Examples of using Extrasolar in English and their translations into Russian
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The closest extrasolar planet.
For extrasolar planets the temperature of the star can be calculated from the color of the star using Planck's law.
It is one of the smallest extrasolar planets discovered so far.
WASP-2b is an extrasolar planet orbiting the star WASP-2 located about 500 light years away in the constellation of Delphinus.
COROT is a satellite designed for extrasolar planet research.
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Working Group on Extrasolar Planets(WGESP) of the International Astronomical Union.
This planet, 55 Cancer f, was the first occurrence of a fifth extrasolar planet in one system.
The ELODIE Northern Extrasolar Planet Search based at the Haute-Provence Observatory in France.
It was discovered in July 1998 by the Geneva Extrasolar Planet Search team.
In 2004, the Geneva Extrasolar Planet Search Team announced the discovery of an extrasolar planet orbiting the star.
Note that the discovery papers do not use the"b" suffix typically used in extrasolar planet designations.
Librae c(23 Lib c) is an extrasolar planet like Jupiter discovered in 2009 orbiting the star 23 Librae.
In 2008 the HATNet Project announced the discovery of extrasolar planet HAT-P-8b around this star.
Recaptive light and other matter which are drawn back into the sun after having left it,together with other energies having extrasolar origin.”.
HAT-P-7b(or Kepler-2b) is an extrasolar planet discovered in 2008.
The concept has expanded to include worlds not only in the Solar System, butin hundreds of other extrasolar systems.
An exoplanet(/ˈɛksoʊplænɪt/) or extrasolar planet is a planet outside the Solar System.
During the 1990s, the measurement of the stellar wobble of nearby stars was used to detect large extrasolar planets orbiting those stars.
It was discovered by the Geneva Extrasolar Planet Search team at ESO's La Silla Observatory using the HARPS spectrograph.
Theoretical planetary astronomyis concerned with dynamics: the application of the principles of celestial mechanics to the Solar System and extrasolar planetary systems.
It should not be confused with HD 108147, which also has an extrasolar planet located in Crux constellation discovered in 2000.
The Microvariability and Oscillations of Stars(MOST) microsatellite, which is dedicated to asteroseismology, has been in operation for seven years and continues to measure and analyse variations in the light of stars,including light curves of transiting extrasolar planets, with unprecedented accuracy.
In 2004, the VLT allowed astronomers to obtain the first picture of an extrasolar planet(2M1207b) orbiting a brown dwarf 173 light-years away.
In 2009 the discovery of an extrasolar planet in orbit around the binary star was announced, detected by variations in the timings of the eclipses of the two stars.
While high metallicity is beneficial for the creation of terrestrial extrasolar planets, an excess amount can be harmful for life.
The utilization of X-ray mirrors for extrasolar X-ray astronomy simultaneously requires: the ability to determine the location at the arrival of an X-ray photon in two dimensions and a reasonable detection efficiency.
The effect has been found to be an important factor shaping the orbits of irregular satellites of the planets,trans-Neptunian objects, extrasolar planets, and multiple star systems.
This table is constructed from information obtained from the Extrasolar Planets Encyclopedia and SIMBAD databases that reference the Nature article as their source.
The Extrasolar Planets Encyclopaedia is an astronomy website, founded in Paris, France at the Meudon Observatory by Jean Schneider in February 1995, which maintains a database of all the currently known and candidate extrasolar planets, with individual pages for each planet and a full list interactive catalog spreadsheet.
The smallest known planet is PSR B1257+12A,one of the first extrasolar planets discovered, which was found in 1992 in orbit around a pulsar.