Differentiation of the asteroid Ceres as revealed by its shape
Parker, J. Wm. ; McFadden, L. A. ; Russell, C. T. ; Stern, S. A. ; Sykes, M. V. ; Young, E. F. ; Thomas, P. C.
[s.l.] : Nature Publishing Group
Published 2005
[s.l.] : Nature Publishing Group
Published 2005
ISSN: |
1476-4687
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Source: |
Nature Archives 1869 - 2009
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Topics: |
Biology
Chemistry and Pharmacology
Medicine
Natural Sciences in General
Physics
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Notes: |
[Auszug] The accretion of bodies in the asteroid belt was halted nearly 4.6 billion years ago by the gravitational influence of the newly formed giant planet Jupiter. The asteroid belt therefore preserves a record of both this earliest epoch of Solar System formation and variation of conditions ...
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Type of Medium: |
Electronic Resource
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URL: |
_version_ | 1798293022231756800 |
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autor | Parker, J. Wm. McFadden, L. A. Russell, C. T. Stern, S. A. Sykes, M. V. Young, E. F. Thomas, P. C. |
autorsonst | Stern, S. A. Sykes, M. V. Young, E. F. Thomas, P. C. |
book_url | http://dx.doi.org/10.1038/nature03938 |
datenlieferant | nat_lic_papers |
hauptsatz | hsatz_simple |
identnr | NLZ23473468X |
insertion_date | 1911-02-25 |
issn | 1476-4687 |
journal_name | Nature |
materialart | 1 |
notes | [Auszug] The accretion of bodies in the asteroid belt was halted nearly 4.6 billion years ago by the gravitational influence of the newly formed giant planet Jupiter. The asteroid belt therefore preserves a record of both this earliest epoch of Solar System formation and variation of conditions ... |
package_name | Nature Publishing Group |
publikationsjahr_anzeige | 2005 |
publikationsjahr_facette | 2005 |
publikationsjahr_intervall | 7994:2005-2009 |
publikationsjahr_sort | 2005 |
publikationsort | [s.l.] |
publisher | Nature Publishing Group |
reference | 437 (2005), S. 224-226 |
search_space | articles |
shingle_author_1 | Parker, J. Wm. McFadden, L. A. Russell, C. T. Stern, S. A. Sykes, M. V. Young, E. F. Thomas, P. C. |
shingle_author_2 | Parker, J. Wm. McFadden, L. A. Russell, C. T. Stern, S. A. Sykes, M. V. Young, E. F. Thomas, P. C. |
shingle_author_3 | Parker, J. Wm. McFadden, L. A. Russell, C. T. Stern, S. A. Sykes, M. V. Young, E. F. Thomas, P. C. |
shingle_author_4 | Parker, J. Wm. McFadden, L. A. Russell, C. T. Stern, S. A. Sykes, M. V. Young, E. F. Thomas, P. C. |
shingle_catch_all_1 | Parker, J. Wm. McFadden, L. A. Russell, C. T. Stern, S. A. Sykes, M. V. Young, E. F. Thomas, P. C. Differentiation of the asteroid Ceres as revealed by its shape Nature Publishing Group [Auszug] The accretion of bodies in the asteroid belt was halted nearly 4.6 billion years ago by the gravitational influence of the newly formed giant planet Jupiter. The asteroid belt therefore preserves a record of both this earliest epoch of Solar System formation and variation of conditions ... 1476-4687 14764687 |
shingle_catch_all_2 | Parker, J. Wm. McFadden, L. A. Russell, C. T. Stern, S. A. Sykes, M. V. Young, E. F. Thomas, P. C. Differentiation of the asteroid Ceres as revealed by its shape Nature Publishing Group [Auszug] The accretion of bodies in the asteroid belt was halted nearly 4.6 billion years ago by the gravitational influence of the newly formed giant planet Jupiter. The asteroid belt therefore preserves a record of both this earliest epoch of Solar System formation and variation of conditions ... 1476-4687 14764687 |
shingle_catch_all_3 | Parker, J. Wm. McFadden, L. A. Russell, C. T. Stern, S. A. Sykes, M. V. Young, E. F. Thomas, P. C. Differentiation of the asteroid Ceres as revealed by its shape Nature Publishing Group [Auszug] The accretion of bodies in the asteroid belt was halted nearly 4.6 billion years ago by the gravitational influence of the newly formed giant planet Jupiter. The asteroid belt therefore preserves a record of both this earliest epoch of Solar System formation and variation of conditions ... 1476-4687 14764687 |
shingle_catch_all_4 | Parker, J. Wm. McFadden, L. A. Russell, C. T. Stern, S. A. Sykes, M. V. Young, E. F. Thomas, P. C. Differentiation of the asteroid Ceres as revealed by its shape Nature Publishing Group [Auszug] The accretion of bodies in the asteroid belt was halted nearly 4.6 billion years ago by the gravitational influence of the newly formed giant planet Jupiter. The asteroid belt therefore preserves a record of both this earliest epoch of Solar System formation and variation of conditions ... 1476-4687 14764687 |
shingle_title_1 | Differentiation of the asteroid Ceres as revealed by its shape |
shingle_title_2 | Differentiation of the asteroid Ceres as revealed by its shape |
shingle_title_3 | Differentiation of the asteroid Ceres as revealed by its shape |
shingle_title_4 | Differentiation of the asteroid Ceres as revealed by its shape |
sigel_instance_filter | dkfz geomar wilbert ipn albert |
source_archive | Nature Archives 1869 - 2009 |
timestamp | 2024-05-06T08:57:48.458Z |
titel | Differentiation of the asteroid Ceres as revealed by its shape |
titel_suche | Differentiation of the asteroid Ceres as revealed by its shape |
topic | W V WW-YZ TA-TD U |
uid | nat_lic_papers_NLZ23473468X |