Earthlight (astronomy)

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The night side of the moon, illuminated by earthshine, becomes visible next to the narrow crescent (11 percent, age of the moon = 3.3 days) with ash-grey moonlight. Image taken 20deg over the western evening sky shortly after the equinox in spring with a particularly steep ecliptic as seen from Berlin. On the left, the star Omicron Arietis (37 Ari, 6,2 ) in the constellation Aries. Aschgraues.Mondlicht.P1162513.jpg
The night side of the moon, illuminated by earthshine, becomes visible next to the narrow crescent (11 percent, age of the moon = 3.3 days) with ash-grey moonlight. Image taken 20° over the western evening sky shortly after the equinox in spring with a particularly steep ecliptic as seen from Berlin. On the left, the star Omicron Arietis (37 Ari, 6,2 ) in the constellation Aries.
During the crescent phase, the darker side of the Moon reflects indirect sunlight, reflected from Earth, while the other side reflects direct sunlight. Earth illuminates.jpg
During the crescent phase, the darker side of the Moon reflects indirect sunlight, reflected from Earth, while the other side reflects direct sunlight.
An 80 mm shot of a crescent Moon with a 10-second exposure, revealing earthshine. The green ghost image was caused by a UV filter on the lens. Earthshine-1.jpg
An 80 mm shot of a crescent Moon with a 10-second exposure, revealing earthshine. The green ghost image was caused by a UV filter on the lens.

Earthlight is the diffuse reflection of sunlight reflected from Earth's surface and clouds. Earthshine (an example of planetshine), also known as the Moon's ashen glow, is the dim illumination of the otherwise unilluminated portion of the Moon by this indirect sunlight. Earthlight on the Moon during the waxing crescent is called "the old Moon in the new Moon's arms", [1] while that during the waning crescent is called "the new Moon in the old Moon's arms". [2]

Contents

Visibility

Earthlight has a calculated maximum apparent magnitude of −17.7 as viewed from the Moon. [3] When the Earth is at maximum phase, the total radiance at the lunar surface is approximately 0.15 W m−2 from Earthlight. This is only 0.01% of the radiance from direct Sunlight. [4] Earthshine has a calculated maximum apparent magnitude of −3.69 as viewed from Earth. [3]

This phenomenon is most visible from Earth at night (or astronomical twilight) a few days before or after the day of new moon, [5] when the lunar phase is a thin crescent. On these nights, the entire lunar disk is both directly and indirectly sunlit, and is thus unevenly bright enough to see. Earthshine is most clearly seen after dusk during the waxing crescent (in the western sky) and before dawn during the waning crescent (in the eastern sky).

The term earthlight would also be suitable for an observer on the Moon seeing Earth during the lunar night, or for an astronaut inside a spacecraft looking out the window. [6] Arthur C. Clarke uses it in this sense in his 1955 novel Earthlight .

High contrast photography is also able to reveal the night side of the moon illuminated by Earthlight during a solar eclipse. [7]

Radio frequency transmissions are also reflected by the moon; for example, see Earth–Moon–Earth communication.

History

The phenomenon was sketched [8] and remarked upon in the 16th century by Leonardo da Vinci, who thought that the illumination came from reflections from the Earth's oceans (we now know that clouds account for much more reflected intensity than the oceans). [9]

It is referenced in "The Ballad of Sir Patrick Spens" (Child Ballad No. 58), in the phrase "‘A saw the new muin late yestreen/ Wi the auld muin in her airm." [10]

See also

Related Research Articles

<span class="mw-page-title-main">Moon</span> Natural satellite orbiting Earth

The Moon is Earth's only natural satellite. It orbits at an average distance of 384,400 km (238,900 mi), about 30 times the diameter of Earth. Over time Earth's gravity has caused tidal locking, causing the same side of the Moon to always face Earth. Because of this, the lunar day and the lunar month are the same length, at 29.5 Earth days. The Moon's gravitational pull – and to a lesser extent, the Sun's – are the main drivers of Earth's tides.

<span class="mw-page-title-main">Lunar phase</span> Shape of the Moons sunlit portion as viewed from Earth

A lunar phase or Moon phase is the apparent shape of the Moon's directly sunlit portion as viewed from the Earth. In common usage, the four major phases are the new moon, the first quarter, the full moon and the last quarter; the four minor phases are waxing crescent, waxing gibbous, waning gibbous, and waning crescent. A lunar month is the time between successive recurrences of the same phase: due to the eccentricity of the Moon's orbit, this duration is not perfectly constant but averages about 29.5 days.

<span class="mw-page-title-main">Planetshine</span> Illumination by reflected sunlight from a planet

Planetshine is the dim illumination, by sunlight reflected from a planet, of all or part of the otherwise dark side of any moon orbiting the body. Planetlight is the diffuse reflection of sunlight from a planet, whose albedo can be measured.

<span class="mw-page-title-main">Extraterrestrial sky</span> Extraterrestrial view of outer space

In astronomy, an extraterrestrial sky is a view of outer space from the surface of an astronomical body other than Earth.

<span class="mw-page-title-main">Astronomy Picture of the Day</span> NASA and MTU website

Astronomy Picture of the Day (APOD) is a website provided by NASA and Michigan Technological University (MTU). It reads: "Each day a different image or photograph of our universe is featured, along with a brief explanation written by a professional astronomer." The photograph does not necessarily correspond to a celestial event on the exact day that it is displayed, and images are sometimes repeated. These often relate to current events in astronomy and space exploration. The text has several hyperlinks to more pictures and websites for more information. The images are either visible spectrum photographs, images taken at non-visible wavelengths and displayed in false color, video footage, animations, artist's conceptions, or micrographs that relate to space or cosmology.

<span class="mw-page-title-main">Eratosthenes (crater)</span> Crater on the Moon

Eratosthenes crater is a relatively deep lunar impact crater that lies on the boundary between the Mare Imbrium and Sinus Aestuum mare regions. It forms the western terminus of the Montes Apenninus mountain range. It is named after ancient Greek astronomer Eratosthenes of Cyrene, who estimated the circumference of the Earth, and the distance from the Earth to the Sun.

<span class="mw-page-title-main">Moonlight</span> Light that reaches Earth from the Moon

Moonlight consists of mostly sunlight reflected from the parts of the Moon's surface where the Sun's light strikes.

<span class="mw-page-title-main">Cone Nebula</span> H II region in the constellation Monoceros

The Cone Nebula is an H II region in the constellation of Monoceros. It was discovered by William Herschel on December 26, 1785, at which time he designated it H V.27. The nebula is located about 830 parsecs or 2,700 light-years away from Earth. The Cone Nebula forms part of the nebulosity surrounding the Christmas Tree Cluster. The designation of NGC 2264 in the New General Catalogue refers to both objects and not the nebula alone.

<span class="mw-page-title-main">Far side of the Moon</span> Hemisphere of the Moon that always faces away from Earth

The far side of the Moon is the lunar hemisphere that always faces away from Earth, opposite to the near side, because of synchronous rotation in the Moon's orbit. Compared to the near side, the far side's terrain is rugged, with a multitude of impact craters and relatively few flat and dark lunar maria ("seas"), giving it an appearance closer to other barren places in the Solar System such as Mercury and Callisto. It has one of the largest craters in the Solar System, the South Pole–Aitken basin. The hemisphere has sometimes been called the "dark side of the Moon", where "dark" means "unknown" instead of "lacking sunlight" – each location on the Moon experiences two weeks of sunlight while the opposite location experiences night.

<span class="mw-page-title-main">Blanchinus (crater)</span> Crater on the Moon

Blanchinus is a lunar impact crater in the rugged south-central highlands of the Moon. It is named after Italian astronomer Giovanni Bianchini whose Latinized name is Blanchinus. Adjacent to its south is the crater Werner, and La Caille is attached to the northwest rim. To its west is the prominent formation Purbach.

<span class="mw-page-title-main">Herschel (Mimantean crater)</span>

Herschel is a large impact crater in the leading hemisphere of the Saturnian moon Mimas, centered on the equator at 112° longitude. It is named after the 18th-century astronomer William Herschel, who discovered Mimas in 1789.

A peak of eternal light (PEL) is a hypothetical point on the surface of an astronomical body that is always in sunlight. Such a peak must have high latitude, high elevation, and be on a body with very small axial tilt. The existence of such peaks was first postulated by Beer and Mädler in 1837. The pair said about the lunar polar mountains: "...many of these peaks have eternal sunshine". These polar peaks were later mentioned by Camille Flammarion in 1879, who speculated that there may exist pics de lumière éternelle at the poles of the Moon. PELs would be advantageous for space exploration and colonization due to the ability of an electrical device located there to receive solar power regardless of the time of day or day of the year, and the relatively stable temperature range.

<span class="mw-page-title-main">NGC 2440</span> Planetary nebula in the constellation Puppis

NGC 2440 is a planetary nebula, one of many in our galaxy. Its central star, HD 62166, is possibly the hottest known white dwarf, about 400,000°F(200,000°C). The nebula is situated in the constellation Puppis.

<span class="mw-page-title-main">Magnitude of eclipse</span> Fraction of the diameter of the eclipsed body which is in eclipse

The magnitude of eclipse is the fraction of the angular diameter of a celestial body being eclipsed. This applies to all celestial eclipses. The magnitude of a partial or annular solar eclipse is always between 0.0 and 1.0, while the magnitude of a total solar eclipse is always greater than or equal to 1.0, and has a theoretically maximum value of around 1.12.

<span class="mw-page-title-main">Lunar observation</span> Methods and instruments used to observe the Moon

The Moon is the largest natural satellite of and the closest major astronomical object to Earth. The Moon may be observed by using a variety of optical instruments, ranging from the naked eye to large telescopes. The Moon is the only celestial body upon which surface features can be discerned with the unaided eyes of most people.

<span class="mw-page-title-main">Lunar X</span>

The Lunar X is a clair-obscur effect in which light and shadow creates the appearance of a letter 'X' on the rim of the Blanchinus, La Caille and Purbach craters.

<span class="mw-page-title-main">Lunar south pole</span> Southernmost point on the Moon

The lunar south pole is the southernmost point on the Moon. It is of interest to scientists because of the occurrence of water ice in permanently shadowed areas around it. The lunar south pole region features craters that are unique in that the near-constant sunlight does not reach their interior. Such craters are cold traps that contain fossil record of hydrogen, water ice, and other volatiles dating from the early Solar System. In contrast, the lunar north pole region exhibits a much lower quantity of similarly sheltered craters.

In astronomy, a phase curve describes the brightness of a reflecting body as a function of its phase angle. The brightness usually refers the object's absolute magnitude, which, in turn, is its apparent magnitude at a distance of one astronomical unit from the Earth and Sun.

<span class="nowrap">2015 TB<sub>145</sub></span> Asteroid

2015 TB145 is a sub-kilometer asteroid, classified as near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 650 meters (2,000 feet) in diameter. It safely passed 1.27 lunar distances from Earth on 31 October 2015 at 17:01 UTC, and passed by Earth again in November 2018.

<span class="mw-page-title-main">Earth phase</span> Phases of the Earth as seen from the Moon

The Earth phase, Terra phase, terrestrial phase, or phase of Earth, is the shape of the directly sunlit portion of Earth as viewed from the Moon. From the Moon, the Earth phases gradually and cyclically change over the period of a synodic month, as the orbital positions of the Moon around Earth and of Earth around the Sun shift.

References

  1. Nemiroff, Robert; Bonnell, Jerry (20 January 2018). "Old Moon in the New Moon's Arms". Astronomy Picture of the Day . NASA. Archived from the original on 17 June 2019. Retrieved 11 January 2020.
  2. Nemiroff, Robert; Bonnell, Jerry (24 March 2012). "The New Moon in the Old Moon's Arms". Astronomy Picture of the Day . NASA. Archived from the original on 3 September 2019. Retrieved 11 January 2020.
  3. 1 2 Agrawal, Dulli Chandra (2016-03-30). "Apparent magnitude of earthshine: a simple calculation". European Journal of Physics. IOP Publishing. 37 (3): 035601. Bibcode:2016EJPh...37c5601A. doi:10.1088/0143-0807/37/3/035601. ISSN   0143-0807. S2CID   124231299.
  4. Glenar, David A.; et al. (March 2019). "Earthshine as an illumination source at the Moon". Icarus. 321: 841–856. arXiv: 1904.00236 . Bibcode:2019Icar..321..841G. doi:10.1016/j.icarus.2018.12.025. S2CID   90262609.
  5. The Eclectic Magazine of Foreign Literature, Science, and Art. Leavitt, Trow, & Company. 1874.
  6. Nemiroff, Robert; Bonnell, Jerry (19 April 2002). "The Old Moon in the New Moon's Arms". Astronomy Picture of the Day . NASA. Archived from the original on 3 September 2019. Retrieved 11 January 2020.
  7. Claro, Michael (October 2, 2019). "Earthshine's Faint Illumination of the Moon Captured in Glorious Eclipse Photo," Space.com. Retrieved 18 May 2023.
  8. da Vinci, Leonardo, "Moon by earthlight, Science Photo Library. Retrieved 18 May 2023.
  9. Carter, Jamie (May 15, 2023). "How to see ghostly 'Da Vinci glow' illuminate the crescent moon this week, Live Science. Retrieved 18 May 2023.
  10. Scottish anonymous (18th century or earlier; date uncertain). "Sir Patrick Spens," Scottish Poetry library. Retrieved 18 May 2023.