
Observable consequences of planet formation models in systems with close-in terrestrial planets. Migration and the formation of systems of hot super-Earths and Neptunes. On the migration-induced resonances in a system of two planets with masses in the Earth mass range. A dynamical analysis of the Kepler-80 system of five transiting planets. Solar system moons as analogs for compact exoplanetary systems. The minimum-mass extrasolar nebula: in situ formation of close-in super-Earths. Mass-radius relation for rocky planets based on PREM. The use of transit timing to detect terrestrial-mass extrasolar planets. On detecting terrestrial planets with timing of giant planet transits. Thirty eclipses of the ultra-short period planet WASP-43 b. The TRAPPIST survey of southern transiting planets. Life-sustaining planets in interstellar space? Nature 400, 32 (1999) 3D climate modelling of close-in land planets: circulation patterns, climate moist instability, and habitability. Habitable zones around main-sequence stars: new estimates. A resonant chain of four transiting, sub-Neptune planets. On the evolution of multiple protoplanets embedded in a protostellar disc. Habitable worlds with JWST: transit spectroscopy of the TRAPPIST-1 system? Mon. A combined transmission spectrum of the Earth-sized exoplanets TRAPPIST-1 b and c. Temperate Earth-sized planets transiting a nearby ultracool dwarf star. Moreover, the seven planets have equilibrium temperatures low enough to make possible the presence of liquid water on their surfaces 6, 7, 8. This architecture suggests that the planets formed farther from the star and migrated inwards 4, 5. The six inner planets form a near-resonant chain, such that their orbital periods (1.51, 2.42, 4.04, 6.06, 9.1 and 12.35 days) are near-ratios of small integers. Our observations reveal that at least seven planets with sizes and masses similar to those of Earth revolve around TRAPPIST-1. Here we report the results of a photometric monitoring campaign of that star from the ground and space. The transiting configuration of these planets, combined with the Jupiter-like size of their host star-named TRAPPIST-1-makes possible in-depth studies of their atmospheric properties with present-day and future astronomical facilities 1, 2, 3. Recently, three Earth-sized planets were detected that transit (that is, pass in front of) a star with a mass just eight per cent that of the Sun, located 12 parsecs away 1. These codes are expired and CANNOT be redeemed.One aim of modern astronomy is to detect temperate, Earth-like exoplanets that are well suited for atmospheric characterization.

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If there is a code that is in the available codes section but doesn't work, let us know so it can be moved!Ī: In the beginning of October. But there usually are codes during major holidays like Christmas and SSO's birthday etc.Ī: If the code has an (expired) tag after it, it doesn't work anymore.


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