
WASP-43 - Wikipedia
WASP-43 is a K-type star about 284 light-years (87 parsecs) away in the Sextans constellation. It is about half the size of the Sun, and has approximately half the mass. WASP-43 has one known planet in orbit, a Hot Jupiter called WASP-43b.
WASP-43b - Wikipedia
WASP-43b, formally named Astrolábos, [2] is a transiting planet in orbit around the young, active, and low-mass star WASP-43 in the constellation Sextans. The planet is a hot Jupiter with a mass twice that of Jupiter, but with a roughly equal radius.
WASP-43 b - Science@NASA
2024年10月24日 · WASP-43 b is a gas giant exoplanet that orbits a K-type star. Its mass is 1.78 Jupiters, it takes 0.8 days to complete one orbit of its star, and is 0.0142 AU from its star. Its discovery was announced in 2011.
NASA’s Webb Maps Weather on Planet 280 Light-Years Away
2024年4月30日 · WASP-43 b is a Jupiter-sized planet roughly 280 light-years away, in the constellation Sextans. The planet orbits its star at a distance of about 1.3 million miles, completing one circuit in about 19.5 hours. Because it is so close to its star, WASP-43 b is probably tidally locked: Its rotation rate and orbital period are the same, such that ...
WASP-43 | NASA Exoplanet Archive
The orbital obliquity of three close-in massive planets hosted by dwarf K-type stars: WASP-43, HAT-P-20 and Qatar-2.
Planet WASP-43 b - Extrasolar Planets Encyclopaedia
Thirty eclipses of the ultra-short period planet WASP-43 b. Detailed information about planet WASP-43 b and its parameters.
A First Look at the JWST MIRI/LRS Phase Curve of WASP-43b
2023年1月16日 · We observed a full-orbit phase curve of the hot Jupiter WASP-43b with MIRI/LRS as part of the Transiting Exoplanet Community Early Release Science Program. Here we report preliminary findings for the instrument performance from …
[2501.03685] Characterizing WASP-43b's interior structure: …
2025年1月7日 · In this context, we aim to re-determine the orbital parameters of WASP-43b-in particular, orbital period, eccentricity, and argument of the periastron-and its orbital evolution. We study the outcomes of the tidal interaction with the host star:whether tidal decay and periastron precession are occurring in the system.
TEPCat: WASP-43 - Keele University
This page summarises the information held within TEPCat for the transiting planetary system WASP-43. Please see here for descriptions of the quantities given below. Discovery and basic observable quantities:
JWST maps the weather on exoplanet WASP-43b | WASP Planets
2024年5月6日 · JWST/MIRI phase curve of WASP-43b (Image Credit: NASA, ESA, CSA, Ralf Crawford (STScI)). “An international team of researchers has successfully used NASA’s James Webb Space Telescope to map the weather on the hot gas-giant exoplanet WASP-43 b.