An international team of researchers has discovered a new planet, GJ 367 b, whose surface temperature may reach 1,500 degrees Centigrade – hot enough to melt all rock and metal – and which takes only eight hours to orbit its star.
In a new study, published in the Science journal, the researchers show that the planet, which is 31 light-years from Earth, is one of the lightest among the nearly 5,000 exoplanets (planets outside our own solar system) that are known today, with half the mass of Earth. It has a diameter of just over 9,000 kilometers – slightly larger than MarsMars is the second smallest planet in our solar system and the fourth planet from the sun. Iron oxide is prevalent in Mars’ surface resulting in its reddish color and its nickname “The Red Planet.” Mars’ name comes from the Roman god of war.”>Mars.
The team says the research represents a step forward in the search for a “second Earth” as it shows astronomers can determine the properties of even very small planets.
Co-author Dr. Vincent Van Eylen (UCL Mullard Space Science Laboratory) said: “In this new study, the size and mass of the planet were calculated using two methods, both of which involved analyzing the light of the planet’s star. One was to measure the minute dip in emitted light from the star as the planet passed in front of it. This was done using data from NASAEstablished in 1958, the National Aeronautics and Space Administration (NASA) is an independent agency of the United States Federal Government that succeeded the National Advisory Committee for Aeronautics (NACA). It is responsible for the civilian space program, as well as aeronautics and aerospace research. It’s vision is “To discover and expand knowledge for the benefit of humanity.””>NASA’s Transiting Exoplanet Survey Satellite (TESSLaunched on April 18, 2018, aboard a SpaceX Falcon 9 rocket, NASA’s Transiting Exoplanet Survey Satellite (TESS) is a mission to search nearby stars for undiscovered worlds with a gold of discovering thousands of exoplanets around nearby bright stars.”>TESS).
“The other method was to infer the mass of the planet from the effect it had on the movement of the star. This motion was slight – at a rate of 80cm a second, it was no more than walking speed – so it’s fantastic that we were able to detect this tiny motion from 31 light-years away.”
The study involved 78 researchers and was led by astronomers at the Institute of Planetary Research at the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR).
Lead author Dr. Kristine Lam, from the DLR, said: “From the precise determination of its radius and mass, GJ 367b is classified as a rocky planet. This places it among the sub-Earth sized terrestrial planets and brings research one step forward in the search for a ‘second Earth’.”
GJ 367 b belongs to the “ultra-short period” (USP) group of exoplanets that orbit their star in less than 24 hours. “We already know a few of these, but their origins are currently unknown,” said Dr. Lam. “By measuring the precise fundamental properties of the USP planet, we can get a glimpse of the system’s formation and evolution history.”
Following the discovery of this planet using TESS and the transit method, the spectrum of its star was then studied from the ground using the HARPSThe High Accuracy Radial velocity Planet Searcher (HARPS) is one of the most successful planet hunters in the history of astronomy. Housed at ESO’s La Silla Observatory and attached to the 3.6-meter telescope, the HARPS spectrograph searches for exoplanets by detecting minute wobbles in a star’s motion.”>HARPS instrument on the European Southern Observatory’s 3.6m telescope.
With the combination of different evaluation methods, the radius and mass of the planet were determined: its radius is 72 percent of Earth’s radius, and its mass 55 percent of Earth’s mass.
By determining its radius and mass with an accuracyHow close the measured value conforms to the correct value.”>accuracy of 7 and 14 percent respectively, the researchers were also able to draw conclusions about the exoplanetAn exoplanet (or extrasolar planet) is a planet that is outside the Solar System, orbiting around a star other than the Sun. The first suspected scientific detection of an exoplanet occurred in 1988, with the first confirmation of detection coming in 1992.”>exoplanet’s inner structure. It is a low-mass rocky planet, but has a higher density than the Earth. “The high density indicates the planet is dominated by an iron core,” said Dr. Szilárd Csizmadia.
“These properties are similar to those of Mercury, with its disproportionately large iron and nickel core that differentiates it from other terrestrial bodies in the Solar System.”
However, the planet’s proximity to its star means it is exposed to an extreme high level of radiation, more than 500 times stronger than what the Earth experiences. The surface temperature could reach up to 1500 degrees CelsiusThe Celsius scale, also known as the centigrade scale, is a temperature scale named after the Swedish astronomer Anders Celsius. In the Celsius scale, 0 °C is the freezing point of water and 100 °C is the boiling point of water at 1 atm pressure.”>Celsius – a temperature at which all rocks and metals would be melted.
The parent star of this newly discovered exoplanet, a red dwarf called GJ 367, is only about half the size of the Sun. This was beneficial for its discovery as the transit signal of the orbiting planet is particularly significant. Red dwarfs are not only smaller, but also cooler than the Sun. This makes their associated planets easier to find and characterize. They are among the most common stellar objects in our cosmic neighborhood and are therefore suitable targets for exoplanet research.
Researchers estimate that these red dwarfs, also known as ‘class M stars’, are orbited by an average of two to three planets, each of which is at most four times the size of Earth.
For more on this discovery, read Sub-Earth Planet Discovered by Astronomers: Boiling New World Is Ultra-Light and Super-Fast.
Reference: “GJ 367b: A dense ultra-short period sub-Earth planet transiting a nearby red dwarf star” by Kristine W. F. Lam, Szilárd Csizmadia, Nicola Astudillo-Defru, Xavier Bonfils, Davide Gandolfi, Sebastiano Padovan, Massimiliano Esposito, Coel Hellier, Teruyuki Hirano, John Livingston, Felipe Murgas, Alexis M. S. Smith, Karen A. Collins, Savita Mathur, Rafael A. Garcia, Steve B. Howell, Nuno C. Santos, Fei Dai, George R. Ricker, Roland Vanderspek, David W. Latham, Sara Seager, Joshua N. Winn, Jon M. Jenkins, Simon Albrecht, Jose M. Almenara, Etienne Artigau, Oscar Barragán, François Bouchy, Juan Cabrera, David Charbonneau, Priyanka Chaturvedi, Alexander Chaushev, Jessie L. Christiansen, William D. Cochran, José R. De Meideiros, Xavier Delfosse, Rodrigo F. Díaz, René Doyon, Philipp Eigmüller, Pedro Figueira, Thierry Forveille, Malcolm Fridlund, Guillaume Gaisné, Elisa Goffo, Iskra Georgieva, Sascha Grziwa, Eike Guenther, Artie P. Hatzes, Marshall C. Johnson, Petr Kabáth, Emil Knudstrup, Judith Korth, Pablo Lewin, Jack J. Lissauer, Christophe Lovis, Rafael Luque, Claudio Melo, Edward H. Morgan, Robert Morris, Michel Mayor, Norio Narita, Hannah L. M. Osborne, Enric Palle, Francesco Pepe, Carina M. Persson, Samuel N. Quinn, Heike Rauer, Seth Redfield, Joshua E. Schlieder, Damien Ségransan, Luisa M. Serrano, Jeffrey C. Smith, Ján Šubjak, Joseph D. Twicken, Stéphane Udry, Vincent Van Eylen and Michael Vezie, 2 December 2021, Science.