Explanation: An annular eclipse of the Sun was visible in parts of the Eastern Hemisphere on Saturday. The above picture was taken at that time by a video camera in Mersing on the East Coast of Malaysia and emailed to APOD yesterday from an internet cafe in Kuala Lumpur. An annular solar eclipse will occur when the Moon's angular size is slightly less than the Sun's angular size. Therefore, when the Moon is directly in front of the Sun, the edges of the Sun are still visible. This solar ring is so bright that the Moon's surface normally appears dark by comparison. The angular sizes of the Sun and Moon change slightly because of the elliptical nature of the Moon's and Earth's orbit. A total solar eclipse would have occurred were the Moon much closer to the Earth.

<<  Avgust  >> Pn Vt Sr Cht Pt Sb Vs           1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31             1995   1996   1997 1998   1999   2000 2001   2002   2003 2004   2005   2006 2007   2008   2009 2010   2011   2012 2013   2014   2015 2016   2017   2018 2019   2020   2021 2022   2023   2024

Yanvar' Fevral' Mart Aprel' Mai Iyun' Iyul' Avgust Sentyabr' Oktyabr' Noyabr' Dekabr'

Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publikacii s klyuchevymi slovami: Sun - eclipse - Moon - Solnechnoe zatmenie - Solnce - Luna - kol'ceobraznoe solnechnoe zatmenie Publikacii so slovami: Sun - eclipse - Moon - Solnechnoe zatmenie - Solnce - Luna - kol'ceobraznoe solnechnoe zatmenie
Sm. takzhe: Zahod Zemli s "Oriona" Apollon-12 i Serveior-3 Ognennoe kol'co nad ostrovom Pashi Kol'ceobraznoe zatmenie nad Patagoniei Zatmenie na voshode Naidite cheloveka na Lune "Muna Liza" Vse publikacii na tu zhe temu >>