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Physical and Mutual Orbit Characteristics of Near-Earth Binary Asteroid (163693) Atira

  • Authors: Aaron P. Deleon, Sean E. Marshall, Tracy M. Becker, Petr Pravec, Ellen S. Howell, Michael C. Nolan, Anne K. Virkki, Edgard G. Rivera-Valentín, Patrick A. Taylor, Bryce T. Bolin, Beth Aponte-Hernández, Israel Cabrera, Peter Kušnirák, Kamil Hornoch, Hana Kučáková

Aaron P. Deleon et al 2024 The Planetary Science Journal 5 .

  • Provider: AAS Journals

Caption: Figure 8.

Resulting CW (opposite-sense) models for the two overall best-fitting models. (a) and (b) are ecliptic longitude, ecliptic latitude (150°, −10°); (c) and (d) are ecliptic longitude, ecliptic latitude (187°, −53°). The red line is the observation, and the blue line is the model. The 3D model in the top right of each frame shows the plane-of-sky view at the time of observation.

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