A meteor shower is a celestial event where numerous meteors appear to radiate from a single point in the night sky. These meteors are caused by meteoroids, small pieces of cosmic debris, entering Earth's atmosphere at high speeds. Most meteoroids are tiny and burn up completely before reaching the surface. Intense showers, known as meteor outbursts or storms, can produce thousands of meteors per hour, like the Leonids. The Meteor Data Centre recognizes hundreds of suspected showers, with about 100 well-established. Resources like NASA provide information on viewing opportunities and maps of active showers.
In 1911, Irish astronomer George Johnstone Stoney, who lived from 1826 to 1911, passed away. In the 1890s, Stoney and British astronomer Arthur Matthew Weld Downing attempted to calculate the position of dust at Earth's orbit.
In 1917, British astronomer Arthur Matthew Weld Downing, who lived from 1850 to 1917, passed away. In the 1890s, Downing and Irish astronomer George Johnstone Stoney attempted to calculate the position of dust at Earth's orbit related to meteor showers.
In 1951, Fred Whipple demonstrated that comets can produce debris by water vapor drag, envisioning them as "dirty snowballs" made up of rock embedded in ice.
In 1966 there was a Leonid storm.
In 1981, Donald K. Yeomans from the Jet Propulsion Laboratory reviewed the history of meteor showers for the Leonids and the dynamic orbit of Comet Tempel-Tuttle. He created a graph showing relative positions of Earth and the comet, and where Earth encountered dense dust, which was republished in Sky and Telescope.
In 1985, E. D. Kondrat'eva and E. A. Reznikov of Kazan State University correctly identified the years when dust released was responsible for past Leonid meteor storms.
In 1994, the Comet Shoemaker–Levy 9 impacted Jupiter, forming a brief trail.
In 1995, Peter Jenniskens predicted the 1995 Alpha Monocerotids outburst from dust trails.
Observations from the 1995 alpha Monocerotids demonstrated how the gravitational pull of planets determines where dust trails pass by Earth's orbit.
In 1999 there was a Leonid storm.
In anticipation of the 1999 Leonid storm, Robert H. McNaught, David Asher, and Esko Lyytinen were the first to apply the dust trail method in the West to predict meteor showers.
In 2001 there were two Leonid storms.
In 2002 there were two Leonid storms.
In 2003, asteroid-looking object (196256) 2003 EH1, origin of the Quadrantids, was discovered.
On March 7, 2004, the panoramic camera on Mars Exploration Rover Spirit recorded a streak believed to have been caused by a meteor from a Martian meteor shower associated with comet 114P/Wiseman-Skiff.
In 2006, Peter Jenniskens published predictions for future dust trail encounters covering the next 50 years.
A strong display from the Martian meteor shower associated with comet 114P/Wiseman-Skiff was expected on December 20, 2007.
The IMO (International Meteor Organization) Meteor Shower Calendar 2017 contains maps of drifting "fixed points".
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