The colour of the dark side of the Moon
(2014) In Astronomy & Astrophysics 563.- Abstract
- Aims. "Earthshine" is the dim light seen on the otherwise dark side of the Moon, particularly when it is close to new. "Earthlight", or reflected sunlight from the Earth, is the source of Earthshine. Using B and V band CCD images of both the dark and bright sides of the Moon, we aim to estimate the Johnson photometry B V colour of the Earthshine for the first time since the late 1960s. From these measurements we are also able to quantify the colour of Earthlight. Methods. We present images of the Moon taken with a small refractor in Hawaii, in B and V bands and taken under favourable conditions so that scattered light in both bands almost completely cancels, yielding a map of the surface in B V colour. Co-addition of 100 such images taken... (More)
- Aims. "Earthshine" is the dim light seen on the otherwise dark side of the Moon, particularly when it is close to new. "Earthlight", or reflected sunlight from the Earth, is the source of Earthshine. Using B and V band CCD images of both the dark and bright sides of the Moon, we aim to estimate the Johnson photometry B V colour of the Earthshine for the first time since the late 1960s. From these measurements we are also able to quantify the colour of Earthlight. Methods. We present images of the Moon taken with a small refractor in Hawaii, in B and V bands and taken under favourable conditions so that scattered light in both bands almost completely cancels, yielding a map of the surface in B V colour. Co-addition of 100 such images taken in rapid succession substantially improves the signal-to-noise ratio, and several sources of photometric bias are eliminated by use of relative methods. Results. The earthlit dark side of the Moon is observed to be 0.150 +/- 0.005 mag bluer in B V than the sunlit bright side, in good agreement with the only known previous measurement of this quantity from 1967. Arguing on the basis of the change in B V for sunlight reflected once off the Moon, we derive a colour for earthlight of B V = 0.44 +/- 0.02 mag (without applying a small, uncertain, phase-dependent reddening correction). The absence of a colour-gradient in the B V image implies that the scattering properties of the atmosphere+optical system are almost exactly matched in the two wavelength bands, the consequences of which are discussed. (Less)
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/4439901
- author
- Thejll, P. ; Flynn, C. ; Gleisner, H. ; Andersen, Torben LU ; Ulla, A. ; Owner-Petersen, Mette LU ; Darudi, A. and Schwarz, H.
- organization
- publishing date
- 2014
- type
- Contribution to journal
- publication status
- published
- subject
- keywords
- atmospheric effects, Earth, techniques: image processing, techniques:, photometric, planets and satellites: surfaces, Moon
- in
- Astronomy & Astrophysics
- volume
- 563
- article number
- A38
- publisher
- EDP Sciences
- external identifiers
-
- wos:000333798000038
- scopus:84896886706
- ISSN
- 0004-6361
- DOI
- 10.1051/0004-6361/201322776
- language
- English
- LU publication?
- yes
- id
- 8da23c25-7bac-42df-9e80-ce791fc9907f (old id 4439901)
- date added to LUP
- 2016-04-01 14:36:01
- date last changed
- 2022-12-12 00:37:48
@article{8da23c25-7bac-42df-9e80-ce791fc9907f,
abstract = {{Aims. "Earthshine" is the dim light seen on the otherwise dark side of the Moon, particularly when it is close to new. "Earthlight", or reflected sunlight from the Earth, is the source of Earthshine. Using B and V band CCD images of both the dark and bright sides of the Moon, we aim to estimate the Johnson photometry B V colour of the Earthshine for the first time since the late 1960s. From these measurements we are also able to quantify the colour of Earthlight. Methods. We present images of the Moon taken with a small refractor in Hawaii, in B and V bands and taken under favourable conditions so that scattered light in both bands almost completely cancels, yielding a map of the surface in B V colour. Co-addition of 100 such images taken in rapid succession substantially improves the signal-to-noise ratio, and several sources of photometric bias are eliminated by use of relative methods. Results. The earthlit dark side of the Moon is observed to be 0.150 +/- 0.005 mag bluer in B V than the sunlit bright side, in good agreement with the only known previous measurement of this quantity from 1967. Arguing on the basis of the change in B V for sunlight reflected once off the Moon, we derive a colour for earthlight of B V = 0.44 +/- 0.02 mag (without applying a small, uncertain, phase-dependent reddening correction). The absence of a colour-gradient in the B V image implies that the scattering properties of the atmosphere+optical system are almost exactly matched in the two wavelength bands, the consequences of which are discussed.}},
author = {{Thejll, P. and Flynn, C. and Gleisner, H. and Andersen, Torben and Ulla, A. and Owner-Petersen, Mette and Darudi, A. and Schwarz, H.}},
issn = {{0004-6361}},
keywords = {{atmospheric effects; Earth; techniques: image processing; techniques:; photometric; planets and satellites: surfaces; Moon}},
language = {{eng}},
publisher = {{EDP Sciences}},
series = {{Astronomy & Astrophysics}},
title = {{The colour of the dark side of the Moon}},
url = {{http://dx.doi.org/10.1051/0004-6361/201322776}},
doi = {{10.1051/0004-6361/201322776}},
volume = {{563}},
year = {{2014}},
}