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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 …
Atmosphere of an Extrasolar Planet Detected for the First Time
WEBSep 28, 2024 · 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 …
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 …
HD 209458 | NASA Exoplanet Archive - California Institute of …
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
WEBApr 22, 2024 · 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'
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 …
The atmosphere of HD 209458b seen with ESPRESSO
WEBWe 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 …
Hubble Finds Three Surprisingly Dry Exoplanets - NASA
WEBJul 24, 2014 · The three planets, known as HD 189733b, HD 209458b, and WASP-12b, are between 60 and 900 light-years away from Earth and were thought to be ideal …
An extended upper atmosphere around the extrasolar planet
WEBMar 13, 2003 · Three transits of HD209458b (named A, B and C hereafter) were sampled in 2001 (on 7–8 September, 14–15 September and 20 October, respectively) with the …
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.
Magnetic moment and plasma environment of HD 209458b as
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 …
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 …
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 …
Broadband transmission spectroscopy of HD 209458b with …
WEBWe aim to make use of ESPRESSO high-resolution spectra, which cover two transits of HD 209458b, to probe the broadband transmission optical spectrum of the planet. Methods. …
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 …
A ground-based near-infrared emission spectrum of the exoplanet …
WEBFeb 4, 2010 · Combinations of the molecules H 2 O, CH 4, CO 2, and CO have been detected in the hot-Jupiter-type exoplanets HD 189733b and HD 209458b during …
WEBknowledge about the atmospheric chemistry via molecular abundance ratios. Combinations of the molecules H2O, CH4, CO2, and CO have been detected in the hot-Jupiter-type …
A ground-based near-infrared emission spectrum of the
WEBFeb 4, 2010 · Unlike recent results for the exoplanet HD 209458b, we find that the emergent spectrum from HD 189733b is best matched by models that do not include an …
HD 209458 – Wikipedia
WEBHD 209458, auch bekannt unter seiner Veränderlichen-Bezeichnung V376 Pegasi, ist ein Stern mit der scheinbaren Helligkeit 8 mag im Sternbild Pegasus.Der Stern ist der …
George TRAMMELL | Doctor of Philosophy | University of
WEBHot Jupiter Upper Atmospheres: Model Transit Signals in Lyman-alpha for HD 209458b. Article. Jan 2012. George Trammell. P. Arras. Z. Li. Gas giant exoplanets in tight orbits …
HD 209458 b - Viquipèdia, l'enciclopèdia lliure
WEBHD 209458 b (tot i que a vegades anomenat no oficialment Osiris) és un planeta extrasolar [9] que orbita HD 209458 en la constel·lació de Pegàs, a 150 anys llum de la Terra.S'hi …
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