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- Hd 209458 b sizeHD 209458b is a gas giant exoplanet that orbits an F-type star1. It is 1.38 times the size of Jupiter but has only 0.69 times its mass2. The planet takes 3.5 days to complete one orbit of its star and is 0.04707 AU from its star1. A group of investigators led by Jeremy Richardson of NASA's Goddard Space Flight Center spectrally measured HD 209458 b's atmosphere in the range of 7.5 to 13.2 micrometres3.Learn more:✕This summary was generated using AI based on multiple online sources. To view the original source information, use the "Learn more" links.Hd 209458 b sizeHD 209458 b is a gas giant exoplanet that orbits an F-type star. Its mass is 0.73 Jupiters, it takes 3.5 days to complete one orbit of its star, and is 0.04707 AU from its star.exoplanets.nasa.gov/exoplanet-catalog/6902/hd-20…Hd 209458 b sizeHD 209458b is 1.38 times the size of Jupiter but has only 0.69 times its mass.www.britannica.com/topic/HD-209458bHd 209458 b sizeA group of investigators led by Jeremy Richardson of NASA's Goddard Space Flight Center spectrally measured HD 209458 b's atmosphere in the range of 7.5 to 13.2 micrometres.en.wikipedia.org/wiki/HD_209458_b
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See all on WikipediaHD 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 … See more
Transits
Spectroscopic studies first revealed the presence of a planet around HD 209458 on November 5, 1999. Astronomers had made careful photometric measurements of several stars … See more
In 2014, a magnetic field around HD 209458 b was inferred from the way hydrogen was evaporating from the planet. It is the first (indirect) detection of a magnetic field on an exoplanet. The magnetic field is estimated to be about one tenth as strong as … See more
• Charbonneau, D. (2003). "HD 209458 and the Power of the Dark Side". In Deming, Drake; Seager, Sara (eds.). Scientific Frontiers in … See more
In August 2008, the measurement of HD 209458 b's Rossiter–McLaughlin effect and hence spin–orbit angle is −4.4 ± 1.4°.
The study in 2012, updated the spin-orbit angle to −5±7°. See more• 51 Pegasi b
• YZ Ceti another extra solar planet with evidence of magnetic fields
• HAT-P-11b another extra solar planet with evidence of magnetic fields
• Tau Boötis b another extra solar planet with evidence of … See more• "European astronomers observe first evaporating planet". Hubble Space Telescope. ESA/NASA. 2003-03-12. Archived from the original on 2008-07-07. Retrieved 2008-06-28.
• Hubble Finds Three Surprisingly Dry Exoplanets See moreWikipedia text under CC-BY-SA license HD 209458 b - NASA Science
WEBHD 209458 b is a gas giant exoplanet that orbits an F-type star. Its mass is 0.73 Jupiters, it takes 3.5 days to complete one orbit of its star, and is 0.04707 AU from its star. Its …
HD 209458b | Distance, Characteristics, & Facts | Britannica
WEBHD 209458b is 1.38 times the size of Jupiter but has only 0.69 times its mass. It orbits surprisingly close to the star—about 9 stellar radii. John Donald Fernie. Science …
HD 209458b - NASA Science
WEBMar 12, 2003 · Astronomers using the Hubble Space Telescope have made the first direct detection of the atmosphere of a planet orbiting a star outside our solar system. The …
Atmosphere of an Extrasolar Planet Detected for the First Time
WEB6 days ago · HD 209458b is estimated to be 70 percent the mass of Jupiter, or 220 times more massive than Earth. Transit observations by Hubble and ground-based telescopes …
Happy Anniversary, Osiris - NASA Science
WEBApr 22, 2024 · An artist's conception of HD 209458 b, an exoplanet whose atmosphere is being torn off at more than 35,000 km/hour by the radiation of its close-by parent star. …
Oxygen and carbon discovered in exoplanet atmosphere 'blow-off'
WEBFeb 2, 2004 · Scientists using the NASA / ESA Hubble Space Telescope have observed the famous extrasolar planet HD 209458b passing in front of its parent star, and found …
HD 209458 - Wikipedia
WEBHD 209458 is radiating 1.8 times the luminosity of the Sun from its photosphere at an effective temperature of 6,071 K. [7] Because the planet transits the star, the star is …
Open Exoplanet Catalogue - HD 209458 b
WEBThis list shows all planetary and stellar components in the system. It gives a quick overview of the hierarchical architecture. HD 209458, stellar object. HD 209458 b, planet, semi …
CHEOPS geometric albedo of the hot Jupiter HD 209458 b
WEBMar 2, 2022 · HD 209458 b has been and remains one of the most frequently studied hot Jupiters in history since its discovery in 1999 (Henry et al. 2000; Charbonneau et al. …
Exoplanets - NASA Science
WEB{"host":"HD 209458","name":"HD 209458 b","priors":{"R*":{"units":"Sol","value":"1.19","reference":"Panek%20et%20al.%202023","uncertainty":"0.02"},"RA":{"units ...
1 The first transiting planet – HD 209458 b - OpenLearn
WEBHD 209458 b orbits the star HD 209458, which is just a catalogue number. Like 51 Pegasi b, HD 209458 b is very unlike any planet in our Solar System. Its orbital period is just …
The orbital motion, absolute mass and high-altitude winds of
WEBJun 24, 2010 · We observed HD 209458 ( V = 7.65) for about five hours on the night of 7 August 2009, using the Very Large Telescope of the European Southern Observatory at …
HD 209458 b - Wikiwand
WEBHD 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 …
The atmosphere of HD 209458b seen with ESPRESSO - No …
WEBBased on the ESPRESSO spectra, we derive the stellar atmospheric parameters of HD 209458 using the Equivalent Width method by means of the STEPAR 1 code (Tabernero …
THE 4.5 μm FULL-ORBIT PHASE CURVE OF THE HOT …
WEBJul 2, 2014 · HD 209458b's observed phase curve, which represent the first 4.5 μm measurements of its nightside emission, indicates that HD 209458b has a day-to-night …
HD 209458b - SpringerLink
WEBJan 1, 2023 · Overview. HD 209458 is a star very similar to the Sun in almost all respects. Because it is relatively nearby, only 47 pc from the Sun, it has the relatively bright …
HD 209458 b - Scientific Lib
WEBHD 209458 b is an extrasolar planet that orbits the Sun-like star HD 209458 in the constellation Pegasus, some 150 light-years from Earth's solar system, with evidence of …
HD 209458 b (Osiris) Planet | 4K - YouTube
WEBFeb 18, 2024 · 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...
Broadband transmission spectroscopy of HD 209458b with …
WEBThe 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, …
WEB1. Introduction. the planet (Charbonneau et al. 2000; Henry et al. 2000; Brown et al. 2001). Of the ten known transiting planets, HD 209458 b, with a radius (at visible wavelengths) …
Scientists Estimate the Magnetic Moment of Exoplanet HD 209458b
WEBNov 21, 2014 · Planet HD 209458b (Osiris) is a hot Jupiter, approximately one-third larger and lighter than Jupiter. It is a hot gaseous giant orbiting very close to the host star HD …
Transmission Spectra of HD 209458b - IOPscience
WEBWe present the transmission spectra of the hot Jupiter HD 209458b taken with the Space Telescope Imaging Spectrograph aboard the Hubble Space Telescope. Our analysis …
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