Posts Tagged ‘Events’

Asteroid 2005 YU55 to Approach Earth on November 8, 2011

Saturday, November 5th, 2011

Source – NASA Near Earth Object Program (NEO):

Don Yeomans, Lance Benner and Jon Giorgini
March 10, 2011

Path of Astroid 2005 YU55

Trajectory of Asteroid 2005 YU55 - November 8-9, 2011
Click on image for animation

Near-Earth asteroid 2005 YU55 will pass within 0.85 lunar distances from the Earth on November 8, 2011. The upcoming close approach by this relatively large 400 meter-sized, C-type asteroid presents an excellent opportunity for synergistic ground-based observations including optical, near infrared and radar data. The attached animated illustration shows the Earth and moon flyby geometry for November 8th and 9th when the object will reach a visual brightness of 11th magnitude and should be easily visible to observers in the northern and southern hemispheres. The closest approach to Earth and the Moon will be respectively 0.00217 AU and 0.00160 AU on 2011 November 8 at 23:28 and November 9 at 07:13 UT.

Discovered December 28, 2005 by Robert McMillan of the Spacewatch Program near Tucson Arizona, the object has been previously observed by Mike Nolan, Ellen Howell and colleagues with the Arecibo radar on April 19-21, 2010 and shown to be a very dark, nearly spherical object 400 meters in diameter. Because of its approximate 20-hour rotation period, ideal radar observations should include tracks that are 8 hours or longer on multiple dates at Goldstone (November 3-11) and when the object enters Arecibo’s observing window on November 8th.

Using the Goldstone radar operating in a relatively new “chirp” mode, the November 2011 radar opportunity could result in a shape model reconstruction with a resolution of as fine as 4 meters. Several days of high resolution imaging (about 7.5 meters) are also planned at Arecibo. As well as aiding the interpretation of the radar observations, collaborative visual and near infrared observations could define the object’s rotation characteristics and provide constraints upon the nature of the object’s surface roughness and mineral composition.

Since the asteroid will approach the Earth from the sunward direction, it will be a daylight object until the time of closest approach. The best time for new ground-based optical and infrared observations will be late in the day on November 8, after 21:00 hours UT from the eastern Atlantic and western Africa zone. A few hours after its close Earth approach, it will become generally accessible for optical and near-IR observations but will provide a challenging target because of its rapid motion across the sky.

Side View

Trajectory of Asteroid 2005 YU55 - November 9, 2011

Although classified as a potentially hazardous object, 2005 YU55 poses no threat of an Earth collision over at least the next 100 years. However, this will be the closest approach to date by an object this large that we know about in advance and an event of this type will not happen again until 2028 when asteroid (153814) 2001 WN5 will pass to within 0.6 lunar distances.

WSF Live Forum: Fabric of the Cosmos

Friday, October 28th, 2011

Source -World Science Festival.

Join a live conversation with Brian Greene, exploring how scientists are piecing together the most complete picture yet of space, time, and the Universe.

Held at at Columbia University’s Miller Theatre, the event begins at 9 PM with the premiere broadcast of the first episode of NOVA’s The Fabric of the Cosmos, followed immediately by a live Q&A hosted by Greene, with special guests including renowned theoretical physicist Leonard Susskind and Saul Perlmutter, winner of the 2011 Nobel Prize in Physics.

The Q&A will also be streamed live as an interactive webcast at 10PM ET/9PM CT at www.worldsciencefestival.com:

•Get the conversation going now and ask your questions via Twitter (using hashtag #WSFforum), or submit questions on the World Science Festival Facebook wall

•Tune in to the live webcast at worldsciencefestival.com on Nov. 2 at 10pm ET and submit your questions live during the webcast »

Falling German satellite ROSAT X-ray astronomy observatory

Friday, October 21st, 2011

Source -Spaceflight Now.

Less than a month after NASA’s falling UARS satellite grabbed the headlines, the German space agency says one of its abandoned satellites will dive back to Earth later this month, but no one knows where it will land.

The ROSAT X-ray astronomy observatory is smaller and less massive than NASA’s Upper Atmospheric Research Satellite, or UARS, which fell back to Earth on Sept. 24. But officials predict it will spread three times more debris and pose a greater threat to people than UARS.

That’s because ROSAT is made of heat-resistant components, especially its primary mirror, which officials say will probably be the largest single fragment that will reach Earth.

The satellite will streak into the atmosphere at 17,000 mph, and temperatures up to 3,000 degrees Fahrenheit will burn up much of the spacecraft.

“All these forces exerted on the satellite cause it to disintegrate, which in turn means that it eventually lands in the form of a long debris trail,” said Heiner Klinkrad, head of the European Space Agency’s space debris office. “The lightweight objects fall to Earth first, similar to leaves from a tree. The really heavy objects land later, because they ultimately have to drill their way through the atmosphere.”

But engineers expect the bulk of ROSAT to survive re-entry, littering its impact point with up to 30 pieces of debris.

The 5,348-pound satellite launched from Florida on a Delta 2 rocket in 1990. ROSAT does not have an engine or propulsion system because it used reaction wheels to point its telescope toward scientific targets in the cosmos.

Up to 3,750 pounds of the satellite could reach Earth’s surface. NASA said they expected 1,200 pounds of UARS to survive re-entry.

There is a 1-in-2,000 chance someone will be struck by fragments of ROSAT on its way down, according to Germany. That equates to odds of about 1-in-14 trillion that any individual person will be hit.

The threat from UARS wasn’t as high. An analysis from NASA showed there was a 1-in-3,200 chance of a collision between a human and a piece of UARS.

The remnants of UARS fell in the remote Pacific Ocean, and ROSAT will likely also end up in the sea, but its impossible to tell where it will crash until hours before.

ROSAT launched in June 1990 on a Delta 2 rocket.

ROSAT, which stands for Roentgen Satellite, was turned off in 1999, and its altitude has gradually dropped since then from an operational orbit more than 350 miles high. The German Aerospace Center, also known as DLR by its German acronym, says the spacecraft should re-enter the atmosphere between Oct. 20 and Oct. 25.

But the margin of error in the re-entry forecast is three days, and officials likely won’t know where the satellite will come down until after it falls. Even one day before re-entry, the time of ROSAT’s demise will only be known with a precision of plus-or-minus five hours, putting entire oceans and continents in the satellite’s flight path.

“All areas under the orbit of ROSAT, which extends to 53 degrees northern and southern latitude could be affected by its re-entry,” said a posting on DLR’s website. “The bulk of the debris will impact near the ground track of the satellite.”

“It will not be possible to make any kind of reliable forecast about where the satellite will actually come down until about one or two hours before the fact,” Klinkrad said. “It will, however, be possible to predict, about one day in advance, which geographical regions will definitely not be affected.”

ROSAT’s orbit was at an average altitude of 149 miles Wednesday.

“This slow descent is due to the friction encountered by the satellite as it enters the outer fringes of Earth atmosphere, which increases the more ROSAT penetrates into our atmosphere,” Klinkrad said.

Klinkrad said the major factor affecting a satellite’s fall from orbit is solar activity. Energy unleashed from the sun causes Earth’s atmosphere to heat up and expand, generating more drag for satellites in low orbits.

Fluctuations in solar activity can quicken or slow a satellite’s re-entry. Experts initially expected ROSAT’s plunge to occur last year, but solar activity turned out to be less than predicted, delaying the re-entry until this month.

Weekend Meteor Shower Oct. 20, 2011:

Friday, October 21st, 2011

Source – NASA Science News:

A map of the morning sky on Saturday, Oct. 22nd at 5:30 a.m. local time, viewed facing southeast.
A map of the morning sky on Saturday, Oct. 22nd at 5:30 a.m. local time, viewed facing southeast.

Weekend Meteor Shower Oct. 20, 2011: Earth is about to pass through a stream of debris from Halley’s comet, source of the annual Orionid meteor shower. Forecasters expect more than 15 meteors per hour to fly across the sky on Saturday morning, Oct. 22nd, when the shower peaks.

Orionids are most easily seen during the dark hours before sunrise. Twilight Orionids, however, are the most beautiful of all. “Although this isn’t the biggest meteor shower of the year, it’s definitely worth waking up for,” says Bill Cooke of the NASA Meteoroid Environment Office. “The setting is dynamite.”

Orionids are framed by some of the brightest and most beautiful constellations in the night sky. The meteors emerge from mighty Orion, the shower’s glittering namesake. From there they streak through Taurus the Bull, the twins of Gemini, Leo the Lion, and Canis Major–home to Sirius, the most brilliant star of all.

This year, the Moon and Mars are part of the show. They’ll form two vertices of a celestial triangle in the eastern sky on Saturday morning while the shower is most active; Regulus is the third vertex. Blue Regulus and red Mars are both approximately of 1st magnitude, so they are easy to see alongside the 35% crescent Moon. Many Orionids will be diving through the triangle in the hours before dawn.

Cooke’s team at the Meteoroid Environment Office will be watching for Orionids that actually hit the Moon.

Cometary debris streams like Halley’s are so wide, the whole Earth-Moon system fits inside. So when there is a meteor shower on Earth, there’s usually one on the Moon, too. Unlike Earth, however, the Moon has no atmosphere to intercept meteoroids. Pieces of debris fall all the way to the surface and explode where they hit. Flashes of light caused by thermal heating of lunar rocks and moondust are so bright, they can sometimes be seen through backyard-class telescopes.

“Since we began our monitoring program in 2005, our group has detected more than 250 lunar meteors,” says Cooke. “Some explode with energies exceeding hundreds of pounds of TNT.”

So far, they’ve seen 15 Orionids hitting the Moon–”two in 2007, four in 2008, and nine in 2009,” recalls Cooke. This year they hope to add to the haul. About 25% of the Moon’s dark terrain will be exposed to Halley’s debris stream, giving the team millions of square miles to scan for explosions.

Watching meteoroids hit the Moon is a good way to learn about the structure of comet debris streams and the energy of the particles therein. It also allows Cooke and colleagues to calculate risk factors for astronauts who, someday, will walk on the lunar surface again.

“Going outside to watch the Orionids might not be a good idea for a moonwalker,” says Cooke.

But it is a good idea for the rest of us. Set your alarm for a few hours before dawn on Saturday morning and enjoy the show.

Author: Dr. Tony Phillips | Credit: Science@NASA

The comet and the coronal mass ejection

Saturday, October 8th, 2011

Source – Phil Blatt at BadAstronomy.com:

NASA \ JPL What’s Up for October 2011?

Wednesday, October 5th, 2011

Source – NASA /JPL Solar System Exploration:

Look for moons and meteors this month!

How to see the “supernova of a generation” with a pair of binoculars

Thursday, September 8th, 2011

Source – Berkeley Lab / lawrence Berkeley National Laboratory:

A supernova discovered yesterday is closer to Earth — approximately 21 million light-years away — than any other of its kind in a generation. Astronomers believe they caught the supernova within hours of its explosion, a rare feat made possible with a specialized survey telescope and state-of-the-art computational tools

At a mere 21 million light-years from Earth, a relatively small distance by astronomical standards, the supernova is still getting brighter, and might even be visible with good binoculars in ten days’ time, appearing brighter than any other supernova of its type in the last 30 years.

NASA: What’s Up For August 2011?

Friday, August 5th, 2011

Source – NASA /JPL Solar System Exploration:

What’s up for August? Planets with atmospheres! Venus has thick clouds, Mars has dust devils, and the outer planets have fierce winds. Why not have a look at Jupiter rising near midnight this month? The Juno Mission to Jupiter launches this month, too.

Vesta Sizes Up

Tuesday, July 19th, 2011

Source – NASA/JPL Dawn Journey to the Asteroid Belt :

This composite image shows the comparative sizes of nine asteroids. Up until now, Lutetia, with a diameter of 81 miles (130 kilometers), was the largest asteroid visited by a spacecraft, which occurred during a flyby.

Vesta, which is also considered a protoplanet because it’s a large body that almost became a planet, dwarfs all other small bodies in this image, with its diameter sizing up at approximately 330 miles (530 kilometers).

The Dawn mission is managed by NASA’s Jet Propulsion Laboratory in Pasadena, Calif., for the agency’s Science Mission Directorate in Washington. Dawn is a project of the directorate’s Discovery Program, managed by NASA’s Marshall Space Flight Center in Huntsville, Ala. UCLA is responsible for overall Dawn mission science. Orbital Sciences Corp. of Dulles, Va., designed and built the Dawn spacecraft. The framing cameras were developed and built under the leadership of the Max Planck Institute for Solar System Research in Katlenburg-Lindau, Germany. The German Aerospace Center (DLR) Institute of Planetary Research in Berlin made significant contributions in coordination with the Institute of Computer and Communication Network Engineering in Braunschweig. The framing camera project is funded by the Max Planck Society, DLR and NASA. JPL is a division of the California Institute of Technology in Pasadena.

More information about Dawn is online at http://www.nasa.gov/dawn and http://dawn.jpl.nasa.gov

NASA Spacecraft to Enter Asteroid’s Orbit on July 15

Thursday, July 14th, 2011

NASA's Dawn spacecraft obtained this image of the giant asteroid Vesta with its framing camera on July 9, 2011. Image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA

NASA/JPL Dawn Journey to the Asteroid Belt :

PASADENA, Calif. — On July 15, NASA’s Dawn spacecraft will begin a prolonged encounter with the asteroid Vesta, making the mission the first to enter orbit around a main-belt asteroid.

The main asteroid belt lies between the orbits of Mars and Jupiter. Dawn will study Vesta for one year, and observations will help scientists understand the earliest chapter of our solar system’s history.

As the spacecraft approaches Vesta, surface details are coming into focus, as seen in a recent image taken from a distance of about 26,000 miles (41,000 kilometers). The image is available at:
Source -

Engineers expect the spacecraft to be captured into orbit at approximately 10 p.m. PDT Friday, July 15 (1 a.m. EDT Saturday, July 16). They expect to hear from the spacecraft and confirm that it performed as planned during a scheduled communications pass that starts at approximately 11:30 p.m. PDT on Saturday, July 16 (2:30 a.m. EDT Sunday, July 17). When Vesta captures Dawn into its orbit, engineers estimate there will be approximately 9,900 miles (16,000 kilometers) between them. At that point, the spacecraft and asteroid will be approximately 117 million miles (188 million kilometers) from Earth.

“It has taken nearly four years to get to this point,” said Robert Mase, Dawn project manager at NASA’s Jet Propulsion Laboratory in Pasadena, Calif. “Our latest tests and check-outs show that Dawn is right on target and performing normally.”

Engineers have been subtly shaping Dawn’s trajectory for years to match Vesta’s orbit around the sun. Unlike other missions, where dramatic propulsive burns put spacecraft into orbit around a planet, Dawn will ease up next to Vesta. Then the asteroid’s gravity will capture the spacecraft into orbit. However, until Dawn nears Vesta and makes accurate measurements, the asteroid’s mass and gravity will only be estimates. So the Dawn team will need a few days to refine the exact moment of orbit capture.

Launched in September 2007, Dawn will depart for its second destination, the dwarf planet Ceres, in July 2012. The spacecraft will be the first to orbit two solar system destinations beyond Earth.

Dawn’s mission to Vesta and Ceres is managed by JPL for NASA’s Science Mission Directorate in Washington. Dawn is a project of the directorate’s Discovery Program, which is managed by NASA’s Marshall Space Flight Center in Huntsville, Ala. UCLA is responsible for overall Dawn mission science. Orbital Sciences Corp. of Dulles, Va., designed and built the spacecraft. The German Aerospace Center, the Max Planck Institute for Solar System Research, the Italian Space Agency and the Italian National Astrophysical Institute are part of the mission team.

For a current image of Vesta and more information about the Dawn mission, visit: http://www.nasa.gov/dawn and http://dawn.jpl.nasa.gov .You also can follow the mission on Twitter at: http://www.twitter.com/nasa_dawn .

Priscilla Vega/Jia-Rui Cook 626-298-3290/818-354-0850
Jet Propulsion Laboratory, Pasadena, Calif.
priscilla.r.vega@jpl.nasa.gov / jccook@jpl.nasa.gov

Dwayne C. Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov