Summary for : 2001 QC298

DynT.TT.BT T.L B T.DDensity (g/cm^3)Δρ/ρDiameter (km)ΔD/DMass (kg)ΔM/MRefAvg.M
TNO--- | --1.42 ± 0.96   (D)68 %244.0 ± 55.022.5 %1.08e+19 ± 7.00e+176 %SEVM
TNO--- | --1.42 ± 0.96   (D)68 %244.0 ± 55.022.5 %1.08e+19 ± 7.00e+176 %Sw.avg
TNO-1.41 ± 0.96   (D)68 %244.0 ± 55.022.5 %1.08e+19 ± 7.00e+176 %C?

Average asteroid densities (g/cm^3):
C = 1.3 ± 0.6, B = 2.4 ± 0.5, S = 2.7 ± 0.5, M = 3.5 ± 1.0, P = 2.8 ± 1.6, X = 1.9 ± 0.8, Xc = 4.9 ± 0.9, Xk = 4.2 ± 0.7 (Ref)

Additional resources:

Note: The density estimates have been ranked from (A) to (E), corresponding to the relative error: (B) less than 20%, (C) between 20 and 50%, (D) between 50 and 100%, and (E) more than 100%. (A) stands for (presumably) reliable estimates (accuracy better than 20%), based on more than 5 mass estimates and 5 diameter estimates, or a spacecraft encounter. Apparently unrealistic densities (ρ > 8) are tagged with (X).

EVM: average by using the Expected Value Method (Ref). w.avg: weighted average (with w = 1/err^2).

T.T: Tholen Tax Class. T.B: Bus & Binzel Tax Class. T T.L: S3OS2 Lazarro (Tholen) Tax Class. T.L B: S3OS2 Lazarro (Bus & Binzel) Tax Class. T.D: DeMeo Tax Class.

Ref: S = SiMDA, C = Carry (2012)


Diameter estimates

DesignationDiameter / Err (km)ΔD/DMethodYearRefNχ2Use
2001 QC298244.00 ± 55.0022.5 % H-mag2008D49 0.00 1

Notes (N):
1: This estimate is discarded for the average diameter (and derived density) calculation in Carry (2012).
2: This estimate is discarded for the average diameter (and derived density) calculation in SiMDA (catalog).

H-mag : Crude estimate from absolute magnitude.



EVM diam. average D = (244.0 ± 55.00) km   (ΔD/D = 23%, SNR = 4.44) Derived bulk density ρ = (1.42 ± 0.96) g/cm3   (Δρ/ρ = 68%, SNR = 1.5)



References
D49(2008):Grundy, W.M., Noll, K.S., Virtanen, J., Muinonen, K., Kern, S.D., Stephens, D.C., Stansberry, J.A., Levison, H.F., Spencer, J.R., 2008. (42355) Typhon Echidna: Scheduling observations for binary orbit determination. Icarus 197, 260–268.


Mass estimates

DesignationMass / Err (kg)ΔM/MMethodYearRefNχ2Use
2001 QC2981.08e+19 ± 7.00e+176 %BinImg 2004M400.00 1

Notes (N):
1: This estimate is discarded for the average mass (and derived density) calculation in Carry (2012).
2: This estimate is discarded for the average mass (and derived density) calculation in SiMDA (catalog).
3: This estimate is an average of individual solutions listed before under the same reference (e.g. M125).

BinImg : Binary imaged at optical wavelength.



EVM mass average M = (1.080 ± 0.070) × 1019 kg   (ΔM/M = 6%, SNR = 15.4) Derived bulk density ρ = (1.42 ± 0.96) g/cm3   (Δρ/ρ = 68%, SNR = 1.5)



References
M40(2004):Margot, J.L., Brown, M.E., Trujillo, C.A., Sari, R., 2004. HST observations of Kuiper Belt binaries, in: AAS/Division for Planetary Sciences Meeting Abstracts