The Planets

Results: 1731



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101

All planets move in ellipses. A planet that moves in a perfectly circular orbit is actually an ellipse with its eccentricity (e) = 0, a parabola has e = 1 and a hyperbola the e > 1. So the closer to zero the planets ecce

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Source URL: www.bambi.net

Language: English - Date: 2005-07-30 23:44:58
    102S
ienti
 Frontiers in Resear
h on Extr asolar Planets ASP Conferen
e Series, Vol. 294, 2003 D. Deming and S. Seager, eds. Monitoring the Planetary Transits of HD 209458b A. B. S
hultz, M. Ko
hte, W. Kinzel, F. Hamilton,

    S ienti Frontiers in Resear h on Extr asolar Planets ASP Conferen e Series, Vol. 294, 2003 D. Deming and S. Seager, eds. Monitoring the Planetary Transits of HD 209458b A. B. S hultz, M. Ko hte, W. Kinzel, F. Hamilton,

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    Source URL: www.astro.umd.edu

    Language: English - Date: 2005-01-04 16:51:56
      1031 CHAPTER 8 PLANETARY MOTIONS 8.1 Introduction The word “planet” means “wanderer” (πλάνητες αστέρες − wandering stars); in contrast to the “fixed stars”, the planets wander around on the cele

      1 CHAPTER 8 PLANETARY MOTIONS 8.1 Introduction The word “planet” means “wanderer” (πλάνητες αστέρες − wandering stars); in contrast to the “fixed stars”, the planets wander around on the cele

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      Source URL: astrowww.phys.uvic.ca

      Language: English - Date: 2011-11-09 15:20:26
        104International Journal of Astrobiology 2 (1) : 35–Printed in the United Kingdom DOI: S1473550403001368 f 2003 Cambridge University Press The habitable zone of Earth-mass planets around 47 UMa : results

        International Journal of Astrobiology 2 (1) : 35–Printed in the United Kingdom DOI: S1473550403001368 f 2003 Cambridge University Press The habitable zone of Earth-mass planets around 47 UMa : results

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        Source URL: www.uta.edu

        Language: English - Date: 2015-06-10 15:34:39
          105Predictions for the correlation between giant and terrestrial extrasolar planets in dynamically evolved systems

          Predictions for the correlation between giant and terrestrial extrasolar planets in dynamically evolved systems

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          Source URL: conference.astro.ufl.edu

          Language: English - Date: 2007-04-24 11:00:37
            106Shedding Light on the Eccentricity Valley:  Gap Heating and Eccentricity Excitation of Giant Planets in Protoplanetary Disks David Tsang (McGill), Neal J. Turner (NASA-JPL) & Andrew Cumming (McGill) arXiv:and a

            Shedding Light on the Eccentricity Valley: Gap Heating and Eccentricity Excitation of Giant Planets in Protoplanetary Disks David Tsang (McGill), Neal J. Turner (NASA-JPL) & Andrew Cumming (McGill) arXiv:and a

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            Source URL: www.tapir.caltech.edu

            Language: English - Date: 2015-11-13 11:26:29
              107Topic  2 Modeling Hot and Cold Planets

              Topic 2 Modeling Hot and Cold Planets

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              Source URL: icp.giss.nasa.gov

              Language: English - Date: 2005-09-12 15:12:24
              108Bad Honnef Physics School  Supported by the Wilhelm and Else Heraeus-Foundation Extrasolar Planets: Formation and Dynamics

              Bad Honnef Physics School Supported by the Wilhelm and Else Heraeus-Foundation Extrasolar Planets: Formation and Dynamics

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              Source URL: www.csh.unibe.ch

              Language: English - Date: 2016-02-02 06:49:51
              109Astronomis
he Gesells
haft Abstra
t Series No. 19, 2002 Abstra
ts of Contributed Talks and Posters presented at the Annual S
ienti
 Meeting of the Astronomis
he Gesells
haft

              Astronomis he Gesells haft Abstra t Series No. 19, 2002 Abstra ts of Contributed Talks and Posters presented at the Annual S ienti Meeting of the Astronomis he Gesells haft

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              Source URL: www.astronomische-gesellschaft.org

              Language: English - Date: 2015-09-07 17:00:36
              1101 CHAPTER 10 COMPUTATION OF AN EPHEMERIS 10.1 Introduction The entire enterprise of determining the orbits of planets, asteroids and comets is quite a large one, involving several stages. New asteroids and comets have to

              1 CHAPTER 10 COMPUTATION OF AN EPHEMERIS 10.1 Introduction The entire enterprise of determining the orbits of planets, asteroids and comets is quite a large one, involving several stages. New asteroids and comets have to

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              Source URL: astrowww.phys.uvic.ca

              Language: English - Date: 2012-07-10 14:30:04