NASA’s roman telescope expected to find 100000 exoplanets

NASA’s Nancy Grace Roman Space Telescope is expected to discover around 100000 previously unknown exoplanets. This would mark a major increase from the nearly 6300 worlds identified so far. The mission will survey distant regions of the Milky Way using transit and microlensing methods.

Scientists at NASA’s Goddard Space Flight Center say the telescope will monitor hundreds of millions of stars in the galactic bulge. It will search areas far beyond the few thousand light years where most known exoplanets have been found to date. Elisa Quintana noted that the effort will cover different galactic environments to study how planet formation varies across the Milky Way.

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NASA's upcoming Nancy Grace Roman Space Telescope may detect dozens of isolated neutron stars in the Milky Way through gravitational microlensing. A new study shows the observatory could measure the masses of these otherwise invisible objects. Researchers expect the mission to provide the first large sample of such stars detected solely by their gravitational effects.

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Astronomers have discovered more than 10,000 previously unidentified candidate exoplanets by re-analyzing data from NASA's Transiting Exoplanet Survey Satellite. The findings, led by Joshua Roth at Princeton University, reveal planets orbiting fainter stars up to 6800 light-years away. While many candidates may prove real, experts caution about a high false positive rate.

NASA's Fermi Gamma-ray Space Telescope has detected gamma-ray signals from the superluminous supernova SN 2017egm, providing evidence that it was powered by a rapidly spinning magnetar. The discovery marks the first confirmed gamma-ray detection from such an extreme stellar explosion. The findings were published in the journal Astronomy & Astrophysics.

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Astronomers using the James Webb Space Telescope have detected an unusually metal-poor atmosphere on the Jupiter-sized exoplanet TOI-5205 b, which orbits a small, cool star. The planet's atmospheric metallicity is lower than that of its host star, challenging theories of giant planet formation. The findings come from a study led by researchers at NASA's Goddard Space Flight Center and Carnegie Science.

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