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HD 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 moreIn 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 a 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 — 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 planet orbits a yellow, Sun-like star called HD …
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 its atmosphere torn off at more than 35,000 …
307 Temporary Redirect - Exoplanet Exploration
WEB307 Temporary Redirect. Temporary Redirect. The document has moved here.
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 …
Exoplanets - NASA Science
WEBHD 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 …
HD 209458 | NASA Exoplanet Archive
WEBHigh angular resolution measurements of the transiting exoplanet host stars HD 189733 and HD 209458 and implications for models of cool dwarfs Boyajian et al. 2015 …
Oxygen and carbon discovered in exoplanet atmosphere 'blow-off'
WEBHD 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 propose a …
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...
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 …
CHEOPS geometric albedo of the hot Jupiter HD 209458 b
WEBMar 2, 2022 — In this Letter, we report a robust > 6σ detection of the occultation depth of HD 209458 b using the CHEOPS space telescope (Benz et al. 2021) and demonstrate that …
HD 209458 b Exoplanet Facts - Universe Guide
WEBHD 209458 b Exoplanet Facts. HD 209458 is located 161.87 light years or 49.63 parsecs from the Earth based on the latest parallax records from the Hipparcos satellite. It would …
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 – Majarra
WEBNicknamed Osiris, HD 209458 b tops a number of lists for first discoveries. It has detectable oxygen and carbon in its atmosphere, and is also evaporating at such a fast …
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 HD 209458 b
WEBEvidence against a strong thermal inversion in HD 209458 b from high-dispersion spectroscopy 2015 SCHWARZ H., BROGI M., de KOK R., BIRBY J. & SNELLEN I. …
2.1 HD 209458 b transit: discovered in a car park - OpenLearn
WEB2.1 HD 209458 b transit: discovered in a car park. HD 209458 b was originally discovered using the same technique that found 51 Pegasi b, the radial velocity method.
Exoplanets - HubbleSite
WEBJan 24, 2024 — This quest took a huge leap forward in 2000 when Hubble studied the exoplanet HD 209458 b, the first extrasolar planet known to make “transits” across the …
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 …
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 …
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