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In this answer I have rearranged an equation from somewhere, and now I can not relocate the source. My re-aranged form is:

$$M_{Abs} = 5 \left(\log_{10}(1329) -\frac{1}{2}\log_{10}(\text{albedo}) -\log_{10}(D_{km})\right)$$

This is the relationship between the absolute magnitude of an object and its diameter and albedo, assuming it is spherical.

Question: What is a good source for any form of this equation to which I can link in my answer?

uhoh
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2 Answers2

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The JPL CNEOS asteroid size estimator and various asteroid albedo papers cite Harris and Harris 1997. That paper is behind a paywall, but Stuart and Binzel 2004 attribute this formula to it: $$ H = C - 5 \log_{10} D - 2.5 \log_{10} p_V$$ where $H$ is absolute magnitude, $p_V$ is albedo, and $C$ = 15.618.

Mike G
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  • That's numerically equivalent and so it will do, thank you! I'm still going to try to find the source that has the exact expression log${}_{10}$(1329) in my own quixocity because it bothers me that I've lost a reference (I suspect due to a variant of this). – uhoh Apr 23 '18 at 22:47
  • It may be trivial, but I finally got my $\log_{10}(1329)$. – uhoh Jan 18 '22 at 20:11
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A source of this mathematical expression is:

THE ALBEDO DISTRIBUTION OF NEAR EARTH ASTEROIDS, Edward L. Wright et.al.

This mathematical expression appears in the introduction to this article, and is attributed there to:

"Application of photometric models to asteroids", by Bowell, Edward ; Hapke, Bruce ; Domingue, Deborah ; Lumme, Kari ; Peltoniemi, Jouni ; Harris, Alan W. pages 524-556

Best regards.

Updated:

The full demonstration of the expression can be found in Appendix A of:

Binary asteroid population. Angular momentum content. P. Pravec, A.W. Harris

$$d \cdot \sqrt p=K\cdot 10^{-\frac H 5}$$

Where:

$$K=2 \ (AU)_{km} \cdot 10^{\frac{V_s}5}$$

The absolute magnitude of Sun is:

$V_s=-26.762$

$(AU)_{km}=149.6\cdot 10^6 \ km$

$$K=2 \cdot 149.6 \cdot 10^6 \cdot 10^{-\frac{26.762}5}=1329 \ km$$

Finally:

$$\boxed{H=5 \log \frac{1329}{d\cdot \sqrt p}}$$

Best regards again.

Albert
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