List Of Star Systems Within 30–35 Light-years
This is a list of star systems within 30–35 light years of Earth. See also * Lists of stars * List of star systems within 25-30 light-years * List of star systems within 35-40 light-years * List of nearest stars and brown dwarfs This list covers all known stars, brown dwarfs, and sub-brown dwarfs within of the Sun. So far, 131 such objects have been found, of which only 22 are bright enough to be visible without a telescope. The visible light needs to reach or excee ... References {{DEFAULTSORT:List of star systems within 30-35 light-years star systems within 30-35 light-years Star systems star systems within 30-35 light-years ... [...More Info...]       [...Related Items...]     OR:     [Wikipedia]   [Google]   [Baidu]   |
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Earth
Earth is the third planet from the Sun and the only astronomical object known to harbor life. While large volumes of water can be found throughout the Solar System, only Earth sustains liquid surface water. About 71% of Earth's surface is made up of the ocean, dwarfing Earth's polar ice, lakes, and rivers. The remaining 29% of Earth's surface is land, consisting of continents and islands. Earth's surface layer is formed of several slowly moving tectonic plates, which interact to produce mountain ranges, volcanoes, and earthquakes. Earth's liquid outer core generates the magnetic field that shapes the magnetosphere of the Earth, deflecting destructive solar winds. The atmosphere of the Earth consists mostly of nitrogen and oxygen. Greenhouse gases in the atmosphere like carbon dioxide (CO2) trap a part of the energy from the Sun close to the surface. Water vapor is widely present in the atmosphere and forms clouds that cover most of the planet. More sola ... [...More Info...]       [...Related Items...]     OR:     [Wikipedia]   [Google]   [Baidu]   |
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2MASS J11592743-5247188
Mass is an intrinsic property of a body. It was traditionally believed to be related to the quantity of matter in a physical body, until the discovery of the atom and particle physics. It was found that different atoms and different elementary particles, theoretically with the same amount of matter, have nonetheless different masses. Mass in modern physics has multiple definitions which are conceptually distinct, but physically equivalent. Mass can be experimentally defined as a measure of the body's inertia, meaning the resistance to acceleration (change of velocity) when a net force is applied. The object's mass also determines the strength of its gravitational attraction to other bodies. The SI base unit of mass is the kilogram (kg). In physics, mass is not the same as weight, even though mass is often determined by measuring the object's weight using a spring scale, rather than balance scale comparing it directly with known masses. An object on the Moon would weigh ... [...More Info...]       [...Related Items...]     OR:     [Wikipedia]   [Google]   [Baidu]   |
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WISE J140533
WISE may refer to: Arts, entertainment, and media * WISE (AM), a radio station licensed to Asheville, North Carolina *WISE-FM, a radio station licensed to Wise, Virginia * WISE-TV, a television station licensed to Fort Wayne, Indiana Education * Web-based Inquiry Science Environment, a program hosted by Berkeley University * Wilberforce Institute for the study of Slavery and Emancipation, a research institute at University of Hull, England * Wind Science and Engineering Research Center (WiSE), at Texas Tech University * World Islamic Sciences and Education University, in Amman, Jordan Organisations and programmes *WISE Campaign, an initiative to encourage women into science and engineering * Work improvement in small enterprises, a programme for improvement of occupational health-and-safety conditions *World Information Service on Energy, an international anti-nuclear network based in Amsterdam *World Innovation Summit for Education, a global forum based in Doha, Qatar * World Ins ... [...More Info...]       [...Related Items...]     OR:     [Wikipedia]   [Google]   [Baidu]   |
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LHS 6167
The initials LHS are used for: Australia * Leumeah High School, New South Wales * Lyneham High School, Australian Capital Territory United Kingdom * Litherland High School, Liverpool, England * Larbert High School, Stenhousemuir, Scotland United States * Lafayette High School (other) * Lahainaluna High School, Maui Hawai’i * Lamar High School (other) * Lanphier High School, Springfield,IL * Lawrence High School (New Jersey) * Lebanon High School (other) * Lee High School (other) * Legacy High School (other) * Lejeune High School, Jacksonville, North Carolina * Lexington High School (other) * Linganore High School, Frederick Co, Maryland * Lowell High School (other) * Ludington High School * Lufkin High School * Lynnwood High School, Lynnwood, Washington * Lynwood High School, Lynwood, California Science and mathematics * Luyten Half-Second catalogue, a star catalogue system * Latin hypercube sampling, in s ... [...More Info...]       [...Related Items...]     OR:     [Wikipedia]   [Google]   [Baidu]   |
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TYC 3251-1875-1
Torneos y Competencias S.A. (abbreviated TyC, also referred as Torneos) is an Argentine sports communications firm created by businessman Carlos Ávila, associated with Jose Santoro, and Héctor Dayan. It is an important force in the world of Argentine sports, with interests in publications and radio and TV broadcasting. Its headquarters are in Buenos Aires. History Torneos started its activities in the Argentine media in 1982, with a golf program. Since then it produced and aired successful programs in network television such as ''El deporte y el hombre'', ''Tenis de Primera'', ''Fútbol de Primera'' and ''La Magia de la NBA''; the most successful of them being the weekly ''Fútbol de Primera'', which summarizes each day of competition in the Argentine first division. In 1994, Torneos launched the channel TyC Sports to broadcast the Argentine Primera Division. Removal of first division television rights In 1992, the company Televisión Satelital Codificada (TSC, a joint vent ... [...More Info...]       [...Related Items...]     OR:     [Wikipedia]   [Google]   [Baidu]   |
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Gliese 358
Gliese may refer to: * Rochus Gliese (1891—1978), a German actor, director, production designer, and art director * Wilhelm Gliese (1915–1993), a German astronomer, best known for the Gliese Catalogue of Nearby Stars * Gliese Catalogue of Nearby Stars, a modern star catalog of stars located within 25 parsecs of the Earth * Gliese 163, a red dwarf located 49 light years from the Sun * Gliese 229, a binary system composed of a red dwarf and a brown dwarf about 19 light years away in the constellation Lepus. * Gliese 581, a red dwarf orbited by several extra-solar planets, at least ** Gliese 581d, a planet in the star's habitable zone * Gliese 667, a triple star system in the constellation of Scorpius containing exoplanet GJ 667 Cc in one of the stars' habitable zone * Gliese 682, a red dwarf in the constellation of Scorpius with two candidate planets, one of which is in the star's habitable zone * Gliese 710 Gliese 710, or HIP 89825, is an orange star in the conste ... [...More Info...]       [...Related Items...]     OR:     [Wikipedia]   [Google]   [Baidu]   |
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61 Ursae Majoris
61 Ursae Majoris, abbreviated 61 UMa, is a single star in the northern circumpolar constellation of Ursa Major. It has a yellow-orange hue and is dimly visible to the naked eye with an apparent visual magnitude of 5.35. The distance to this star is 31.2 light years based on parallax, and it is drifting closer with a radial velocity of −5.2 km/s. The star has a relatively high proper motion traversing the sky at the rate of yr−1. The stellar classification of 61 UMa is G8V, matching a late G-type main-sequence star. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. It is considered a solar-type star, having physical properties that make it similar to the Sun. The star has 93% of the mass of the Sun and 86% of the Sun's radius. It is roughly two billion years old and is spinning with a projected rotational velocity of 3.3 km/s, for a period of 17.1 days. The me ... [...More Info...]       [...Related Items...]     OR:     [Wikipedia]   [Google]   [Baidu]   |
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2MASS J11553952-3727350
Mass is an intrinsic property of a body. It was traditionally believed to be related to the quantity of matter in a physical body, until the discovery of the atom and particle physics. It was found that different atoms and different elementary particles, theoretically with the same amount of matter, have nonetheless different masses. Mass in modern physics has multiple definitions which are conceptually distinct, but physically equivalent. Mass can be experimentally defined as a measure of the body's inertia, meaning the resistance to acceleration (change of velocity) when a net force is applied. The object's mass also determines the strength of its gravitational attraction to other bodies. The SI base unit of mass is the kilogram (kg). In physics, mass is not the same as weight, even though mass is often determined by measuring the object's weight using a spring scale, rather than balance scale comparing it directly with known masses. An object on the Moon would weigh ... [...More Info...]       [...Related Items...]     OR:     [Wikipedia]   [Google]   [Baidu]   |
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HR 4458
HR 4458 is a binary star system in the equatorial constellation of Hydra. It has the Gould designation 289 G. Hydrae; ''HR 4458'' is the Bright Star Catalogue designation. At a distance of 31.13 light years, it is the closest star system to the Solar System within this constellation. This object is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 5.97. It is moving closer to the Earth with a heliocentric radial velocity of −22 km/s. The primary component is K-type main-sequence star with a stellar classification of K0 V. It is around five billion years old with 84% of the Sun's radius. The star is radiating 37% of the Sun's luminosity from its photosphere at an effective temperature of 5,241 K. It has been examined for the presence of an infrared excess, but none was detected. There is a common proper motion companion at an angular separation of 16.2″, corresponding to a projected separation of . This ... [...More Info...]       [...Related Items...]     OR:     [Wikipedia]   [Google]   [Baidu]   |
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Gliese 1227
Gliese may refer to: * Rochus Gliese (1891—1978), a German actor, director, production designer, and art director * Wilhelm Gliese (1915–1993), a German astronomer, best known for the Gliese Catalogue of Nearby Stars * Gliese Catalogue of Nearby Stars, a modern star catalog of stars located within 25 parsecs of the Earth * Gliese 163, a red dwarf located 49 light years from the Sun * Gliese 229, a binary system composed of a red dwarf and a brown dwarf about 19 light years away in the constellation Lepus. * Gliese 581, a red dwarf orbited by several extra-solar planets, at least ** Gliese 581d, a planet in the star's habitable zone * Gliese 667, a triple star system in the constellation of Scorpius containing exoplanet GJ 667 Cc in one of the stars' habitable zone * Gliese 682, a red dwarf in the constellation of Scorpius with two candidate planets, one of which is in the star's habitable zone * Gliese 710 Gliese 710, or HIP 89825, is an orange star in the conste ... [...More Info...]       [...Related Items...]     OR:     [Wikipedia]   [Google]   [Baidu]   |
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GJ 3512
GJ 3512 is a nearby star in the northern circumpolar constellation of Ursa Major. It is invisible to the naked eye but can be observed using a telescope, having an apparent visual magnitude of +15.05. The star is located at a distance of 31 light-years from the Sun based on parallax. It has a high proper motion, traversing the celestial sphere at the rate of yr−1. The measurement of the star's radial velocity is poorly constrained, but it appears to be drifting further away at a rate of ~8 km/s. The stellar classification of GJ 3512 is dM5.5, which determines this to be a small red dwarf star that is generating energy through core hydrogen fusion. It displays a moderate amount of magnetic activity with a Sun-like cycle lasting 14 years. A low-level variability lasting matches the approximate rotation period. The star has 12.5% of the mass of the Sun and 16% of the Sun's radius. It is radiating 1.6% of the luminosity of the Sun from its photosphe ... [...More Info...]       [...Related Items...]     OR:     [Wikipedia]   [Google]   [Baidu]   |