• LOGIN
    Login with username and password
Repository logo

BORIS Portal

Bern Open Repository and Information System

  • Publications
  • Theses
  • Research Data
  • Projects
  • Organizations
  • Researchers
  • More
  • Collections
  • Statistics
  • LOGIN
    Login with username and password
Repository logo
Unibern.ch
  1. Home
  2. Publications
  3. GRAIL Gravity Field Determination Using the Celestial Mechanics Approach

GRAIL Gravity Field Determination Using the Celestial Mechanics Approach

Details
Files
DOI
10.7892/boris.99183
Abstract
To determine the gravity field of the Moon, the NASA mission GRAIL (Gravity Recovery and Interior Laboratory) inherits its concept from the GRACE (Gravity Recovery and Climate Experiment) mission. The use of inter-satellite Ka-band range-rate (KBRR) observations enables data acquisition even when the spacecraft are not tracked from the Earth. The data allows for a highly accurate estimation of the lunar gravity field on both sides of the Moon, which is crucial to improve the understanding of its internal structure and thermal evolution. In this presentation we discuss GRAIL-based lunar gravity fields generated with the Celestial Mechanics Approach. KBRR observations and position data (GNI1B products) are used to solve for the lunar gravity field parameters in a generalized orbit determination problem. Apart from normalized spherical harmonic coefficients up to degrees n <= 200, also arc- and satellite-specific parameters, like initial state vectors and pseudo-stochastic pulses, are set up as common parameters for all measurement types. The latter shall compensate for imperfect models of non-gravitational accelerations, e.g., caused by solar radiation pressure. In addition, especially for the data of the primary mission phase, it is essential to estimate time bias parameters for the KBRR observations. We compare our results from the nominal and from the extended mission phase with the official Level 2 gravity field models first released in October 2013. Our results demonstrate that the lunar gravity field can be recovered with a high quality by adapting the Celestial Mechanics Approach, even when using pre-GRAIL or pre-SELENE gravity field models as a priori fields and when replacing sophisticated models of non-gravitational accelerations by appropriately spaced and constrained pseudo-stochastic pulses.
Date Issued
2014-04
Publication Type
Conference Item
Subject(s)
500 Science > 520 Astronomy
Language(s)
en
Author(s)
Arnold, Daniel  
Astronomisches Institut der Universität Bern (AIUB)  
Bertone, Stefano  
Astronomisches Institut der Universität Bern (AIUB)  
Jäggi, Adrian  
Astronomisches Institut der Universität Bern (AIUB)  
Beutler, Gerhard  
Emeriti, Phil.-nat. Fakultät  
Bock, Heike  
Astronomisches Institut der Universität Bern (AIUB)  
Meyer, Ulrich  
Astronomisches Institut der Universität Bern (AIUB)  
Mervart, Leos  
Astronomisches Institut der Universität Bern (AIUB)  
Additional Credits
Astronomisches Institut der Universität Bern (AIUB)  
Emeriti, Phil.-nat. Fakultät  
Journal
Geophysical research abstracts
Publisher
Copernicus Publications
ISSN
1607-7962
Title of Event
EGU General Assembly 2014
Access(Rights)
open.access
Show full item
BORIS Portal
Bern Open Repository and Information System
Build: 0eaa7c [ 7.08. 11:06]
Explore
  • Projects
  • Funding
  • Publications
  • Research Data
  • Organizations
  • Researchers
  • Audiovisual Material
  • Software & other digital items
  • Events
More
  • About BORIS Portal
  • BORIS Portal & Open Science
  • Send Feedback
  • Cookie settings
  • Service Policy
Follow us on
  • Mastodon
  • YouTube
  • LinkedIn
UniBe logo
Repository logo COAR Notify