The 2009 Leonid Meteor Shower

This year's Leonid meteor shower peaks on Tuesday, Nov. 17th. If forecasters are correct, the shower should produce a mild but pretty sprinkling of meteors over North America followed by a more intense outburst over Asia. The phase of the Moon will be new, setting the stage for what could be one of the best Leonid showers in years.

"We're predicting 20 to 30 meteors per hour over the Americas, and as many as 200 to 300 per hour over Asia," says Bill Cooke of NASA's Meteoroid Environment Office. "Our forecast is in good accord with independent theoretical work by other astronomers."

Leonids are bits of debris from Comet Tempel-Tuttle. Every 33 years the comet visits the inner solar system and leaves a stream of dusty debris in its wake. Many of these streams have drifted across the November portion of Earth's orbit. Whenever we hit one, meteors come flying out of the constellation Leo.

"We can predict when Earth will cross a debris stream with pretty good accuracy," says Cooke. "The intensity of the display is less certain, though, because we don't know how much debris is in each stream." Caveat observer!
The first stream crossing on Nov. 17th comes around 0900 UT (4 a.m. EST, 1 a.m. PST). The debris is a diffuse mix of particles from several old streams that should produce a gentle display of two to three dozen meteors per hour over North America. Dark skies are recommended for full effect.

"A remarkable feature of this year's shower is that Leonids will appear to be shooting almost directly out of the planet Mars," notes Cooke.

It's just a coincidence. This year, Mars happens to be passing by the Leonid radiant at the time of the shower. The Red Planet is almost twice as bright as a first magnitude star, so it makes an eye-catching companion for the Leonids: sky map.

The next stream crossing straddles the hour 2100-2200 UT, shortly before dawn in Indonesia and China. At that time, Earth will pass through a pair of streams laid down by Comet Tempel-Tuttle in 1466 and 1533 AD. The double crossing could yield as many as 300 Leonids per hour.

This side of Earth will be facing the Leonid debris stream at the time of the Nov. 17th outburst. Observers in India, China and Indonesia are favored with dark, pre-dawn skies.

"Even if rates are only half that number, it would still be one of the best showers of the year," says Cooke.

The Leonids are famous for storming, most recently in 1999-2002 when deep crossings of Tempel-Tuttle's debris streams produced outbursts of more than 1000 meteors per hour. The Leonids of 2009 won't be like that, but it only takes one bright Leonid streaking past Mars to make the night worthwhile.

Enjoy the show.

Dragon X Launch Schedule

2009 Launches

Date: 23 November 2009, Monday
Mission: Diamond Ring flight test
Launch Vehicle: Diamond Ring PTR-01
Launch Site: Dragon X Space Agency
Launch Complex - EFTP 0019
Launch Window: 10.45am – 11.00am (TBD)
Description: Dragon X Space Agency will launch the Diamond Ring rocket on its first flight test for the FOB operating.

2010 Launches

Date: 2010
Mission: Diamond Ring 2nd flight test
Launch Vehicle: Diamond Ring PTR-02
Launch Site: Dragon X Space Agency Launch Complex – EFTP 0019
Launch Window: (TBD)
Description: 2nd flight test for Diamond Ring

Date: 2010
Mission: Launch EX exploration
Launch Vehicle: EX exploration rocket
Launch Site: Dragon X IMSS Launch – Holder-Hand
Launch Window: (TBD)
Description: Launch an explosion missile for Weapon Manufacture Industry-WMI

Date: 2010
Mission: Diamond Ring Final Confirmation Flight
Launch Vehicle: Diamond Ring PTR-03
Launch Site: Dragon X Space Agency Launch Complex – RLP 1A
Launch Window: (TBD)
Description: Launch Diamond Ring for the final flight in the “Diamond Ring Flight Test Programmed”

DIAMOND RING FLIGHT TEST

23 November 2009

Time(s): 10.45 a.m. – 11.00 a.m. (TBD)

Location: Dragon X Space Agency Launch Complex – EFTP 0019 launch pad

Dragon X Space Agency will launch the Diamond Ring rocket on a first flight test for transport payload to ORP and GTP. The “Diamond Ring Flight Test Programmed” that was launched by the Space Exploration Cooperation – Space X, is to collect the data from Diamond Ring PTR -01 during the flight onto the FOB operating.


The Dragon X Space Agency Launch Complex Viewing Dots will be closed during this launch.

A Mars Rover Named "Curiosity"

If you found your grandmother's diary, tattered and dust covered, up in the attic, would you read it? Of course you would. Granny was a pistol! Brush off the dust, open up the little book, and foray into her lively and interesting past.
Dust cloaks some fascinating tales in other places, too. NASA scientists will soon brush the dust off some Martian rocks that are practically bursting their seams to give their lively account of the red planet's past. The Mars Science Lab -- aptly named "Curiosity" -- is heading up there in 2011 to read the diary of Mars.

The small, car-sized rover will ramble about on the rocky surface, gizmos at full tilt, not only brushing dust off rocks but also vaporizing them with a laser beam, gathering samples to analyze on the spot, taking high resolution photographs, and more.

"Curiosity will be prospecting for organic molecules, the chemical building blocks of life," says Joy Crisp of NASA's Jet Propulsion Laboratory. "We want to find out whether Mars' environment was, or still is, capable of harboring life."
"To answer the question 'Is there life on Mars?' the most reasonable and productive approach is to look for organic compounds, which could be from life past or present, or from meteorites," explains Michael Meyer of NASA headquarters. "If you find anything, you know you're in a region that could preserve evidence of life, if there was any. We have maps from our orbiters, but we don't know which of the promising looking regions actually contains anything, much less the mother lode."

"The rock record is of particular interest," says Crisp. "It has a record from billions of years ago and can answer questions like 'Where and for how long might Mars have been habitable?' 'Was it cold or warm there in the past?' 'Was the water there acidic or salty?'"

Curiosity will be the first red planet rover since Spirit and Opportunity. Though it would be hard to match the twins' toughness, Curiosity will have a much greater range, more instruments, and a bigger, stronger robotic arm. It will be nuclear powered instead of solar, so there will be no worries about dust on solar panels causing energy supplies to plummet. It will have much more power, more consistently.

"Curiosity will even land in a new fashion," says Crisp. "Spirit and Opportunity were sitting on top of a lander that hit on the surface and bounced, protected by airbags, before coming to rest and opening up. They then had to drive off the top of the lander. A descent stage called Sky Crane will gently lower Curiosity (no airbags needed) via cables, which will be cut once the rover's wheels set down.

Meyer adds, "The most important difference is that Spirit and Opportunity aren't analytical labs – they are more for observing. This newest rover will be performing a more comprehensive study of the Martian environment."
Remote sensing instruments located on Curiosity's mast will scout around for promising targets and perform some long-distance analysis before the vehicle moves in for a closer look.

"Curiosity will have a laser on its mast that can take aim at a rock and vaporize a small spot on it," says Crisp. "This produces a plasma cloud that tells us about that rock's chemistry. We'll look at the light reflected off the cloud to characterize rocks and soils from up to 9 meters away. We’ll be able to classify minerals, ices, and organic molecules without having to drive as much."

The mast also sports a high-resolution camera called, naturally, Mastcam. It will observe, photograph, and videotape geological structures and features, like craters, gullies, and dunes.

"Siblings." This artist's concept compares Curiosity (left) to Spirit (right).

The rover's robotic arm wields its own unique instruments. APXS, the Alpha Particle X-Ray Spectrometer, will measure the abundance of chemical elements in the dust, soils, rocks, and processed samples. MAHLI, the Mars Hand Lens Imager, will return color images like those of typical digital cameras and act like a geologist's magnifying lens. Its images can be used to examine the structure and texture of rocks, dust, and frost at the micrometer to centimeter scale.

One laboratory instrument inside the rover's body will explore the red planet by "sniffing" the air, bird-dog style. SAM, short for Sample Analysis at Mars, has vents that open to the atmosphere to determine where to take samples, for example if it detects methane in the area.

"That's important because methane can be released by microbes," explains Crisp, "or by liquid water reacting with rock at depths under the surface. Water 'down under' could be a niche for subterranean life. SAM can also be used to sniff the gases released after baking a rock or soil sample in its oven."

In addition, Curiosity will carry instruments for observing Martian weather and measuring cosmic radiation bombarding the planet's surface.

"This rover is intrinsically spectacular in terms of what the mission will do," says Meyer. "It's a keystone for the future. It sets the stage for understanding whether organics are preserved on Mars and will tell us what we need to use to find out.

"Now – where's that diary?