The annual Leonid meteor shower hit its regular peak over the weekend, but stargazers who missed the event caught the second act of the shooting stars show late on Monday, Nov. 19 and early on Tuesday, Nov. 20.

 

November is the time of the Leonid meteor shower, when the meteors come swarming into our night sky view every as the Earth passes through a debris stream from an ancient comet. These ultra-swift light streaks appear to emanate from out of the constellation of Leo (hence the name, "Leonid"), a star pattern that currently  rises in the northeast at 11 p.m. local time, and remains in view for the rest of the night. 

 

The traditional peak for the Leonids occurred before dawn on the morning of Nov. 17. Many reports however, indicate that this year's display was unusually weak, with most people reporting no more than five to 10 meteors per hour. 

 

But it was not the end of the Leonids for this year. The year 2012 offered some of us another chance early on Nov. 20 when the Earth passed through another Leonids debris stream.

 

Leonid's comet legacy

The Leonid meteor shower is created by debris from the comet Tempel-Tuttle, which orbits the sun every 33 years. During the closest approach to the sun, the star's heat causes some of the comet’s ice to crumble off, taking some dusty debris with it. Those lanes of debris are what Earth passes through each November to create the Leonids.

 

The average Leonid visible to the naked eye is scarcely larger than a grain of sand. We know them best when they reach the Earth's upper atmosphere and flare into streaks of light from friction with the rarefied air. They enter the atmosphere at an immense velocity — 45 miles per second (72 kilometers per second), or 162,000 mph (261,000 kph) — and its kinetic energy is used up in such processes as the instantaneous production of light, heat and ionization.

 

Thus, such a small particle can be seen as a “shooting star” from more than 100 miles away. Obviously, however, it's really the light energy that it develops and not the particle itself that we see.

 

 

How to see 600-year-old comet dust

This year the best time to look for the Leonids might actually come in the early morning hours of Tuesday, Nov. 20. Two veteran experts in the field of meteor science, Jérémie Vaubaillonof France and Mikhail Maslov of Russia, have independently calculated that the Earth is on target to pass directly through a small clump of dust shed by comet Tempel-Tuttle when it swept around the sun in the year 1400 A.D. [How Meteor Showers Work (Infographic)]

 

That interaction is expected to occur between about 12:30 a.m. and 3:00 a.m. EST, meaning that those living in eastern North America should have the best views. Maslov is forecasting 12:36 a.m. EST, while Vaubaillon says it will occur at 2:58 a.m. EST.

 

Still, don’t expect a tremendous number of meteors. Maslov, in fact, believed the display will likely not exceed 15 Leonids per hour as seen from a dark sky location (even less if you’re trying to watch from a brightly-lit city).  Vaubaillon, meanwhile, concurs: "The density of particles doesn't look very high. Maybe a brief outburst at best."

 

Super-bright fireball meteors?

When a comet releases particles into space most are indeed the size of dust and sand grains, but there are also some larger pieces too, ranging from pebble size to perhaps a child’s marble. Those kinds of pieces can create outstandingly bright meteors, or "fireballs," perhaps even meteors that explode in their flight across the sky, known as "bolides."

 

After a number of revolutions around the sun, most of the dust-sized particles become dispersed so only the larger pieces remain. Time is of no human consequence to these meteors. In the case of the clump of particles shed by Tempel-Tuttle in 1400, it has circled the sun 18 times. So if there’s anything left out there in space, there might at least be some of those larger pebble-sized pieces. [Surprise Fireball Lights Up U.K. Sky (Video)]

 

The dazzling Leonid meteors are well-known for leaving particularly long-enduring incandescent sky trails, sometimes lingering for many seconds or even minutes. With binoculars you can see these trains drifting against the backdrop of stars, indicative of swift winds in the very high atmosphere. 

 

Over the central and western United States and Canada, the Leonids peak occurred earlier in the night (on Monday evening), but viewing circumstances were less favorable.

 

Along the West Coast for instance, the peak was from 9:30 p.m. to midnight PST late Monday night.  At best, perhaps a bright Earth-grazing meteor or two could be glimpsed. Earth-grazing meteors are space rocks that enter the Earth's atmosphere at a low angle, from the point of view of a given stargazer, and appear to scoot slowly and dramatically along the horizon.

 

Or will Leonids Part 2 fizzle?

Maslov predicted that the meteor brightness will be “somewhat lower than average.” Robert Lunsford of the American Meteor Society said:  “It does not sound like anything exciting and that is why I did not mention it in my weekly outlook. But I hope … that the meteors may be bright … time will tell.”

 

Bill Cooke of NASA’s Meteoroid Environmental Office at the Marshall Space Flight Center in Alabama was also somewhat cautious.

 

"In this case it is probably more where or when the particles were ejected than how fast. The small stuff from 1400 may be perturbed just right to intersect the Earth, though in past showers older Leonid trails have tended to have larger particles, such as in 1998," Cooke said. "My advice would be to look Tuesday morning — I will be."

 

Editor's note: If you snap an amazing photo of the Leonid meteor shower and would like to share it with SPACE.com for a possible story or image gallery, send images, comments and location information to managing editor Tariq Malik at tmalik@space.com.

 

Joe Rao serves as an instructor and guest lecturer at New York's Hayden Planetarium. He writes about astronomy for The New York Times and other publications.

 

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This story was originally written for SPACE.com and was republished with permission here. Copyright 2012 SPACE.com, a TechMediaNetwork company.