Exoplanet travel bureau

Digital Trends space writer for six years, covering human space exploration, planetary… Space This extreme exoplanet has a highly unusual orbit This artist’s impression shows a Jupiter-like exoplanet that is on its way to becoming a hot Jupiter — a large, Jupiter-like exoplanet that orbits very close to its star. NOIRLab/NSF/AURA/J. da Silva (Spaceengine)Exoplanets come in all sorts of shapes and sizes, and can be weird in all sorts of ways. There are football shaped exoplanets and exoplanets where it rains gemstones; ones with the density of cotton candy and ones with one lava hemisphere. But new research has uncovered an exoplanet called TIC 241249530 b which is unusual in a different sort of way, as it has one of the most extreme orbits discovered to date. Read more Space Exoplanet catalog details over 100 worlds beyond our solar system TOI-1798 is a system that is home to two planets. The inner planet is a strange Super-Earth so close to its star that one year on this alien world lasts only half an Earth day. W. M. Keck Observatory/Adam MakarenkoA new catalog of exoplanets from two telescopes shows the incredible variety of planets that exist beyond our solar system. The catalog, using data from NASA's TESS (Transiting Exoplanet Survey Satellite) space telescope and the ground-based W. M. Keck Observatory, shows 126 planets, along with the radius, mass, density and temperature of each. Read more Space James Webb observes extremely hot exoplanet with 5,000 mph winds Astronomers using the James Webb

Another for the ExoClock project by Simon Dawes of the transit of exoplanet TrES-3b.TrES-3b is in a very tight orbit around its host star, TrES-3, transiting the stellar disk once per 31 hours. For comparison, Mercury orbits the sun once every 88 days. TrES-3b is just a little larger than Jupiter, yet orbits around its parent star much closer than Mercury does, making it a “hot jupiter.” The transit of Exoplanet TrES-3b by CMHASD member & trustee Dr. Mike Rushton using an eVscope for the ExoClock project.TrES-3b is a gas giant exoplanet orbiting the star GSC 03089-00929 a G-type star and is 0.02282 AU from its star. It has an orbital period of just 31 hours and nearly twice the mass of Jupiter. It was found by the Trans-Atlantic Exoplanet Survey in 2007. It was discovered in the constellation Hercules about 10 degrees west of the star Vega.The planet TrES-3b is named Umbäässa. The name was selected in the NameExoWorlds campaign by Liechtenstein, during the 100th anniversary of the IAU. In the local dialect of southern Liechtenstein, Umbäässa is a small and barely visible ant. Another for the ExoClock project by CMHASD member & trustee Martin Crow of ExoPlanet TOI-1728b; a warm Super-Neptune orbiting an M-dwarf host. More observations for the ExoClock project by Simon Dawes of Qatar-1b in the constellation of Draco taken on the 7th July 2023. Another set of observations for the ExoClock project by member Simon Dawes :-)Simon wrote ''This was a tricky observation, a bright star with faint comparisons, on the night of the summer solstice - the worst night of the year for astronomy, due to the lack of real night - there were 627 15s exposures which, when processed, works out at about 60Gb of disk space - for a single O-C measurement!''''This far-off blue planet may look like a friendly haven – but don’t be deceived! Weather here is deadly. The planet’s cobalt blue colour comes from a hazy, blow-torched atmosphere containing clouds laced with glass. Howling winds send the storming glass sideways at 5,400 mph (2km/s), whipping all in a sickening spiral. It’s death by a million cuts on this slasher planet!'' Ref: 189733b is an exoplanet approximately 64.5 light-years away in the constellation of Vulpecula. The planet was discovered on October 5, 2005. HD 189733b orbits its host star once every 2.2 days.The closest transiting hot Jupiter to Earth, scientists have extensively studied the exoplanet's atmosphere. Researchers have found that the planet has an unusual rain of molten glass. Another set of transit observations for the ExoClock project by Simon Dawes of Exoplanet HAT-P-12b.HAT-P-12b is 468 light years away from Earth, orbiting a 13th magnitude K-type star in the constellation

Canes Venatici. It is was discovered by the HATNet Project on April 29, 2009. The transit of EPIC 246851721b measured by CMHASD member and trustee Martin Crow for the ExoClock project on the 21st January 2023. The transit depth is a mere 5 thousandths of a magnitude. EPIC 246851721b is a gas giant exoplanet that orbits an F-type star in the constellation Taurus. Its mass is 3 Jupiters, it takes 6.2 days to complete one orbit of its star and is 0.07229 AU from its star. This planet was discovered by Yu et al. 2018. The discovery was made with the space telescope 0.95 m Kepler Telescope. This is a montage of the exo-planet transits that CMHASD member and trustee Simon Dawes observed in 2022 for the ExoClock project. A total of 60 for 2022. Well done Simon! A huge congratulations to CMHASD trustees Martin Crow and Simon Dawes for jointly winning the BAA Sir Patrick Moore Prize for Pro-Am work on Exoplanet observations with the ExoClock project along with a Mr Adrian Jones.Below is a photo of Martin and Simon being presented with their certificates by the President of the BAA David Arditti on Saturday 10th December 2022 at the BAA Christmas Meeting. From left to right: David Arditti, Adrian Jones, Martin Crow & Simon Dawes. The videos from the British Astronomical Association (BAA) Exoplanet Division Online Workshop held on Saturday 12th November are now available to watch on the BAA YouTube Channel.The below talk titles are links to watch the videos. Two videos are by CMHASD members Rodney Buckland and Martin Crow.Introduction by Roger DymockExoplanet Division updateEXPLORE introductionAriel and ExoClock with Anastasia KokoriMission and observational efficiencyExoClock – a model of pro-am collaborationEXPLORE Part 1 – Detecting exoplanets with Rodney BucklandObservationModellingSearching databasesZooniverseHow to discover an exoplanet (telescope and camera not required) with Roger DymockEXPLORE Part 2 with Martin CrowIntroduction to HOPSSynchronous observations to detect shallow transitsData mining transit observations for variable star photometryAstroImageJ with Richard LeeAn alternative to HOPSClick to download a zip of the User Guide for the Observation Planner for AstroImageJ and sample files.Observing with robotic telescopes by Rodney BucklandEXPLORE NEEDS EXPLORERS with Roger DymockRodney's VideoMartin's Video

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