754 Malabar

It was discovered in 1906 by German astronomer August Kopff from Heidelberg, and was named in honor of a Dutch-German solar eclipse expedition to Christmas Island in 1922.

[5] This object is orbiting at a distance of 2.99 AU from the Sun with a period of 5.16 years and an eccentricity (ovalness) of 0.048.

[3] Photometric measurements of this asteroid made in 2003 resulted in a light curve showing a rotation period of 11.740±0.005 h and a brightness variation of 0.45±0.03 in magnitude.

[5] This is a Ch-class asteroid in the Bus asteroid taxonomy, showing a broad absorption band in its carbonaceous spectrum near a wavelength of 0.7 μm.

This feature is interpreted as due to iron-bearing phyllosilicates on the surface.