A meteor shower is a celestial event where numerous meteors appear to originate from a single point in the night sky. These meteors are caused by meteoroids, streams of cosmic debris, entering Earth's atmosphere at high speeds. Typically, meteors are small, often disintegrating before reaching the surface. Intense showers, known as outbursts or storms (like the Leonids), can produce over 1,000 meteors per hour. The Meteor Data Centre lists many suspected showers, with about 100 well-established. Resources like NASA provide information on viewing opportunities and active showers.
In 1911, Irish astronomer George Johnstone Stoney, who had been calculating the position of dust at Earth's orbit, passed away.
In 1917, British astronomer Arthur Matthew Weld Downing, who had been calculating the position of dust at Earth's orbit, passed away.
In 1933, the Draconids produced a meteor storm.
In 1946, the Draconids produced a meteor storm, with zenithal hourly rates of thousands of meteors per hour.
In 1951, Fred Whipple demonstrated that comets can produce debris by water vapor drag and by breakup, envisioning comets as "dirty snowballs".
In 1951, Fred Whipple proposed that comets are "dirty snowballs" that shed meteoritic debris as their volatiles are ablated by solar energy in the inner Solar System.
The Leonid meteor storm in 1966 was one of the most intense, recording peak rates that exceeded 120,000 meteors per hour.
In 1981, Donald K. Yeomans of the Jet Propulsion Laboratory reviewed the history of meteor showers for the Leonids and the history of the dynamic orbit of Comet Tempel-Tuttle, showing relative positions of the Earth and Tempel-Tuttle and marking where Earth encountered dense dust.
In 1985, E. D. Kondrat'eva and E. A. Reznikov of Kazan State University correctly identified the years when dust was released which was responsible for several past Leonid meteor storms.
In 1994, Comet Shoemaker–Levy 9 impacted Jupiter, forming a brief trail.
In 1995, Peter Jenniskens predicted the 1995 Alpha Monocerotids outburst from dust trails.
In 1995, observations of the alpha Monocerotids demonstrated how the gravitational pull of planets affects the dust trail's path near Earth's orbit, leading to meteor showers in some years.
In 1999, there was a Leonid meteor storm.
In anticipation of the 1999 Leonid storm, Robert H. McNaught, David Asher, and Esko Lyytinen were the first to apply this method in the West.
In 2001, there were Leonid meteor storms.
In 2002, there were Leonid meteor storms.
In 2003, Peter Jenniskens argued that short-period meteor showers like Quadrantids and Geminids are from infrequent disintegrations of dormant comets.
On March 7, 2004, the panoramic camera on Mars Exploration Rover Spirit recorded a streak believed to be a meteor from a Martian meteor shower associated with comet 114P/Wiseman-Skiff.
In 2006, Jenniskens published predictions for future dust trail encounters covering the next 50 years.
A strong display was expected on December 20, 2007, from a Martian meteor shower associated with comet 114P/Wiseman-Skiff.
The IMO Meteor Shower Calendar 2017 features maps of drifting "fixed points" of meteor showers.
Finnish astronomer Esko Lyytinen predicted a potential Perseids meteor storm in August 2028, with peak rates of at least 1,000 meteors per hour possible.
Astronomers don't anticipate the next Leonid meteor storm until around 2034.
Astronomers have predicted a potentially prolific Draconid meteor storm in 2098, with peak rates potentially reaching 20,000 meteors per hour.
Astronomers don't anticipate the next Leonid meteor storm until around 2099.
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