GJ. Recent surveys have revealed that planets intermediate in size between Earth and Neptune (“super-Earths”) are among the most common planets in the Galaxy[1, 2, 3]. As a result, the internal structure of GJ 1214b would be extraordinarily different from that of our world. “ The high temperatures and high pressures would form exotic materials like ‘hot ice’ or ‘superfluid water’, substances that are completely alien to our everyday experience, ” Berta said. GJ 1214b 3D GCM assuming a global mean surface pressure of 105 Pa and a surface albedo of 0.4. The planet GJ 1214b is the second known super-Earth with a measured mass and radius. Its current location was too hot for icy-building blocks to exist in the protoplanetary disk where the planet was born. Astronomers have confirmed the existence of a waterworld orbiting another sun, 40 light years away from us. Its density and enormous water reserves seem to confirm this. 2017, for an overview of available transit observations). It is much closer to its sun. But both temperature and pressure are high to the point that water could exist on this planet in the form of a superfluid and hot ice! De plus, des études ont montré que les super-Terres comme GJ 1214b étaient sans doute les plus répandues dans la Voie lactée. For that reason, scientists have nicknamed the planet "the waterworld". A large part of its mass consists of water much more than the earth but not comparable to our water. This planet According to a 2012 study based on observations by the Hubble Space Telescope, GJ 1214 b is actually a massive water world encapsulated by a dense and steamy atmosphere. It orbits a red-dwarf star every 38 hours at a distance of 2 million kilometres, giving it an estimated temperature of 230 degrees Celsius. 8. "GJ 1214b is like no planet we know of," Berta said. " Using the Hubble Space Telescope, U.S. astronomers discovered the planet GJ 1214b is shrouded by clouds and its temperature is caused by its nearby parent star. It is the most likely known candidate for being an ocean planet. Image credit: CfA/David Aguilar . The Astrophysical Journal, 716:1208–1216, 2010 June 20. Marley et al. GJ 1214b orbits the host star close to it, in contrast to Uranus and Neptune. Recent measurements have shown its near-infrared transmission spectrum to be flat, pointing to a high-altitude opacity source in the exoplanet 's atmosphere, either equilibrium condensate clouds or photochemical hazes. Une perspective d'importance alors que ce type de planètes reste largement méconnu. The winds are westerly at the equator and easterly in the midlatitudes. The surface temperature of the planet GJ 1214b reaches 232º Celsius. The planet’s mass (6.6 M⊕) and radius (2.7 R⊕) imply a density that is too low to be explained by rock and water ice alone. Gj 1214b - The Waterworld. Case Study: Origins of Gas Layer on GJ 1214b. Currently, water in GJ 1214b has a consistency that is very strange and will seem very familiar to us, as a result of high temperature and atmospheric pressure is great, the water will be more like hot ice thick or act more … In the end, the actual planet atmospheric composition depends on the interior composition of the planet, the mass and temperature of the planet, and the planet evolution. Discovered in 2009 , the planet is about 2.7 times Earth’s diameter and is almost 7 times as massive. In 2010, CfA scientist Jacob Bean and colleagues reported that they had measured the atmosphere of GJ 1214b, finding it likely that it was composed mainly of water. If it is a water world, it could possibly be thought of as a bigger and hotter version of Jupiter's Galilean moon Europa. This planet, orbiting an M4.5 star only 13 pc from the Earth, is of particular interest because it lies between the Earth and Neptune in size and may be a member of a new class of planet that is neither terrestrial nor gas giant. GJ 1214b and the prospects for liquid water on super Earths - Volume 6 Issue S276 - Leslie A. Rogers, Sara Seager GJ 1214b Angela M. Zalucha (Massachusetts Institute of Technology, Southwest Research Institute) Nikku Madhusudhan (Yale) Tim Michaels (Southwest Research Institute) The super-Earth GJ 1214b gravitational acceleration: 8.93 m s–2 radius: 2.678 R e distance from star: 0.01432 AU stellar flux at planet: 21519 W m–2 rotation period: 1.5803925 Earth days (synchronous) (Charbonneau et al. GJ 1214b has no land, but only oceans that stretch all over the surface. GJ 1214b is about 2.7 times wider than Earth's but with a mass seven times higher. POST. Although warm as an oven, it is still cooler than any other known transiting planet because it orbits a very dim star. The temperature of the stellar corona is estimated to be about 3.5 × 10 6 K. Planetary system. GJ 1214b (Charbonneau et al. GJ 1214b yield a day-side equilibrium temperature of 660 K for redistribution of incident energy over the day-side only, and 555 K for efficient redistribution over the entire planet, if the planet’s Bond albedo is zero. Final score: 15 points. 2–He atmosphere scenarios for the warm super-Earth GJ 1214b using an optimal estimation retrieval technique. According to study author Zachory Berta, then at the Harvard-Smithsonian Center for Astrophysics, in a press release, “GJ 1214b is like no planet we know of. The data seem to confirm that GJ 1214b has a very steamy atmosphere, thick with water vapor. Gliese 1214 b (often shortened to GJ 1214 b) is an exoplanet that orbits the star Gliese 1214, and was discovered in December 2009.Its parent star is 48 light-years from the Sun, in the constellation Ophiuchus.As of 2017, GJ 1214 b is the most likely known candidate for being an ocean planet. lincholn6echo. • GJ 1214b is the first super-Earth to have a potentially observable atmosphere with current instrumentation • Transmission spectroscopy of the planet’s atmosphere can break the degeneracy between interior composition models • Clouds can add additional complexity to the interpretation of GJ 1214b’s spectral signature. A … GJ 1214b has now become the world's hot with temperatures around 200 C (392 F) 7. Discovered by the MEarth project and investigated further by the HARPS spectrograph on ESO’s 3.6-metre telescope at La Silla, GJ1214b is the second super-Earth exoplanet for which astronomers have determined the mass and radius, giving vital clues about its structure. The planet GJ 1214b, shown here in an artist’s conception with two hypothetical moons, orbits a “red dwarf” star 40 light-years from Earth. Published on 23 February 2012. We present three-dimensional atmospheric circulation models of GJ 1214b, a 2.7 Earth-radius, 6.5 Earth-mass super Earth detected by the MEarth survey. Wikipedia Report. This artist’s impression shows how the newly discovered super-Earth surrounding the nearby star GJ1214 may look. Even more intriguing is that due to the temperature (being so close to its red dwarf star makes it around 450 degrees Fahrenheit) and extreme pressures, all that water gets a bit…exotic. Therefore, if GJ 1214b contains a significant amount of water, it is reasonable to think that the planet has experienced the orbital migration. GJ 1214b: an unusual waterworld; GJ 1214b: an unusual waterworld. The super-Earth GJ 1214b, which has 6.5 times the mass of our Earth, orbits its star once every 38 hours at a distance of only 1.3 million miles. 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