File:2010 UM26-2010 RN221 HST Jewitt et al. 2023.jpg

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English: Composite image showing UM26 and RN221. Tiger stripes at the upper right are caused by the inter-chip gap. The cores of both objects are clipped in order to emphasize faint structures in the sky background caused by imperfectly removed trailed field stars and galaxies. The projected antisolar and negative heliocentric velocity vectors are marked −S and −V, respectively. A scale bar shows 10″ and 15,000 km at the distance of the asteroid pair.
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Source Figure 1 from https://iopscience.iop.org/article/10.3847/1538-3881/acfc1f
Author David Jewitt, Yoonyoung Kim, Jing Li, Max Mutchler/Hubble Space Telescope/NASA

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current17:14, 12 November 2023Thumbnail for version as of 17:14, 12 November 20231,350 × 967 (1.6 MB)Nrco0e (talk | contribs)Uploaded a work by David Jewitt, Yoonyoung Kim, Jing Li, Max Mutchler/Hubble Space Telescope/NASA from Figure 1 from https://iopscience.iop.org/article/10.3847/1538-3881/acfc1f with UploadWizard

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