Credit & Copyright: John Gleason
(Celestial Images)
Explanation:
In 1997,
Comet Hale-Bopp's intrinsic brightness exceeded any comet since
1811.
Since it peaked on the other side of the Earth's orbit,
however, the comet appeared only brighter than any comet in
two decades.
Visible above are the
two tails shed by
Comet Hale-Bopp.
The
blue ion tail is composed of
ionized gas molecules, of which
carbon monoxide
particularly glows blue when reacquiring
electrons.
This tail is created by the particles from the fast
solar wind interacting
with gas from the comet's head.
The blue
ion tail points directly away from the
Sun.
The light colored
dust tail is created
by bits of grit that have come off the
comet's nucleus
and are being pushed away by the
pressure of light from the Sun.
This tail points nearly away from the Sun.
The above photograph was taken in March 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 |
Январь Февраль Март Апрель Май Июнь Июль Август Сентябрь Октябрь Ноябрь Декабрь |
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
|
Публикации с ключевыми словами:
Comet Hale-Bopp - comet tail - комета Хейла-Боппа - кометные хвосты
Публикации со словами: Comet Hale-Bopp - comet tail - комета Хейла-Боппа - кометные хвосты | |
См. также:
Все публикации на ту же тему >> | |
