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Based on data from the NASA exoplanet archive, Eyes on the Exoplanet enables uses to zoom in on more than 1000 planets orbiting distant stars.Exoplanets can be filtered by relevant criteria such as Earth-sized, large rocky planets, gas giants, etc. Distances to these planets are expressed in travel time by car, plane, etc. [9]
On 6 January 2020, NASA reported the discovery of TOI-700 d, the first Earth-sized exoplanet in the habitable zone discovered by the TESS. The exoplanet orbits the star TOI-700 100 light-years away in the Dorado constellation. [80] The TOI-700 system contains two other planets: TOI-700 b, another Earth-sized planet, and TOI-700 c, a super-Earth.
The Exoplanet Archive serves photometric time-series data from surveys that aim to discover transiting exoplanets, such as the Kepler Mission and CoRoT. The database provides access to over 22 million light curves from space and ground-based exoplanet transit survey programs, including: Kepler and K2 Public Survey Data; CoRoT Exoplanet Survey data
The Nancy Grace Roman Space Telescope will expand the search for exoplanets as well as rogue planets, or worlds that travel through space without orbiting stars.
HD 189733 b is an exoplanet in the constellation of Vulpecula approximately 64.5 light-years (19.8 parsecs) away [7] from the Solar System.Astronomers in France discovered the planet orbiting the star HD 189733 on October 5, 2005, by observing its transit across the star's face. [1]
The planet is located some 1,200 light-years away. A light-year is 5.8 trillion miles. It's the second-lightest exoplanet found so far based on its dimensions and mass, according to the ...
NASA will keep NExSS well-stocked with data to sift through. Missions over the next decade are expected to lengthen our list of exoplanets. The earliest dedicated mission, the Transiting Exoplanet ...
SWEEPS search area. SWEEPS search area detail. The stars that were monitored in this astronomical survey were all located in the Sagittarius-I Window. [2] The Sagittarius Window is a rare view to the Milky Way's central bulge stars: our view to most of the galaxy's central stars is generally blocked by lanes of dust. [3]