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.

Credit:

ESO

Over de afbeelding

Id:eso0711c
Type:Kaart
Publicatiedatum:7 maart 2007
Gerelateerde berichten:eso0711
Grootte:1555 x 1026 px

Over het object

Naam:asteroid 2000 PH5
Type:Solar System : Interplanetary Body : Asteroid
Categorie:Solar System

Afbeeldingstypen

Grote JPEG
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