary planet is a planet that orbits two stars instead of one.
Circumbinary planet and Kepler (spacecraft) · Circumbinary planet and Methods of detecting exoplanets ·
Circumstellar habitable zone
In astronomy and astrobiology, the circumstellar habitable zone (CHZ), or simply the habitable zone, is the range of orbits around a star within which a planetary surface can support liquid water given sufficient atmospheric pressure.
Circumstellar habitable zone and Kepler (spacecraft) · Circumstellar habitable zone and Methods of detecting exoplanets ·
CoRoT
CoRoT (French: Convection, Rotation et Transits planétaires; English: Convection, Rotation and planetary Transits) was a space observatory mission which operated from 2006 to 2013.
CoRoT and Kepler (spacecraft) · CoRoT and Methods of detecting exoplanets ·
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.
Cygnus (constellation) and Kepler (spacecraft) · Cygnus (constellation) and Methods of detecting exoplanets ·
Doppler spectroscopy
Doppler spectroscopy (also known as the radial-velocity method, or colloquially, the wobble method) is an indirect method for finding extrasolar planets and brown dwarfs from radial-velocity measurements via observation of Doppler shifts in the spectrum of the planet's parent star.
Doppler spectroscopy and Kepler (spacecraft) · Doppler spectroscopy and Methods of detecting exoplanets ·
Exoplanet
An exoplanet or extrasolar planet is a planet outside our solar system.
Exoplanet and Kepler (spacecraft) · Exoplanet and Methods of detecting exoplanets ·
Gaia (spacecraft)
Gaia is a space observatory of the European Space Agency (ESA) designed for astrometry: measuring the positions and distances of stars with unprecedented precision.
Gaia (spacecraft) and Kepler (spacecraft) · Gaia (spacecraft) and Methods of detecting exoplanets ·
HATNet Project
The Hungarian Automated Telescope Network (HATNet) project is a network of six small fully automated "HAT" telescopes.
HATNet Project and Kepler (spacecraft) · HATNet Project and Methods of detecting exoplanets ·
Herschel Space Observatory
The Herschel Space Observatory was a space observatory built and operated by the European Space Agency (ESA).
Herschel Space Observatory and Kepler (spacecraft) · Herschel Space Observatory and Methods of detecting exoplanets ·
High Accuracy Radial Velocity Planet Searcher
The High Accuracy Radial velocity Planet Searcher (HARPS) is a high-precision echelle planet finding spectrograph installed in 2002 on the ESO's 3.6m telescope at La Silla Observatory in Chile.
High Accuracy Radial Velocity Planet Searcher and Kepler (spacecraft) · High Accuracy Radial Velocity Planet Searcher and Methods of detecting exoplanets ·
Hubble Space Telescope
The Hubble Space Telescope (HST) is a space telescope that was launched into low Earth orbit in 1990 and remains in operation.
Hubble Space Telescope and Kepler (spacecraft) · Hubble Space Telescope and Methods of detecting exoplanets ·
Jet Propulsion Laboratory
The Jet Propulsion Laboratory (JPL) is a federally funded research and development center and NASA field center in Pasadena, California, United States, with large portions of the campus in La Cañada Flintridge, California.
Jet Propulsion Laboratory and Kepler (spacecraft) · Jet Propulsion Laboratory and Methods of detecting exoplanets ·
Johannes Kepler
Johannes Kepler (December 27, 1571 – November 15, 1630) was a German mathematician, astronomer, and astrologer.
Johannes Kepler and Kepler (spacecraft) · Johannes Kepler and Methods of detecting exoplanets ·
Jupiter
Jupiter is the fifth planet from the Sun and the largest in the Solar System.
Jupiter and Kepler (spacecraft) · Jupiter and Methods of detecting exoplanets ·
Kepler-16b
Kepler-16b (formally Kepler-16 (AB)-b) is an extrasolar planet.
Kepler (spacecraft) and Kepler-16b · Kepler-16b and Methods of detecting exoplanets ·
Kepler-70b
Kepler-70b (formerly known as its Kepler Object of Interest designation KOI-55.01; sometimes listed as KOI-55 b) is an exoplanet discovered orbiting the subdwarf B star (sdB) Kepler-70.
Kepler (spacecraft) and Kepler-70b · Kepler-70b and Methods of detecting exoplanets ·
Kepler-70c
Kepler-70c (formerly called KOI-55.02; sometimes listed as KOI-55 c) is a planet discovered orbiting the sdB star Kepler-70.
Kepler (spacecraft) and Kepler-70c · Kepler-70c and Methods of detecting exoplanets ·
List of exoplanets
This is a list of exoplanets.
Kepler (spacecraft) and List of exoplanets · List of exoplanets and Methods of detecting exoplanets ·
Main sequence
In astronomy, the main sequence is a continuous and distinctive band of stars that appear on plots of stellar color versus brightness.
Kepler (spacecraft) and Main sequence · Main sequence and Methods of detecting exoplanets ·
Methods of detecting exoplanets
Any planet is an extremely faint light source compared to its parent star.
Kepler (spacecraft) and Methods of detecting exoplanets · Methods of detecting exoplanets and Methods of detecting exoplanets ·
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society (MNRAS) is a peer-reviewed scientific journal covering research in astronomy and astrophysics.
Kepler (spacecraft) and Monthly Notices of the Royal Astronomical Society · Methods of detecting exoplanets and Monthly Notices of the Royal Astronomical Society ·
Moon
The Moon is an astronomical body that orbits planet Earth and is Earth's only permanent natural satellite.
Kepler (spacecraft) and Moon · Methods of detecting exoplanets and Moon ·
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.
Kepler (spacecraft) and NASA · Methods of detecting exoplanets and NASA ·
Neptune
Neptune is the eighth and farthest known planet from the Sun in the Solar System.
Kepler (spacecraft) and Neptune · Methods of detecting exoplanets and Neptune ·
Occultation
An occultation is an event that occurs when one object is hidden by another object that passes between it and the observer.
Kepler (spacecraft) and Occultation · Methods of detecting exoplanets and Occultation ·
The Portable Document Format (PDF) is a file format developed in the 1990s to present documents, including text formatting and images, in a manner independent of application software, hardware, and operating systems.
Kepler (spacecraft) and PDF · Methods of detecting exoplanets and PDF ·
Photometry (astronomy)
Photometry is a technique of astronomy concerned with measuring the flux, or intensity of an astronomical object's electromagnetic radiation.
Kepler (spacecraft) and Photometry (astronomy) · Methods of detecting exoplanets and Photometry (astronomy) ·
Planetary phase
A planetary phase is a period of time during which a certain portion of a planet's area reflects sunlight from the perspective of a given vantage point.
Kepler (spacecraft) and Planetary phase · Methods of detecting exoplanets and Planetary phase ·
PLATO (spacecraft)
PLAnetary Transits and Oscillations of stars (PLATO) is a space observatory under development by the European Space Agency for launch in 2026.
Kepler (spacecraft) and PLATO (spacecraft) · Methods of detecting exoplanets and PLATO (spacecraft) ·
Proceedings of SPIE
Proceedings of SPIE is the conference record of the SPIE.
Kepler (spacecraft) and Proceedings of SPIE · Methods of detecting exoplanets and Proceedings of SPIE ·
Radial velocity
The radial velocity of an object with respect to a given point is the rate of change of the distance between the object and the point.
Kepler (spacecraft) and Radial velocity · Methods of detecting exoplanets and Radial velocity ·
Red dwarf
A red dwarf (or M dwarf) is a small and relatively cool star on the main sequence, of M spectral type.
Kepler (spacecraft) and Red dwarf · Methods of detecting exoplanets and Red dwarf ·
Science (journal)
Science, also widely referred to as Science Magazine, is the peer-reviewed academic journal of the American Association for the Advancement of Science (AAAS) and one of the world's top academic journals.
Kepler (spacecraft) and Science (journal) · Methods of detecting exoplanets and Science (journal) ·
Solar analog
Solar-type star, solar analogs (also analogues), and solar twins are stars that are particularly similar to the Sun.
Kepler (spacecraft) and Solar analog · Methods of detecting exoplanets and Solar analog ·
Solar System
The Solar SystemCapitalization of the name varies.
Kepler (spacecraft) and Solar System · Methods of detecting exoplanets and Solar System ·
Space Interferometry Mission
The Space Interferometry Mission, or SIM, also known as SIM Lite (formerly known as SIM PlanetQuest), was a planned space telescope proposed by the U.S. National Aeronautics and Space Administration (NASA), in conjunction with contractor Northrop Grumman.
Kepler (spacecraft) and Space Interferometry Mission · Methods of detecting exoplanets and Space Interferometry Mission ·
Star
A star is type of astronomical object consisting of a luminous spheroid of plasma held together by its own gravity.
Kepler (spacecraft) and Star · Methods of detecting exoplanets and Star ·
Sun
The Sun is the star at the center of the Solar System.
Kepler (spacecraft) and Sun · Methods of detecting exoplanets and Sun ·
Supernova
A supernova (plural: supernovae or supernovas, abbreviations: SN and SNe) is a transient astronomical event that occurs during the last stellar evolutionary stages of a star's life, either a massive star or a white dwarf, whose destruction is marked by one final, titanic explosion.
Kepler (spacecraft) and Supernova · Methods of detecting exoplanets and Supernova ·
The Astrophysical Journal
The Astrophysical Journal, often abbreviated ApJ (pronounced "ap jay") in references and speech, is a peer-reviewed scientific journal of astrophysics and astronomy, established in 1895 by American astronomers George Ellery Hale and James Edward Keeler.
Kepler (spacecraft) and The Astrophysical Journal · Methods of detecting exoplanets and The Astrophysical Journal ·
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.
Kepler (spacecraft) and Transit (astronomy) · Methods of detecting exoplanets and Transit (astronomy) ·
Transiting Exoplanet Survey Satellite
The Transiting Exoplanet Survey Satellite (TESS) is a space telescope for NASA's Explorers program, designed to search for exoplanets using the transit method in an area 400 times larger than that covered by the Kepler mission.
Kepler (spacecraft) and Transiting Exoplanet Survey Satellite · Methods of detecting exoplanets and Transiting Exoplanet Survey Satellite ·
White dwarf
A white dwarf, also called a degenerate dwarf, is a stellar core remnant composed mostly of electron-degenerate matter.
Kepler (spacecraft) and White dwarf · Methods of detecting exoplanets and White dwarf ·
Wide Angle Search for Planets
WASP or Wide Angle Search for Planets is an international consortium of several academic organisations performing an ultra-wide angle search for exoplanets using transit photometry.
Kepler (spacecraft) and Wide Angle Search for Planets · Methods of detecting exoplanets and Wide Angle Search for Planets ·
The list above answers the following questions
- What Kepler (spacecraft) and Methods of detecting exoplanets have in common
- What are the similarities between Kepler (spacecraft) and Methods of detecting exoplanets
Kepler (spacecraft) and Methods of detecting exoplanets Comparison
Kepler (spacecraft) has 249 relations, while Methods of detecting exoplanets has 189. As they have in common 48, the Jaccard index is 10.96% = 48 / (249 + 189).
References
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