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HD 209458 b - NASA Science
HD 209458 b is a gas giant exoplanet that orbits an F-type star. Learn about its mass, orbit, discovery method, and more from NASA's Exoplanet Catalog.
Other content from science.nasa.govHD 209458 b - Wikipedia
HD 209458 b is an exoplanet that orbits the solar analog HD 209458 in the constellation Pegasus, some 157 light-years (48 parsecs) from the Solar System. The radius of the planet's orbit is 0.047 AU (7.0 million km; 4.4 million mi), or one-eighth the radius of Mercury's orbit (0.39 AU (36 million mi; 58 million km)). This small radius results in a year that is 3.5 Earth-days long and an estimated surf…
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HD 209458 - Wikipedia
HD 209458 is a star with an orbiting exoplanet in the constellation Pegasus. It has an apparent visual magnitude of 7.65 and an absolute magnitude of 4.28. Because it is located at a distance of 157 light-years (48 parsecs) from the Sun as measured via parallax, it is not visible to the unaided eye. With good binoculars or a small telescope it should be easily detectable. The system is drifting closer wi…
Wikipedia · Text under CC-BY-SA license- Estimated Reading Time: 6 mins
HD 209458b - NASA Science
Mar 12, 2003 · Learn about HD 209458b, a 'hot Jupiter' that orbits very close to its star and has a evaporating atmosphere. See the first Hubble observations of an extrasolar planet atmosphere and how it may lose its mass.
Happy Anniversary, Osiris - NASA Science
Nov 5, 2015 · HD 209458 b is the first exoplanet discovered by the transit method and the first with a detectable atmosphere. It orbits very close to its star and loses gas at more than 35,000 km/hour, creating a carbon and oxygen envelope …
Atmosphere of an Extrasolar Planet Detected for the First Time
5 days ago · HD 209458b is a hot Jupiter that orbits very close to its star and has a sodium-rich atmosphere. Astronomers used Hubble's spectrometer to analyze the light passing through …
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HD 209458b | Distance, Characteristics, & Facts | Britannica
HD 209458b is the first planet detected by transit and the first with measured mass. It is a Jupiter-like planet with strong winds and a short orbit around a Sun-like star.
Exoplanet Exploration
HD 209458 b is a super-Earth planet orbiting a Sun-like star at 0.05 AU. It has a highly eccentric orbit, a low albedo, and a long period of 3.5 days. See its physical and orbital properties, …
HD 209458 | NASA Exoplanet Archive
24 rows · High angular resolution measurements of the transiting exoplanet host stars HD 189733 and HD 209458 and implications for models of cool dwarfs. New and updated stellar …
The atmosphere of HD 209458b seen with ESPRESSO
We observed two transits of the iconic gas giant HD 209458b between 380 and 780 nm, using the high-resolution ESPRESSO spectrograph. The derived planetary transmission spectrum …
Oxygen and carbon discovered in exoplanet atmosphere 'blow-off'
Feb 2, 2004 · HD 209458b, also known as Osiris, is a hot Jupiter that evaporates hydrogen, oxygen and carbon at a high rate. Scientists use Hubble to observe its atmosphere and …
ESA - Artist's impression of exoplanet HD 209458 b
Mar 20, 2023 · The NASA/ESA Hubble Space Telescope became the first satellite to ever measure the composition of an atmosphere of an exoplanet. HD 209458 b is a popular target for space missions, being also revisited by ESA’s Cheops mission in 2020.
HD 209458 b (Osiris) Planet | 4K - YouTube
HD 209458 b, nicknamed "Osiris" after the Egyptian god of the underworld, is an exoplanet that orbits the solar analog HD 209458 in the constellation Pegasus...
The orbital motion, absolute mass and high-altitude winds of
Jun 24, 2010 · Here, high-dispersion ground-based spectroscopy of a transit of the extrasolar planet HD 209458b is reported. This allowed the radial component of the planet's orbital …
Broadband transmission spectroscopy of HD 209458b with …
The detection of a giant planet orbiting the bright solar-type star HD 209458 represents a major cornerstone in exoplanet research. First detected using the radial velocity method, HD 209458 …
HD 209458 b - Wikiwand
HD 209458 b is an exoplanet that orbits the solar analog HD 209458 in the constellation Pegasus, some 157 light-years from the Solar System. The radius of the planet's orbit is 0.047 AU, or …
Transmission Spectra of HD 209458b - IOPscience
We present the transmission spectra of the hot Jupiter HD 209458b taken with the Space Telescope Imaging Spectrograph aboard the Hubble Space Telescope. Our analysis …
THE 4.5 μm FULL-ORBIT PHASE CURVE OF THE HOT JUPITER HD 209458b
Jul 2, 2014 · HD 209458b is predicted to be in synchronous rotation about its host star with a hot spot that is shifted eastward of the substellar point by superrotating equatorial winds. Here we present the first full-orbit observations of HD 209458b, in which its 4.5 μm emission was recorded with Spitzer /IRAC.
HD 209458 b - Wikipedia, la enciclopedia libre
HD 209458 b es un planeta extrasolar que orbita la estrella de tipo solar HD 209458 en la constelación de Pegaso a 150 años luz de nuestro sistema solar. El planeta ha sido llamado …
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