Credit & Copyright: Tunc Tezel
(TWAN)
Explanation:
This composite of images spaced some 5 to 9 days apart,
from late April (bottom right) through November 5 (top left),
traces the retrograde motion of
ruddy-colored Mars through
planet Earth's night sky.
To connect the dots and dates in this 2018 Mars retrograde loop,
just slide your cursor over the picture
(and check out this animation).
But Mars didn't actually reverse the direction of its orbit.
Instead, the apparent backwards motion with respect to the background
stars is a reflection of the motion of the Earth itself.
Retrograde motion
can be
seen each time Earth overtakes
and laps planets orbiting farther from the Sun, the
Earth moving more rapidly through its own relatively close-in orbit.
On July 27, Mars was near its favorable 2018 parihelic opposition,
when Mars was closest to the Sun in its orbit
while also
opposite the Sun in Earth's sky.
For that date, the frame used in this composite was taken during the
total lunar eclipse.
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' |
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:
Mars - Mars - protivostoyanie
Publikacii so slovami: Mars - Mars - protivostoyanie | |
Sm. takzhe:
Vse publikacii na tu zhe temu >> | |
