Blending the distinctions among groups of minor bodies: a portrait of the Centaur-comet “transition” object P/2010 C1 (Scotti)

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Table 9

Model dust mass-loss rate for P/2010 C1 (Scotti).

[m²]	[kg]		[kg/s]
	Lower limit	Upper limit	Lower limit	Upper limit

3.79 × 10⁶	1.6 × 10⁵	5.1 × 10⁵	0.1	15

Notes.

^(a)

Derived dust cross-section.

^(b)

Derived dust mass in the coma annulus. The lower limit corresponds to grains in the range 10 μm−1 cm, The upper limit corresponds to grains in the range 10 μm−10 cm.

^(c)

Derived dust mass-loss rate: the lower limit corresponds to grains in the range 10 μm–1 cm crossing the projected coma annulus at v = 1 m/s, the upper limit corresponds to grains in the range 10 μm–10 cm crossing the projected coma annulus at v = 50 m/s.

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