Astronomers report the invention of a brand new heat Jupiter exoplanet orbiting a distant star within the open cluster Messier 67. The newfound extrasolar world, designated S1429 b, is sort of twice as large as Jupiter. The discovering was detailed in a paper printed March 5 on the pre-print server arXiv.
Heat Jupiters are gasoline giant planets with orbital periods between 10 and 200 days. This makes them difficult targets for transit detection and radial velocity (RV) follow-up research in comparison with their shorter-orbit counterparts, dubbed scorching Jupiters.
Just lately a crew of astronomers, led by Luis Thomas of the College Observatory Munich in Germany, have carried out spectroscopic observations of 11 stars in Messier 67 (or M67 for brief, dubbed additionally the King Cobra Cluster)—an previous and well-populated Galactic open cluster (OC).
The observational marketing campaign, which employed primarily the Liveable Planet Finder (HPF) spectrograph mounted on the 10m Passion-Eberle Telescope (HET) on the McDonald Observatory in Texas, was a part of the “Seek for Big Planets in M67” RV survey.
“Between December 2019 and March 2022, we continued the observations of 11 stars in M67 with the Liveable Planet Finder spectrograph (HPF). We included six stars that confirmed potential long-term RV variations and 5 stars on the turn-off level of M67 which had no beforehand printed information,” the researchers wrote within the paper.
The observations carried out by Thomas’ crew resulted within the detection of a brand new planet round a turn-off level star of spectral kind F9.5V generally known as S1429. The newly discovered alien world, which acquired designation S1429 b, is the sixth planet found in Messier 67.
Based on the paper, S1429 b has a minimal mass of 1.8 Jupiter lots and orbits its host star each 77.48 days on a probably round orbit, at a distance of roughly 0.384 AU from it. The equilibrium temperature of the planet was estimated to be about 683 Ok.
The mum or dad star S1429, situated some 2,800 light years away from the Earth, is about two instances bigger than the sun, whereas its mass is only one.26 solar lots. The star is estimated to be 4.3 billion years previous, has an effective temperature of practically 6,000 Ok, and its metallicity is at a degree of -0.013 dex.
Summing up the outcomes, the authors of the paper underlined that the total six identified planet-hosting stars in Messier 67, together with S1429, are distributed over completely different evolutionary levels.
Particularly, there are three scorching Jupiters orbiting main-sequence stars and the longer interval planets orbit a turn-off level star and two crimson giants. They famous that every one the three scorching Jupiters on this cluster have minimal lots considerably beneath one Jupiter mass.
Extra info:
Luis Thomas et al, Seek for big planets in M67 V: a heat Jupiter orbiting the turn-off star S1429, arXiv (2024). DOI: 10.48550/arxiv.2403.02911
Journal info:
arXiv
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Heat Jupiter exoplanet orbiting distant star detected (2024, March 14)
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