UK Space Frontiers 2035 Archives

Top – the total planetary flux as measured in flux units for cloud-free planetary atmospheres. Bottom – the percent contribution of reflected light to the total flux as a function of wavelength (R = 300). Colored bands in the top panel show the photometric (hashed) and spectroscopic (solid) coverage from current and future facilities over this wavelength range. Figure updated from Mayorga + (2019) and included with permission of L. C. Mayorga. -- astro-ph.IM

Astronomy & Telescopes, Atmospheres, Climate, Weather, Exoplanets, -moons, -comets, Imaging & Spectroscopy, Status Report

Transiting Exoplanets As The Immediate Future For Population-level Atmospheric Science

by Keith CowingJanuary 17, 2026January 17, 2026

The transit method, during which a planet’s presence is inferred by measuring the reduction in flux as it passes in front of its parent star, is a highly successful exoplanet […]

UK Space Frontiers 2035

Transiting Exoplanets As The Immediate Future For Population-level Atmospheric Science

How A Deep-sea Protein Adapts To An Extreme Environment

Fingerprints Inside Our Sun Could Reveal If It Once Swallowed A Planet

Climates Of Gl 514 b

Cosmic Radiation at Flight Altitudes Rises When the Sun Is Less Active

The History Of Enzyme Evolution Embedded In Metabolism