Change in the rotation of 2000 PH5

Relative change in the rotation period as a function of time. The observed relative variation in the rotation period is seen to change from year to year (black dots). The solid curve is the expected theoretical YORP strength derived from the 3-D shape model.

Kilde:

ESO

Om billedet

Id:eso0711c
Type:Diagram
Udgivelsesdato:7. marts 2007
Relaterede pressemeddelelser:eso0711
Størrelse:1555 x 1026 px

Om objektet

Navn:asteroid 2000 PH5
Type:Solar System : Interplanetary Body : Asteroid
Kategori:Solar System

Billedformater

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Skrærm JPEG
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