TOI-2195 A b is an inflated hot Neptune that likely originated as a Jovian planet losing ~90% mass through Roche lobe overflow during EKL-driven high-eccentricity migration triggered by a wide binary companion.
Kepler Planet-Detection Mission: Introduction and First Results
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
abstract
Super Earths, planets between 5-10 Earth masses, are the most common type of exoplanet known, yet are completely absent from our Solar system. As a result, their detailed properties, compositions, and formation mechanisms are poorly understood. NASA's Transiting Exoplanet Survey Satellite (TESS) will identify hundreds of Super-Earths orbiting bright stars, for the first time allowing in-depth characterisation of these planets. At the University of Southern Queensland, we are host to the MINERVA-Australis project, dedicated wholly to the follow-up characterisation and mass measurement of TESS planets. We give an update on the status of MINERVA-Australis and our expected performance.
fields
astro-ph.EP 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
The MINERVA-Australis facility has contributed to the discovery of 40 new exoplanets over a decade of operations confirming TESS candidates.
citing papers explorer
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Discovery of an Inflated Hot Neptune and Its Formation from Jovian Mass Loss
TOI-2195 A b is an inflated hot Neptune that likely originated as a Jovian planet losing ~90% mass through Roche lobe overflow during EKL-driven high-eccentricity migration triggered by a wide binary companion.
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Finding Alien Worlds in Queensland -- A Decade of MINERVA-Australis
The MINERVA-Australis facility has contributed to the discovery of 40 new exoplanets over a decade of operations confirming TESS candidates.