In 2009, Photometric observations of this asteroid were made at the Palmer Divide Observatory in Colorado Springs, Colorado. The resulting asymmetrical light curve shows a synodic rotation period of 9.156 ± 0.001 hours with a brightness variation of 0.37 ± 0.02 in magnitude. This is consistent with the result of an independent study performed in 1965.
- Kryszczynska, A.; et al. (October 2012). "Do Slivan states exist in the Flora family?. I. Photometric survey of the Flora region". Astronomy & Astrophysics. 546: 51. Bibcode:2012A&A...546A..72K. doi:10.1051/0004-6361/201219199. A72.
- Yeomans, Donald K., "364 Isara", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 2013-03-25.
- Warner, Brian D. (October 2009), "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2009 March-June", The Minor Planet Bulletin, 36 (4), pp. 172–176, Bibcode:2009MPBu...36..172W, doi:10.1016/j.pss.2012.03.009.
- 364 Isara at the JPL Small-Body Database
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