1995
DOI: 10.1016/0032-0633(95)00127-1
|View full text |Cite
|
Sign up to set email alerts
|

The slow rotation of 253 Mathilde

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

0
30
0

Year Published

1996
1996
2003
2003

Publication Types

Select...
10

Relationship

0
10

Authors

Journals

citations
Cited by 49 publications
(30 citation statements)
references
References 11 publications
0
30
0
Order By: Relevance
“…MSI has rectangular pixels (27 × 16 µm), corresponding to 162 × 96 µrad/pixel. constraint on the spin period of Mathilde, which according to Mottola et al (1995) is 417 h (with a lightcurve amplitude of 0.45 mag). No changes in shadow positions were noted over a period of some 10 min when the highest resolution views are available, from which Thomas et al set a lower limit of 1.8 days on Mathilde's spin period.…”
Section: Shape Size and Mean Densitymentioning
confidence: 99%
“…MSI has rectangular pixels (27 × 16 µm), corresponding to 162 × 96 µrad/pixel. constraint on the spin period of Mathilde, which according to Mottola et al (1995) is 417 h (with a lightcurve amplitude of 0.45 mag). No changes in shadow positions were noted over a period of some 10 min when the highest resolution views are available, from which Thomas et al set a lower limit of 1.8 days on Mathilde's spin period.…”
Section: Shape Size and Mean Densitymentioning
confidence: 99%
“…These data provide an excellent range of viewing angles, although parts of the southern area of the asteroid were viewed over only a very small range of aspects. Because of the slow rotation rate (418 h; Mottola et al 1995), lighting was effectively constant during the 25-min encounter.…”
Section: Data and Techniquesmentioning
confidence: 99%
“…Mathilde is a large Ctype asteroid [Binzel et al, 1996] of mean diameter -60 km that has been recently discovered to have an anomalously large rotation period of 17.4 days [Mottola et al, 1995]. This rotation is more than an order of magnitude slower than that of typical asteroids.…”
Section: Mission Backgroundmentioning
confidence: 99%