In April 2007, a rotational lightcurve of Saskia was obtained from photometric observations by French amateur astronomer Pierre Antonini. Lightcurve analysis gave a well-defined rotation period of 7.348±0.001 hours with a brightness variation of 0.36 magnitude (U=3).[12][14] In December 2016, an identical period with an amplitude of 0.28 magnitude was determined by Daniel Klinglesmith at Etscorn Campus Observatory (719), New Mexico (U=3-).[13] This result supersedes two previous observations that gave a period of 7.34 and 7.349 hours, respectively (U=2/3-).[18][19]
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's WISE telescope, Saskia measures between 39.8 and 44.1 kilometers in diameter and its surface has an albedo between 0.06 and 0.112,[7][9][10][11] while the Japanese Akari satellite determined a diameter of 43.10 kilometers with an albedo of 0.069.[8] The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.10 and derives a smaller diameter of 33.69 kilometers based on an absolute magnitude of 10.48.[14]
^ abKlinglesmith, Daniel A., III (April 2017). "Spin-Shape Model Lightcurves". The Minor Planet Bulletin. 44 (2): 127–129. Bibcode:2017MPBu...44..127K. ISSN1052-8091.{{cite journal}}: CS1 maint: numeric names: authors list (link)
^Buchheim, Robert K. (September 2006). "Lightcurves of asteroids 125 Liberatrix, 461 Saskia, and 2781 Kleczek". The Minor Planet Bulletin. 33 (3): 63. Bibcode:2006MPBu...33...63B. ISSN1052-8091.
^Klinglesmith, Daniel A. III; Hanowell, Jesse; Risley, Ethan; Turk, Janek; Vargas, Angelica; Warren, Curtis Alan (October 2013). "Inversion Model Candidates". The Minor Planet Bulletin. 40 (4): 190–193. Bibcode:2013MPBu...40..190K. ISSN1052-8091.