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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 … 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 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…
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HD 209458b - NASA Science
WEBMar 12, 2003 · The planet orbits a yellow, Sun-like star called HD 209458, located 150 light-years away in the constellation Pegasus. Astronomers using the Hubble Space …
HD 209458b | Distance, Characteristics, & Facts | Britannica
WEBHD 209458b, the first extrasolar planet detected by its transit across its star’s face and the first extrasolar planet whose mass was directly measured. HD 209458 is a seventh …
Atmosphere of an Extrasolar Planet Detected for the First Time
WEB4 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 …
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HD 209458 | NASA Exoplanet Archive
WEBA uniform analysis of HD 209458b Spitzer/IRAC light curves with Gaussian process models Evans et al. 2015 | Reference Overview High-energy irradiation and mass …
Happy Anniversary, Osiris - NASA Science
WEBNov 5, 2015 · Today marks the anniversary of the discovery exoplanet HD 209458 b. Nicknamed "Osiris," after the Egyptian god of the underworld, this hot Jupiter is having …
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 …
Oxygen and carbon discovered in exoplanet atmosphere 'blow-off'
WEBScientists using the NASA / ESA Hubble Space Telescope have observed the famous extrasolar planet HD 209458b passing in front of its parent star, and found oxygen and …
Magnetic moment and plasma environment of HD …
WEBNov 21, 2014 · Transit observations of HD 209458b in the stellar Lyman-α (Lyα) line revealed strong absorption in both blue and red wings of the line interpreted as hydrogen atoms escaping from the planet’s exosphere at …
The orbital motion, absolute mass and high-altitude winds of
WEBJun 24, 2010 · Here we report high-dispersion ground-based spectroscopy of a transit of the extrasolar planet HD 209458b.
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 ...
An extended upper atmosphere around the extrasolar planet
WEBMar 13, 2003 · The planet in the system HD209458 is the first one for which repeated transits across the stellar disk have been observed 1, 2. Together with radial velocity …
Chemical fingerprint reveals a migrating exoplanet
WEBApr 14, 2021 · An international team of astronomers analyzed the light of an exoplanet labeled HD 209458b – also known as Osiris – and found as many as six molecules in …
HD 209458b - SpringerLink
WEBJan 1, 2023 · Definition. HD 209458b was the first exoplanet observed to transit its host star. History. Arguments based on simple geometry predict that about one out of ten …
The dark days are overcast: Iron-bearing clouds on HD 209458 b …
WEBAug 30, 2024 · We simulate the geometric albedo spectra of hot Jupiter exoplanets HD 209458 b and WASP-43 b, based on global climate model (GCMs) post-processed with …
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...
NASA Finds Super-Hot Planet with Unique Comet-Like Tail
WEBJul 14, 2010 · Astronomers using NASA's Hubble Space Telescope have confirmed the existence of a baked object that could be called a "cometary planet." The gas giant …
Comparative Planetary Atmospheres: Models of TrES-1 and HD …
WEBJun 7, 2005 · We present new self-consistent atmosphere models for the transiting planets TrES-1 and HD 209458b. The planets were recently observed with the Spitzer Space T …
The Transiting Exoplanets HD 209458 and TrES-1 | aavso
WEBIn 1999 the 7.7-magnitude G0V-type star in the constellation of Pegasus, HD 209458, also known as V376 Peg, was found to have a Jupiter-like planet orbiting about it. The planet, …
(PDF) A Unified Theory for the Atmospheres of the Hot and Very …
WEBHD 209458b is a long-term target for the detection of optical flux from the MOST satellite. Rowe et al. (2007) find a new 1σ upper limit to the planet-to-star flux ratio. Figure 12b …
WEBWe compare the atmosphere of HD 149026b to other well-known transiting planets, including the recently discovered HD 189733b, which we show has a planet-to-star flux …
HD 209458 — Вікіпедія
WEBhd 209458 — зірка з екзопланетою, що обертається в сузір’ї Пегаса.Її видима зоряна величина становить 7,65 [2], а абсолютна величина — 4,28 [5].Оскільки вона …
Astronomy - Extrasolar, Planetary, Systems | Britannica
WEBJul 26, 2024 · HD 209458b Artist's conception of the extrasolar planet HD 209458b, some 150 light-years from Earth. Many of these planets are unlike those of the solar system. …
HD 209458 - Vikipedi
WEBHD 209458 b, Kanatlıat takımyıldızında Güneş benzeri bir yıldız olan HD 209458 yörüngesinde dönen bir ötegezegendir. Spektroskopik çalışmalar ilk olarak 5 Kasım …
Isabelle Baraffe — Wikipédia
WEBIsabelle Baraffe est une physicienne française et professeure d'astrophysique à l' université d'Exeter. Ses recherches portent sur le développement de nouveaux modèles …
Tau Boötis b - Vikipedi
WEBTau Boötis b ya da daha net bir ifadeyle Tau Boötis Ab, yaklaşık 51 ışık yılı uzaklıkta bulunan bir ötegezegendir.Gezegen ve ana yıldızı, Uluslararası Astronomi Birliği'nin …
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