page_title: 968 Petunia
hierarchical_section_title: 968 Petunia
caption_attribution_description: English: 3D convex shape model of 968 Petunia, computed using light curve inversion techniques. J. Hanuš, J. Ďurech, M. Brož, B. D. Warner&#32;(June 2011).&#32;"A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method". Astronomy and Astrophysics&#32;530: A134. DOI:10.1051/0004-6361/201116738. ISSN 0004-6361. arXiv
context_page_description: 968 Petunia, is a stony asteroid of the Itha family, approximately 28 kilometers in diameter, located in the outer region of the asteroid belt. It was discovered on 24 November 1921, by astronomer Karl Reinmuth at the Heidelberg Observatory in southern Germany. The bright S-type asteroid has a long rotation period of 61.3 hours. It was named after the genus of flowering plants, Petunia.
context_section_description: 968 Petunia (prov. designation: A921 WJ or 1921 KW), is a stony asteroid of the Itha family, approximately 28 kilometers (17 miles) in diameter, located in the outer region of the asteroid belt. It was discovered on 24 November 1921, by astronomer Karl Reinmuth at the Heidelberg Observatory in southern Germany. The bright S-type asteroid has a long rotation period of 61.3 hours. It was named after the genus of flowering plants, Petunia.
caption: Modelled shape of Petunia from its lightcurve
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