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Gaia is so accurate it can predict microlensing events

Gaia is so accurate it can predict microlensing events
phys.org - get the latest breaking news, showbiz & celebrity photos, sport news & rumours, viral videos and top stories from phys.org Daily Mail and Mail on Sunday newspapers.

Kunming
Yunnan
China
Chinese
Hsu-jie
University-of-chinese-academy-sciences
Chinese-academy-of-sciences
Key-laboratory-for-the-structure
Monthly-notices-of-the-royal-astronomical-society
College-of-information-engineering-at-kunming-university
Chinese-academy
Yunnan-observatories

Gaia is so Accurate it Can Predict Microlensing Events

Gaia is so Accurate it Can Predict Microlensing Events
universetoday.com - get the latest breaking news, showbiz & celebrity photos, sport news & rumours, viral videos and top stories from universetoday.com Daily Mail and Mail on Sunday newspapers.

Kunming
Yunnan
China
Chinese
Hsu-jie
Key-laboratory-for-the-structure
Chinese-academy-of-sciences
University-of-chinese-academy-sciences
College-of-information-engineering-at-kunming-university
Monthly-notices-of-the-royal-astronomical-society
Chinese-academy
Yunnan-observatories

Gaia telescope's new data reveals 'goldmine' of over 500,000 undiscovered stars and more

New data from the Gaia space telescope are being called a cosmic "goldmine," including never-seen-before stars, 380 gravity-lensed quasars, and the orbits of over 150,000 asteroids.

Katja-weingrill
Laurent-galluccio
Omega-centauri
Christine-ducourant
Timo-prusti
European-space-agency
Milky-way
Data-release
Gaia-collaboration
Alexey-mints
Gaia-data-release

A super-massive Neptune-sized planet

Neptune-sized planets exhibit a wide range of compositions and densities, depending on factors related to their formation and evolution history, such as the distance from their host stars and atmospheric escape processes. They can vary from relatively low-density planets with thick hydrogen–helium atmospheres1,2 to higher-density planets with a substantial amount of water or a rocky interior with a thinner atmosphere, such as HD 95338 b (ref. 3), TOI-849 b (ref. 4) and TOI-2196 b (ref. 5). The discovery of exoplanets in the hot-Neptune desert6, a region close to the host stars with a deficit of Neptune-sized planets, provides insights into the formation and evolution of planetary systems, including the existence of this region itself. Here we show observations of the transiting planet TOI-1853 b, which has a radius of 3.46 ± 0.08 Earth radii and orbits a dwarf star every 1.24 days. This planet has a mass of 73

United-states
American
Collier-cameron
Telescopio-carlos
Monte-carlo
Exoplanet-community-early-release-science-program
Ames-research-center
Photometric-all-sky-survey
Morris
Mission-conference
International-astronomical-union
Sloan-digital-sky

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