Asteroid body

Results: 27



#Item
11THE ASTRONOMICAL JOURNAL, 116 : 3029È3037, 1998 December[removed]The American Astronomical Society. All rights reserved. Printed in U.S.A. THREE-BODY MEAN MOTION RESONANCES AND THE CHAOTIC STRUCTURE OF THE ASTEROID BELT

THE ASTRONOMICAL JOURNAL, 116 : 3029È3037, 1998 December[removed]The American Astronomical Society. All rights reserved. Printed in U.S.A. THREE-BODY MEAN MOTION RESONANCES AND THE CHAOTIC STRUCTURE OF THE ASTEROID BELT

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Source URL: www.boulder.swri.edu

Language: English - Date: 2005-06-21 14:13:54
12You	
  Know	
  Where	
  the	
  Parent	
  Body	
  is	
  but	
   Where	
  are	
  the	
  Co-­‐orbitals?	
   	
     H.R.	
  Lai,	
  C.T.	
  Russell,	
  M.	
  Connors,	
  H.Y.	
  Wei,	
  G.L.	
  Delz

You  Know  Where  the  Parent  Body  is  but   Where  are  the  Co-­‐orbitals?       H.R.  Lai,  C.T.  Russell,  M.  Connors,  H.Y.  Wei,  G.L.  Delz

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Source URL: nesf2014.arc.nasa.gov

Language: English - Date: 2015-01-13 15:52:49
13Body-Fixed Coordinate Systems for Asteroid (4) Vesta Revision history:  August 20, 2012, first draft by Jian-Yang Li (Planetary Science Institute, [removed])  September 18, 2012, revised by Jian-Yang Li (Planeta

Body-Fixed Coordinate Systems for Asteroid (4) Vesta Revision history:  August 20, 2012, first draft by Jian-Yang Li (Planetary Science Institute, [removed])  September 18, 2012, revised by Jian-Yang Li (Planeta

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Source URL: sbn.psi.edu

Language: English - Date: 2013-10-18 12:53:10
14Name ________________________________ Why are many astronomical bodies round? Here is an activ ity in which you us e astronomical photogr aphs of various solar system b odies, and determine how big a body has to be befor

Name ________________________________ Why are many astronomical bodies round? Here is an activ ity in which you us e astronomical photogr aphs of various solar system b odies, and determine how big a body has to be befor

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Source URL: www.nasa.gov

Language: English - Date: 2013-04-30 20:24:10
15Sample Return Questions (from Mark, Hal and Mike) 1) How do we identify small body targets for sample return missions? Most people in the decadal feedback liked comet surface sample return and volatile-rich asteroid samp

Sample Return Questions (from Mark, Hal and Mike) 1) How do we identify small body targets for sample return missions? Most people in the decadal feedback liked comet surface sample return and volatile-rich asteroid samp

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Source URL: www.lpi.usra.edu

Language: English - Date: 2009-11-25 20:33:00
162002 GT: A 2020 Future Deep Impact Flyby Target Randal Borlase Mentor: Mike Hicks 2002 GT was first discovered in April 03, 2002 by Spacewatch (JPL Small Body Database). It has recently been of interest for a flyby from

2002 GT: A 2020 Future Deep Impact Flyby Target Randal Borlase Mentor: Mike Hicks 2002 GT was first discovered in April 03, 2002 by Spacewatch (JPL Small Body Database). It has recently been of interest for a flyby from

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Source URL: www.lacitycollege.edu

Language: English - Date: 2013-09-30 08:47:50
17Small Body Science Issues Joe Nuth, lead SBAG [removed]  Organization of Outline

Small Body Science Issues Joe Nuth, lead SBAG [removed] Organization of Outline

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Source URL: www.lpi.usra.edu

Language: English - Date: 2010-08-09 12:29:46
18Small Body Science and Technology Panel Andrew F. Cheng JHU/APL [removed]

Small Body Science and Technology Panel Andrew F. Cheng JHU/APL [removed]

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Source URL: www.lpi.usra.edu

Language: English - Date: 2011-02-19 00:28:44
19Small Body Science Issues Joe Nuth, lead SBAG [removed]  Organization of Outline

Small Body Science Issues Joe Nuth, lead SBAG [removed] Organization of Outline

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Source URL: www.lpi.usra.edu

Language: English - Date: 2011-01-25 06:01:08
20David Jewitt (UCLA) : Disintegrating Asteroid P/2013 R3 • Discovered by ground-based telescopes • Resolved by HST as multiple, evolving body • Asteroidal orbit @3AU • No dynamical path to the Kuiper belt • Fi

David Jewitt (UCLA) : Disintegrating Asteroid P/2013 R3 • Discovered by ground-based telescopes • Resolved by HST as multiple, evolving body • Asteroidal orbit @3AU • No dynamical path to the Kuiper belt • Fi

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Source URL: www.lpi.usra.edu

- Date: 2014-03-25 14:26:42