astro.wikisort.org - Meteorite

Gliese 832 c (also known as Gl 832 c or GJ 832 c) is an extrasolar planet candidate located approximately 16 light-years (4.93 parsecs, or about 151.4 trillion km) away in the constellation of Grus, orbiting the star Gliese 832, a red dwarf.[1][2] Existence of the planet was disputed in 2022, after finding its putative orbital period close to the rotation period of the parent star.[3]

This article uses bare URLs, which are uninformative and vulnerable to link rot. (September 2022)

Gliese 832 c

An artist's impression of Gliese 832 c.
Orbital characteristics
Semi-major axis	0.162 (± 0.017) AU
Eccentricity	0.18 (± 0.13)
Orbital period (sidereal)	35.68 (± 0.03) d
Star	Gliese 832
Physical characteristics
Mean radius	≥1.5(?) REarth
Mass	≥5.4 (± 1) MEarth
Temperature	253 K (−20 °C; −4 °F)

It is in its star's habitable zone and a big reason for its high rating is it receives the same amount of solar flux as the earth in the habitable exoplanets catalog. The planet has a mass of 5.2 Earth's masses and an estimated radius of >1.5 Earth radii.

To date, it is the fifth-closest known potentially habitable exoplanet to Earth.[2] The closest potentially habitable exoplanet is Proxima Centauri b at 4.244 light years. Second is Ross 128 b at 10.92 light years away, followed by Luyten b (and not counting the unconfirmed planets Tau Ceti e and f). Fourthly is Wolf 1061c at 13.8 light years from the sun.

Characteristics Of Gliese 832 c

Mass, radius, and temperature

Gliese 832 c has a mass of approximately 5.2 times that of Earth. If it had the same density of Earth it would have a radius of around 1.75 R_Earth or possibly the planet could have a higher density with a smaller radius. Its temperature is predicted to be relatively similar to Earth's, but is subject to significant swings as it orbits its star. The planet has a relatively high eccentricity, taking it very near to the predicted inner edge of the habitable zone. The planet's average equilibrium temperature is predicted to be 253 kelvins (−20 °C), but is estimated to vary from 233 kelvins (−40 °C) at apstellion to 280 kelvins (7 °C) at.[4] However, because of its large mass, it may have a dense atmosphere, which could make it much hotter and more like the planet Venus.[5][6]

Host star

The planet orbits a (M-type) star named Gliese 832, orbited by a total of two known planets. The star has a mass of 0.45 M_☉ and a radius of 0.48 R_☉. It has a temperature of 3620 K and is estimated to be about 9.54 billion years old.[7] In comparison, the Sun is 4.6 billion years old[8] and has a temperature of 5778 K.[9]

The star's apparent magnitude, or how bright it appears from Earth's perspective, is 10.19. Therefore, it is too dim to be seen with the naked eye. It is of spectral class M2V.

Orbit

The planet orbits its host star with about 3% of the Sun's luminosity approximately every 36 days, 10 times shorter than earth's year.[4] and an orbital radius 0.162 times that of Earth (compared to Mercury's orbital distance of 0.389 AU).

Habitability

The planet is a super-Earth mass planet orbiting in its star's habitable zone. Although it orbits its star much closer than the Earth orbits the Sun, it orbits a red dwarf, receiving approximately as much energy from it as the Earth does from its star.[2] It is not known whether Gliese 832 c transits its host star, something which would be required in order to detect any atmosphere the planet may have and determine its composition.

Its host star (Gliese 832) has 45% of the Sun's mass, and as a result, stars like Gliese 832 have the ability to live up to 50–60 billion years, 5–6 times longer than the Sun will live.[10]

The planet is likely tidally locked, with one side of its hemisphere permanently facing towards the star, while the opposite side shrouded in eternal darkness. However, between these two intense areas, there would be a sliver of habitability – called the terminator line, where the temperatures may be suitable (about 273 K (0 °C; 32 °F)) for liquid water to exist. Additionally, a much larger portion of the planet may be habitable if it supports a thick enough atmosphere to transfer heat to the side facing away from the star.

In the case that Gliese 832 c possesses a Venusian-like atmosphere, which it could have due to its eccentric orbit (and the stellar flux reaching 1.45 S_🜨, high enough to boil any oceans on its surface), the planet would be inhospitable because of a runaway greenhouse effect on its surface. Any oceans on its surface would have boiled away due to the dense atmosphere, and as this occurred, the temperature would have risen to around 322 K (49 °C; 120 °F). The water vapor would accumulate in the atmosphere to the point where the surface temperature would rise to around 700 K (427 °C; 800 °F) as the planet would have been overwhelmed by water vapor (which is a powerful greenhouse gas).[11] Little amounts of carbon dioxide would have been present, as Gliese 832 c was/is probably an ocean planet. The surface pressure would have also increased to around 100 times Earth's surface pressure (100 kilopascals, 100 atm.) because of the amount of water vapor in the atmosphere. The net result would be that Gliese 832 c being a desert planet, rather than an ocean planet.

Discovery and impact

Gliese 832 c was discovered by an international team of astronomers led by Robert A. Wittenmyer.[2][4] It is the newest and closest to earth member of the top three most Earth-like worlds in the Habitable Exoplanets Catalog.[4]

The planet's discoverers described the planet as "the nearest best habitable world candidate so far".[12]

Further research may be done on Gliese 832 c to see if it is suitable for life.[6]

See also

• Gliese 832 b
• Extrasolar life
• Exobiology
• List of potentially habitable exoplanets

References

External links

• Artist's conception of Gliese 832
• Artist's conception of Gliese 832 compared to the earth
• The original study

На других языках

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[de] Gliese 832c

Gliese 832c ist ein Exoplanet, der den rund 16 Lichtjahre von der Sonne entfernten Roten Zwerg Gliese 832 im Sternbild Kranich umkreist. Er wurde 2014 von einem Team um den australischen Astronomen Robert A. Wittenmeyer von der University of New South Wales mittels der Radialgeschwindigkeitsmethode entdeckt.[3][4] Der Planet ist einer von zwei Planeten, die Gliese 832 umkreisen, neben dem bereits 2008 entdeckten und weiter außen umlaufenden jupiterähnlichen Planeten Gliese 832b.[5][4] Er befindet sich in der habitablen Zone seines Zentralsterns.[2]

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- [en] Gliese 832 c

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[es] Gliese 832 c

Gliese 832 c (o GJ 832 c) es un exoplaneta supertierra confirmado, que orbita la estrella enana roja Gliese 832, a una distancia de 16,1 años luz de la Tierra en la constelación de Grus. Su descubrimiento, anunciado en 2014, se realizó por el método de velocidad radial. Con un IST del 81 %, es uno de los exoplanetas confirmados con mayor parentesco con la Tierra.[1][2]

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[ru] Глизе 832 c

Глизе 832 c — экзопланета в созвездии Журавля, обращающаяся вокруг красного карлика Глизе 832. Находится на расстоянии примерно 16 световых лет от Солнца.

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