page_title: 3247 Di Martino
hierarchical_section_title: 3247 Di Martino
caption_attribution_description: English: 3D convex shape model of 3247 Di Martino, 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: 3247 Di Martino is a dark Nysa family asteroid from the inner regions of the asteroid belt. It was discovered on 30 December 1981, by American astronomer Edward Bowell at Lowell's Anderson Mesa Station near Flagstaff, Arizona, in the United States. The asteroid has a rotation period of 5.4 hours and measures approximately 13 kilometers in diameter. It was named for Italian astronomer Mario di Martino.
context_section_description: 3247 Di Martino (prov. designation: 1981 YE) is a dark Nysa family asteroid from the inner regions of the asteroid belt. It was discovered on 30 December 1981, by American astronomer Edward Bowell at Lowell's Anderson Mesa Station near Flagstaff, Arizona, in the United States. The asteroid has a rotation period of 5.4 hours and measures approximately 13 kilometers (8 miles) in diameter. It was named for Italian astronomer Mario di Martino.
caption: Shape model of Di Martino from its lightcurve
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