Eric Gaidos

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H + 3 emission is the dominant cooling mechanism in Jupiter's thermosphere and a useful probe of temperature and ion densities. The H + 3 ion is predicted to form in the thermospheres of close-in 'hot Jupiters' where its emission would be a significant factor in the thermal energy budget, affecting temperature and the rate of hydrogen escape from the(More)
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. ABSTRACT We present revised properties for 196,468 stars observed by the NASA(More)
The search for habitable planets like Earth around other stars fulfills an ancient imperative to understand our origins and place in the cosmos. The past decade has seen the discovery of hundreds of planets, but nearly all are gas giants like Jupiter and Saturn. Recent advances in instrumentation and new missions are extending searches to planets the size(More)
The phase or orbital light curves of extrasolar terrestrial planets in reflected or emitted light will contain information about their atmospheres and surfaces complementary to data obtained by other techniques such as spectrosopy. We show calculated light curves at optical and thermal infrared wavelengths for a variety of Earth-like and Earth-unlike(More)
In agreement with previous work, we show that the presence of the short-lived radionuclide 26 Al in the early Solar System was unlikely (< 2% a priori probability) to be the result of direct introduction of supernova ejecta into the gaseous disk during the Class II stage of protosolar evolution. We also show that Bondi-Hoyle accretion of any contaminated(More)
I propose to carry out a systematic investigation of planet harboring M dwarfs. Specifically, over the course of my thesis I will: i) develop and refine a new high-precision method of sub-millimagnitude " snapshot " photometry to help discover and investigate more transiting planets; ii) apply this method to differential spectroscopy; iii) calibrate(More)
  • Nicholas A Moskovitz, Eric Gaidos, Darren M Williams
  • 2008
We investigate the influence of lunar-like satellites on the infrared orbital light curves of Earth-analog extra-solar planets. Such light curves will be obtained by NASA's Terrestrial Planet Finder (TPF) and ESA's Darwin missions as a consequence of repeat observations to confirm the companion status of a putative planet and to determine its orbit. We use(More)