Transient lunar phenomenon 

This map, based on a survey of 300 TLPs by Barbara Middlehurst and Patrick Moore, shows the approximate distribution of observed events. Red-hued events are in red; the remainder are yellow.
This map, based on a survey of 300 TLPs by Barbara Middlehurst and Patrick Moore, shows the approximate distribution of observed events. Red-hued events are in red; the remainder are yellow.

A transient lunar phenomenon (TLP) or "Lunar Transient Phenomena" (LTP), refers to short-lived lights, colors, or changes in appearance of the lunar surface.

Claims of short-lived phenomena go back at least 1,000 years, with some having been observed independently by multiple witnesses or reputable scientists. Nevertheless, the majority of transient lunar phenomena reports are irreproducible and do not possess adequate control experiments that could be used to distinguish among alternative hypotheses. Few reports concerning these phenomena are ever published in peer reviewed scientific journals, and rightfully or wrongfully, the lunar scientific community rarely discusses these observations.

Most lunar scientists will acknowledge that transient events such as outgassing and impact cratering do occur over geologic time: the controversy lies in the frequency of such events.

Contents

Description of events

Reports of transient lunar phenomena range from foggy patches to permanent changes of the lunar landscape. Cameron[1] classifies these as (1) gaseous, involving mists and other forms of obscuration, (2) reddish colorations, (3) green, blue or violet colorations, (4) brightenings, and (5) darkenings. Two extensive catalogs of transient lunar phenomena exist,[1][2] with the most recent tallying 2254 events going back to the 6th century. Of the most reliable of these events, at least one-third come from the vicinity of the Aristarchus plateau.

A few of the more famous historical events of transient phenomena include the following:

Explanations

Explanations for the transient lunar phenomena fall in four classes: outgassing, impact events, electrostatic phenomena, and unfavorable observation conditions.

Outgassing

Some TLPs may be caused by gas escaping from underground cavities. A number of these gaseous events are purported to display a distinctive reddish hue, while others have appeared as white clouds or an indistinct haze. The majority of TLPs appear to be associated with floor-fractured craters, the edges of lunar maria, or in other locations linked by geologists with volcanic activity. However, it should be noted that these are some of the most common targets when viewing the Moon, and this correlation could be an observational bias.

In support of the outgassing hypothesis, data from the Lunar Prospector alpha particle spectrometer indicate the recent outgassing of radon to the surface.[19] In particular, results show that radon gas was emamating from the vicinity of the craters Aristarchus and Kepler during the time of this two year mission. These observations could be explained by the slow and visually imperceptible diffusion of gas to the surface, or by discrete explosive events. In support of explosive outgassing, it has been suggested that a roughly 3 km diameter region of the lunar surface was "recently" modified by a gas release event.[20][21] However, the age of this feature is believed to be about 1 million years old, suggesting that such large phenomena occur only infrequently.

Impact events

Impact events are continually occurring on the lunar surface. The most common events are those associated with micrometeorites, as might be encountered during meteor showers. Impact flashes from such events have been detected from multiple and simultaneous Earth based observations.[22][23][24] Furthermore, impact clouds were detected following the crash of ESA's SMART-1 spacecraft.[25] Impact events leave a visible scar on the surface, and these could be detected by analyzing before and after photos of sufficiently high resolution. No impact craters having formed between the Apollo-era, Clementine (global resolution 100 metre, selected areas 7-20 metre) and SMART-1 (resolution 50 metre) missions have been identified.

Electrostatic phenomena

8 individual frames taken from a video of the Lunar crater Clavius showing the effect of the Earth´s atmosphere on astronomical images.
8 individual frames taken from a video of the Lunar crater Clavius showing the effect of the Earth´s atmosphere on astronomical images.

It has been suggested that effects related to either electrostatic charging or discharging might be able to account for some of the transient lunar phenomena. One possibility is that electrodynamic effects related to the fracturing of near surface materials could charge any gasses that might be present, such as implanted solar wind or radiogenic daughter products.[26] If this were to occur at the surface, the subsequent discharge from this gas might be able to give rise to phenomenon visible from Earth. Alternatively, it has been proposed that the triboelectric charging of particles within a gas borne dust cloud could give rise to electrostatic discharges visible from Earth.[27] Finally, electrostatic levitation of dust near the terminator could potentially give rise to some form of phenomenon visible from Earth.[28]

Unfavorable observation conditions

It is possible that many transient phenomena might not be associated with the Moon itself, but could be a result of unfavorable observing conditions or phenomenon associated with the Earth. For instance, some reported transient phenomena are for objects near the resolution of the employed telescopes. The Earth's atmosphere can give rise to significant temporal distortions that could be confused with actual lunar phenomena (see astronomical seeing). Other non-lunar explanations include the viewing of Earth orbiting satellites and meteors, or observational error.[24]

Are TLPs real?

The most significant problem that faces reports of transient lunar phenomena is that the vast majority of these were made by either a single observer, or at a single location on Earth (or both). The multitude of reports for transient phenomena occurring at the same place on the Moon could be used as evidence supporting their existence. However, in the absence of eyewitness reports from multiple observers at multiple locations on Earth for the same event, these must be regarded with caution. As discussed above, an equally plausible hypothesis for the majority of these events is that they are caused by the terrestrial atmosphere. If an event were to be observed at two different places on Earth at the same time, this could be used as evidence against an atmospheric origin.

One attempt to overcome the above problems with transient phenomena reports was made during the Clementine mission by a network of amateur astronomers. Several events were reported, of which four of these were photographed both beforehand and afterwards by the spacecraft. However, careful analysis of these images shows no discernible differences at these sites.[29] This does not necessarily imply that these reports were a result of observational error, as it is possible that outgassing events on the lunar surface might not leave a visible marker, but neither is it encouraging for the hypothesis that these were authentic lunar phenomena.

Observations are currently being coordinated by the Association of Lunar and Planetary Observers and the British Astronomical Association to re-observe sites where transient lunar phenomena were reported in the past. By documenting the appearance of these features under the same illumination and libration conditions, it is possible to judge whether some reports were simply due to a misinterpretation of what the observer regarded as an abnormality. Furthermore, with digital images it is possible to simulate atmospheric spectral dispersion, astronomical seeing blur and light scattering by our atmosphere to determine if these phenomena could explain some of the original TLP reports.

See also

References

Cited references

  1. ^ a b W. Cameron. "Analyses of Lunar Transient Phenomena (LTP) Observations from 557–1994 A.D.".
  2. ^ Barbara Middlehurst, Jaylee Burley, Patrick Moore, and Barbara Welther (1968). "Chronological Catalog of Reported Lunar Events". NASA TR R-277. 
  3. ^ Jack B. Hartung (1976). "Was the Formation of a 20-km Diameter Impact Crater on the Moon Observed on June 18, 1178?". Meteoritics 11: 187–194. 
  4. ^ "The Giordano Bruno Crater". BBC.
  5. ^ Herschel, W. (1956, May). Herschel’s ‘Lunar volcanos.’ Sky and Telescope, pp. 302-304. (Reprint of An Account of Three Volcanos in the Moon, William Herschel’s report to the Royal Society on April 26, 1787, reprinted from his Collected Works (1912))
  6. ^ Kopal, Z. (1966, December). Lunar flares. Astronomical Society of the Pacific Leaflets, 9, 401-408
  7. ^ J. F. Julius Schmidt (1867). "The Lunar Crater Linne". Astronomical register 5: 109–110. 
  8. ^ Dinsmore Alter (1959). "The Kozyrev Observations of Alphonsus". Publications of the Astronomical Society of the Pacific 71: 46–47. 
  9. ^ Greenacre, J. A. (1963, December). A recent observation of lunar color phenomena. Sky & Telescope, 26(6), 316-317
  10. ^ Zahner, D. D. (1963-64, December-January). Air force reports lunar changes. Review of Popular Astronomy, 57(525), 29, 36.
  11. ^ Ley, W. (1965). Ranger to the moon (p. 71). New York: The New American Library of World Literature, Inc.
  12. ^ Cameron, W. S. (1978, July). Lunar transient phenomena catalog (NSSDC/WDC-A-R&S 78-03). Greenbelt, MD: NASA Goddard Space Flight Center
  13. ^ Meaburn, J. (1994, June). Z. Kopal. Quarterly Journal of the Royal Astronomical Society, 35, 229-230
  14. ^ Moore, P. (2001). Thomas Rackham, 1919-2001. Journal of the British Astronomical Association, 111(5), 291.
  15. ^ Kopal, Z. & Rackham, T. W. (1963). Excitation of lunar luminescence by solar activity. Icarus, 2, 481-500
  16. ^ Kopal, Z. (1965, May). The luminescence of the moon. Scientific American, 212(5), 28
  17. ^ Kopal, Z. & Rackham, T. W. (1964, March). Lunar luminescence and solar flares. Sky & Telescope, 27(3), 140-141
  18. ^ Audouin Dollfus (2000). "Langrenus: Transient Illuminations on the Moon". Icarus 146: 430–443. doi:10.1006/icar.2000.6395. 
  19. ^ S. Lawson, W. Feldman, D. Lawrence, K. Moore, R. Elphic, and R. Belian (2005). "Recent outgassing from the lunar surface: the Lunar Prospector alpha particle spectrometer". J. Geophys. Res. 110: doi=10.1029/2005JE002433. doi:10.1029/2005JE002433 (inactive 2008-06-28). 
  20. ^ G. Jeffrey Taylor (2006). "Recent Gas Escape from the Moon". Planetary Science Research Discoveries.
  21. ^ P. H. Schultz, M. I. Staid, and C. M. Pieters (2006). "Lunar activity from recent gas release". Nature 444: 184–186. doi:10.1038/nature05303. 
  22. ^ Tony Phillips (Nov. 30, 2001). "Explosions on the Moon".
  23. ^ Brian Cudnik, David W. Palmer, David M. Palmer, Anthony Cook, Roger Venable, and Peter Gural (2003). "The Observation and Characterization of Lunar Meteoroid Impact Phenomena". Earth, Moon and Planets 93: 97–106. doi:10.1023/B:MOON.0000034498.32831.3c. 
  24. ^ a b "Lunar impact monitoring". NASA.
  25. ^ "SMART-1 impact flash and dust cloud seen by the Canada-France-Hawaii Telescope" (2006).
  26. ^ Richard Zito (1989). "A new mechanism for lunar transient phenomena". Icarus 82: 419–422. doi:10.1016/0019-1035(89)90048-1. 
  27. ^ David Hughes (1980). "Transient lunar phenomena". Nature 285: 438. doi:10.1038/285438a0. 
  28. ^ Trudy Bell and Tony Phillips (Dec. 7 2005). "New Research into Mysterious Moon Storms".
  29. ^ B. Buratti, W. McConnochie, S. Calkins, and J. Hillier (2000). "Lunar transient phenomena: What do the Clementine images reveal?". Icarus 146: 98–117. doi:10.1006/icar.2000.6373. 

General references

External links