Grazing lunar occultation explained

A grazing lunar occultation (also lunar grazing occultation, lunar graze, or just graze) is a lunar occultation in which as the occulted star disappears and reappears intermittently on the edge of the Moon.[1] A team of many observers can combine grazes and reconstruct an accurate profile of the limb lunar terrain.

Since graze paths rarely pass over established observatories, amateur astronomers use portable observing equipment and travel to sites along the shadow path limits. The goal is to report the UTC of each event as accurately as possible, and GPS disciplined devices are frequently used as the time-base.Two methods are used to observe:

Such observations are useful for:

See also

References

  1. Book: Buchheim, R. . The Sky is Your Laboratory: Advanced Astronomy Projects for Amateurs . Springer New York . Springer Praxis Books . 2007 . 978-0-387-73995-3 . 2021-10-08 . 40.
  2. Examination of the Hipparcos Proper Motion System from Lunar Occultation Analysis. IAU Colloq. 180: Towards Models and Constants for Sub-Microarcsecond Astrometry. 115. Soma. Mitsuru. 2000tmcs.conf..115S. 2000.
  3. Sôma. Mitsuru. Kato. Yuji. 2002-01-01. Limb profiles of the Moon from grazing occultation observations collected at RGO. National Astronomical Observatory of Japan. 6. 75–105. 2002PNAOJ...6...75S.
  4. Stephenson. F. R.. Morrison. L. V.. Hohenkerk. C. Y.. 2016-12-01. Measurement of the Earth's rotation: 720 BC to AD 2015. Proc. R. Soc. A. en. 472. 2196. 20160404. 10.1098/rspa.2016.0404. 28119545. 1364-5021. 5247521. 2016RSPSA.47260404S.

Further reading

External links