HomeHomeUpUpSearchSearchE-mailMail
NEW

Magnitude of the Moon

The magnitude of the Moon is in many cases approximated by using the formula of Allen (1973, page 144), as for instance used by Schaefer (2000, page 129). It is known that Allen's formula is not valid for large Phase Angles (>150°). A formula for a larger range is needed if one wants to perform e.g naked eye First/Last Crescent predictions (Phase Angles upto 176°). A pity that such a range is not yet (status 2022) covered by empirical data, e.g. not in the paper of Mallama&Hilton (2018). O this page a Moon magnitutde formula is proposed.

Phase curve of inner planets

Mallama&Hilton (2018, Fig. 1) have phase (relative magnitude) curves for the inner planets, see below:

Inner planets'
        magnitude

Investigating phase curve for the Moon.

As above can be seen: The behavior of inner planets' phase curve is similar for all of them. But this behavior is not similar to what Russell (1916, page 117) proposes for the Moon, which is: "the assumption that the moon’s light continues to vary nearly as the cube of the elongation from the sun is probably as good a guide as any".
The question is: Is it correct to say 'probably as good a guide as any' (as stated in 1916)? Or is it better to look at for analogical ideas from the inner planets' magnitude (of 2018).

In below graphs some tentative Moon's phase curves (black) are shown: The well-known Allen's phase curve (Moon - Allen) is the continuous black line. Russells' mean magnitude (Russell, 1916, Table III) is shown by the black triangles (Moon - Russell). A possible extrapolation of Allen is porposed by Segura González (2021, page 5) based on the above statement of Russel's cube of elongation; this results in the black dotted line (Moon - Allen&Russell).

Inner planets'
        magnitude

The Moon - Allen&Russell magnitude formula (black dotted curve) is something like

// PA = Phase Angle, r = distance Sun-Moon [in AU ~ 1] and R = distance Moon-Earth [in Earth Radii ~ 60.34]

PA=abs(PA)
Comp = 5 * log10(r * R)
If PA<=105.4065
Magn=
21.62+0.026*PA+0.000000004*PA^4+Comp
else

Magn=5.264522.33551*log10((180-PA)^3))+Comp

The Moon is much closer to the Earth than Mercury, while Mercury is closer to the Sun and has a smoother surface than the Moon (Mallama&Wang&Howard, 2002, page 260); it is not yet known (status 2022) how the Moon's magnitude behaves close to 180°. The smoother surface of Mercury could mean a relative brightness/magnitude that is higher/lower for Mercury than for the Moon.
When including the seen behavior of the inner planets (behavior seen in the above graph (Mallama, 2018, Fig. 1)) in Allen's magnitude of the Moon; Reijs derived the black dashed line (Moon - Allen&Mercury). The adjusted magnitude formula Moon - Allen&Mercury becomes:

PA=abs(PA)
Comp = 5 * log10(r * R)
If PA<=125
Magn=
‑21.62+0.026*PA+0.000000004*PA^4+Comp
else
Magn=‑21.8164+0.06328*PA‑0.0016336*PA^2+0.000033644*PA^3
0.00000034265*PA^4+0.0000000016893*PA^50.0000000000030334*PA^6+Comp

This magnitude formula though provides a increasing luminance with larger phase angles (see Segura González [2022]).

So another formula is needed, like Allen's magnitude plus Samaha's formula (see Segura González [2022], formula (3)) which has a luminance that decreases towards 180 phase angle:

PA=abs(PA)
Comp = 5 * log10(r * R)
If PA<=147.1385465
Magn=
21.62+0.026*PA+0.000000004*PA^4+Comp
else

Magn=-4.5444-2.5*log10((180-a)^3))+Comp

This has also been tested.

Remember that these magnitude formula are not empirical formulas. If you know such an empirical formula, let me know.

Testing

This Moon's magnitude formula has beeen tested as part of the sweph and ARCHAEOCOSMO package, see this page.

Acknowledgements

I would like to thank people, such as Wenceslao Segura González, Dieter Koch, Anthony Mallama, Alois Treindl and others for their help, encouragement and/or constructive feedback. Any remaining errors in methodology or results are my responsibility of course!!! If you want to provide constructive feedback, let me know.

References

Allen, C.W.: Astrophysical quantities. London, The Athlone press 1973.
Segura González, Wenceslao: Danjon limit: Helwan method. pp. 1-117  2021.
Segura González, Wenceslao: Magnitude of the Moon at large phase angles. In:  (2022).
Mallama, Anthony et al.: Photometry of Mercury from SOHO/LASCO and Earth: The phase function from 2 to 170°. In: Icarus 155  (2002), pp. 253-264.
Mallama, Anthony and James L. Hilton: Computing apparent planetary magnitudes for The Astronomical Almanac. pp. 1-64  2018.
Russell, Henry Norris: The stellar magnitudes of the Sun, Moon and planets. In: American Astronomical Society 43, pp. 103-129.
Schaefer, Brad E.: New methods and techniques for historical astronomy and archaeoastronomy. In: Archaeoastronomy: The journal of astronomy in culture XV  (2000), pp. 121-135.


Disclaimer and Copyright
HomeHomeUpUpSearchSearchE-mailMail

Major content related changes: March 1st, 2022