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19962026
most citedThe Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III

2.5k citations

Showing 2009 · astro-ph.EPShow all

13 papers · 2 filters

astro-ph.EP2009★ 130 cited

Kepler-7b: A Transiting Planet with Unusually Low Density

David W. Latham, William J. Borucki, David G. Koch +18

We report the discovery and confirmation of Kepler-7b, a transiting planet with unusually low density. The mass is less than half that of Jupiter, Mp = 0.43 Mj, but the radius is f…

astro-ph.EP2009★ 35 cited

Origin and Evolution of Saturn's Ring System

Sebastien Charnoz, Luke Dones, Larry W. Esposito +2

The origin and long-term evolution of Saturn's rings is still an unsolved problem in modern planetary science. In this chapter we review the current state of our knowledge on this…

astro-ph.EP2009★ 315 cited

Transmission Spectra of Three-Dimensional Hot Jupiter Model Atmospheres

J. J. Fortney, M. Shabram, A. P. Showman +4

We compute models of the transmission spectra of planets HD 209458b, HD 189733b, and generic hot Jupiters. We examine the effects of temperature, surface gravity, and metallicity f…

astro-ph.EP2009★ 524 cited

Cometary Origin of the Zodiacal Cloud and Carbonaceous Micrometeorites

David Nesvorny, Peter Jenniskens, Harold F. Levison +2

The zodiacal cloud is a thick circumsolar disk of small debris particles produced by asteroid collisions and comets. Here, we present a zodiacal cloud model based on the orbital pr…

astro-ph.EP2009★ 83 cited

Eclipsing Binary Trojan Asteroid Patroclus: Thermal Inertia from Spitzer Observations

Michael Mueller, Franck Marchis, Joshua P. Emery +5

We present mid-infrared (8-33 micron) observations of the binary L5-Trojan system (617) Patroclus-Menoetius before, during, and after two shadowing events, using the Infrared Spect…

astro-ph.EP2009★ 23 cited

Deciphering the Origin of the Regular Satellites of Gaseous Giants - Iapetus: the Rosetta Ice-Moon

Ignacio Mosqueira, Paul R. Estrada, Sebastien Charnoz

Here we show that Iapetus can serve to discriminate between satellite formation models. Its accretion history can be understood in terms of a two-component gaseous subnebula, with…