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Hill sphere

  • The Surrender Software

    The Surrender Software

  • Monte Carlo Methods to Calculate Impact Probabilities⋆

    Monte Carlo Methods to Calculate Impact Probabilities⋆

  • Can Moons Have Moons?

    Can Moons Have Moons?

  • Constraints on the Habitability of Extrasolar Moons 3 ¯Glob Its Orbit-Averaged Global Energy flux Fs

    Constraints on the Habitability of Extrasolar Moons 3 ¯Glob Its Orbit-Averaged Global Energy flux Fs

  • Hill Sphere

    Hill Sphere

  • Journal of Physics Special Topics an Undergraduate Physics Journal

    Journal of Physics Special Topics an Undergraduate Physics Journal

  • Evolution of a Terrestrial Multiple Moon System

    Evolution of a Terrestrial Multiple Moon System

  • Diagram for Question 1 the Cosmic Perspective by Bennett, Donahue, Schneider and Voit

    Diagram for Question 1 the Cosmic Perspective by Bennett, Donahue, Schneider and Voit

  • Roche Limit.  Formation of Small Aggregates

    Roche Limit.  Formation of Small Aggregates

  • Multi-Body Mission Design in the Saturnian System with Emphasis on Enceladus Accessibility

    Multi-Body Mission Design in the Saturnian System with Emphasis on Enceladus Accessibility

  • Arxiv:1612.05945V1 [Astro-Ph.EP] 18 Dec 2016 Served for the Hot Jupiters HD 189733 B (Wyttenbach Et Al

    Arxiv:1612.05945V1 [Astro-Ph.EP] 18 Dec 2016 Served for the Hot Jupiters HD 189733 B (Wyttenbach Et Al

  • Dynamical Evolution of the Early Solar System, Because Their Spin Precession Rates Are Much Slower Than Any Secular Eigenfrequencies of Orbits

    Dynamical Evolution of the Early Solar System, Because Their Spin Precession Rates Are Much Slower Than Any Secular Eigenfrequencies of Orbits

  • Habitability of Exomoons at the Hill Or Tidal Locking Radius

    Habitability of Exomoons at the Hill Or Tidal Locking Radius

  • A Search for Satellites Around Ceres

    A Search for Satellites Around Ceres

  • A Case Study on Capturing Asteroid 2006 Rh120 and 2020

    A Case Study on Capturing Asteroid 2006 Rh120 and 2020

  • Survival of Exomoons Around Exoplanets 2

    Survival of Exomoons Around Exoplanets 2

  • The Tidal Downsizing Hypothesis of Planet Formation

    The Tidal Downsizing Hypothesis of Planet Formation

  • Four Winters of Photometry with ASTEP South at Dome C, Antarctica? N

    Four Winters of Photometry with ASTEP South at Dome C, Antarctica? N

Top View
  • The Threat of Centaurs for Terrestrial Planets and Their Orbital Evolution As Impactors
  • • Wednesday (Today): • Thursday
  • Thermal Design and Performance of the Balloon-Borne Large Aperture Submillimeter Telescope for Polarimetry Blastpol
  • The Freedom Or Soviet Space Story
  • NASA Computational Case Study Where Is My Moon 7
  • Orbital Excitation of the Giant Planets & Its Relation to the Late Heavy
  • 13Th Space Simulation Conference
  • Efficient Early Moon Devolatilisation Just After Its Formation, Through Tidally Assisted Hydrodynamic Escape
  • A New Disintegrative Capture Theory for the Origin of the Moon Peter D
  • Pebble Accretion by Bodies on Eccentric Orbits and The
  • Origin and Mineralogy of Lunar Meteorites. a Study for Lunar Mining and Resources Exploitation
  • Arxiv:2102.08611V1 [Astro-Ph.EP] 17 Feb 2021 Pebbles, Carrying Distinct Isotopic Signatures
  • Pebble Accretion by Planets on Eccentric Orbits and the Mass Ratios of Exoplanets
  • Bring: an Observatory Dedicated to Monitoring the $\Beta $ Pictoris B
  • Photometry of 2006 RH120: an Asteroid Temporary Captured Into a Geocentric Orbit
  • Download This Article in PDF Format
  • { Planetary Science }
  • THE EVOLUTION of GIANT IMPACT EJECTA and the AGE of the MOON. W.F. Bottke1, D. Vokrouhlicky2, S. Marchi1 T. Swindle3 E. R. D. Sc


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