Open main menu
Home
Random
Recent changes
Special pages
Community portal
Preferences
About Wikipedia
Disclaimers
Incubator escapee wiki
Search
User menu
Talk
Dark mode
Contributions
Create account
Log in
Editing
Meteoroid
(section)
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
=== In the Solar System === Most meteoroids come from the [[asteroid belt]], having been perturbed by the gravitational influences of planets, but others are particles from [[comet]]s, giving rise to [[meteor shower]]s. Some meteoroids are fragments from bodies such as Mars or the [[Moon]], that have been thrown into space by an impact. Meteoroids travel around the Sun in a variety of orbits and at various velocities. The fastest move at about {{cvt|42|km/s|mph|}} through space in the vicinity of Earth's orbit. This is [[escape velocity]] from the Sun, equal to the square root of two times Earth's speed, and is the upper speed limit of objects in the vicinity of Earth, unless they come from interstellar space. Earth travels at about {{cvt|29.6|km/s|mph|}}, so when meteoroids meet the atmosphere head-on (which only occurs when meteors are in a [[retrograde orbit]] such as the [[Leonids]], which are associated with the retrograde comet [[55P/Tempel–Tuttle]]) the combined speed may reach about {{cvt|71|km/s|mph|}} (see [[Specific energy#Astrodynamics]]). Meteoroids moving through Earth's orbital space average about {{cvt|20|km/s|mph|}},<ref>{{cite journal |author=Interagency Group (Space) Working Group on Orbital Debris |title=Report on Orbital Debris |date=February 1989 |website=NASA Technical Reports Server |page=1 |url=https://ntrs.nasa.gov/citations/19900003319 |hdl=2060/19900003319 |access-date=2023-05-31 |archive-date=2023-05-31 |archive-url=https://web.archive.org/web/20230531171611/https://ntrs.nasa.gov/citations/19900003319 |url-status=dead}}</ref> but due to Earth's gravity meteors such as the [[Phoenicids]] can make atmospheric entry at as slow as about 11 km/s. On January 17, 2013, at 05:21 PST, a one-meter-sized comet from the [[Oort cloud]] entered Earth atmosphere over [[California]] and [[Nevada]].<ref name="CAMS"/> The object had a retrograde orbit with perihelion at 0.98 ± 0.03 [[Astronomical unit|AU]]. It approached from the direction of the constellation [[Virgo (constellation)|Virgo]] (which was in the south about 50° above the horizon at the time), and collided head-on with Earth's atmosphere at {{cvt|72|±|6|km/s|mph}}<ref name="CAMS">{{cite web |title=2013 January 17 Sierra Nevada fireball |publisher=[[SETI Institute]] |first=Peter |last=Jenniskens |author-link=Peter Jenniskens |url=http://cams.seti.org/index-archive3.html |access-date=2014-11-16}} | {{cite web |url=http://www.seti.org/seti-institute/news/earth-collides-with-comet |title=Earth Collides Head-On with Small Comet |publisher=[[SETI Institute]] |access-date=2013-01-25 |archive-date=2013-01-28 |archive-url=https://web.archive.org/web/20130128052127/http://www.seti.org/seti-institute/news/earth-collides-with-comet}}</ref> vaporising more than {{cvt|100|km|ft|-4}} above ground over a period of several seconds.
Edit summary
(Briefly describe your changes)
By publishing changes, you agree to the
Terms of Use
, and you irrevocably agree to release your contribution under the
CC BY-SA 4.0 License
and the
GFDL
. You agree that a hyperlink or URL is sufficient attribution under the Creative Commons license.
Cancel
Editing help
(opens in new window)