Future space missions that aim to detect and characterize Earth-like exoplanets will require an instrument that efficiently measures spectra of these planets, placing strict requirements on detector performance. The upcoming […]
Earth-like Planet
Three Short-period Earth-sized Planets Around M dwarfs Discovered By TESS: TOI-5720b, TOI-6008b And TOI-6086b
One of the main goals of the NASA’s TESS (Transiting Exoplanet Survey Satellite) mission is the discovery of Earth-like planets around nearby M-dwarf stars.
Super-Earths and Earth-like Exoplanets
In the last few years astronomical surveys have expanded the reach of planetary science into the realm of small and dense extrasolar worlds. These share a number of characteristics with […]
The Impact Of Ozone On Earth-like Exoplanet Climate Dynamics: The Case Of Proxima Centauri b
The emergence of the James Webb Space Telescope and the development of other advanced observatories (e.g., ELTs, LIFE and HWO) marks a pivotal moment in the quest to characterize the […]
Purple Is The New Green: Biopigments And Spectra Of Earth-like Purple Worlds
With more than 5,500 detected exoplanets, the search for life is entering a new era. Using life on Earth as our guide, we look beyond green landscapes to expand our […]
Closeby Habitable Exoplanet Survey (CHES). I. Astrometric Noise and Planetary Detection Efficiency due to Stellar Spots and Faculae
The Closeby Habitable Exoplanet Survey (CHES) is dedicated to the astrometric exploration for habitable-zone Earth-like planets orbiting solar-type stars in close proximity, achieving unprecedented micro-arcsecond precision.
Optimized Bandpasses For The Habitable Worlds Observatory’s ExoEarth Survey
A primary scientific goal of the future Habitable Worlds Observatory will be the direct detection and characterization of Earth-like planets. Estimates of the exoplanet yields for this concept will help […]
A Gap In The Densities Of Small Planets Orbiting M Dwarfs: Rigorous Statistical Confirmation Using The Open-source Code RhoPop
Using mass-radius-composition models, small planets (R≲2R⊕) are typically classified into three types: iron-rich, nominally Earth-like, and those with solid/liquid water and/or atmosphere.
Populating The Milky Way: Characterising Planet Demographics by Combining Galaxy Formation Simulations and Planet Population Synthesis Models
Stellar populations and their distribution differ widely across the Galaxy, which is likely to affect planet demographics.
Extreme Eruption on Young Sun-like Star Signals Savage Environment for Developing Exoplanets
Astronomers have detected an extreme eruption from a young star that became more than a hundred times brighter in only a few hours.
