Archive for the ‘asteroids’ Category

The 2010 Geminids!

Monday, December 13th, 2010

Credit: Wally Pacholka TWAN


WHAT: Geminid Meteor Shower

WHEN: December 13 / 14

WHERE: The Night Sky!

OBSERVING and SHARING:

While Gemini currently rises from the east horizon around 9pm, tonight’s first-quarter moon sets around 1am local time, when Gemini is higher overhead, so best observations will likely be in the hours between 2am and dawn, local time.

Don’t overlook tonight’s first-quarter Moon with Jupiter, earlier in the evening, and all those celestial goodies surrounding Gemini, throughout the night!

If your skies are too cloudy to see the Geminids, you can listen to their radar echoes on Spaceweather Radio!

NASA is hosting an all-night Geminids webchat, from 11pm – 5am EST, where you can have your questions answered by  NASA astronomer Bill Cooke!

Twitter-users are including the #Geminid hashtag to share their observations from around the world.

Photograph tonight’s meteor shower with helpful hints from this article, by Dennis Bodzash.

Collect tonight’s meteor shower with this micrometeorites how-to from Brian Carusella.

Contribute to meteor science with the International Meteor Organization’s electronic visual report form, here, and the American Meteor Society’s fireball reporting form, here.

FUN FACTS:

Meteor showers occur when our planet encounters the debris fields of passing comets.  Much of the debris is dust-sized particles, but some streams can contain larger objects ranging from gravel to small rocks.  Individually, these particles are known as meteoroids.

Most debris fields are ancient, having been left tens and hundreds of years ago, by comets as they near the Sun.  As the material leaves a comet, it falls into orbit as a collective stream or elongated patch.  Some streams can extend for millions of miles.

As Earth moves through a comet’s debris field, those particles (meteoroids) passing through our atmosphere are vaporized, resulting in the bright streaks that we call meteors.

Meteoroids that survive their encounter with our atmosphere, and actually impact the Earth’s surface as a small rock, are known as meteorites.

Meteor showers are named for the constellation from which the meteors appear to emanate, rather than for their physical origins.  That apparent, or visual, origin point is known as the “radiant.”

Observed nearly every December since the late 1800s, the Geminids are named for the constellation Gemini, with their radiant appearing to be just north of Gemini’s two brightest stars, Castor and Pollux.

Although Geminid meteors are slower and exhibit less trails than most other meteors, Geminids put on a fantastic display as one of the more prolific and consistent meteor showers of the year.

Geminids activity has steadily increased through the decades, with plateau peak rates reaching as high as +/-120 in more recent years.  A 2005 analysis of sixty years of observation data suggests the Geminid stream to be about 6,000 years old.

A meteor shower’s physical origin is known as the “parent body” or “progenitor.”  Geminid meteors originate in Earth’s encounter with the debris field of the near-Earth-object, 3200 Phaethon.

The Geminids’ progenitor, 3200 Phaethon, became the first asteroid discovered by a spacecraft, when scientists spotted it in images from the multi-national Infrared Astronomical Satellite (IRAS.)  Those scientists were Simon F Green and John K Davies, and the year was 1983.

3200 Phaethon is categorized as an Apollo class near-Earth-object, as well as a potentially hazardous asteroid (PHA,) with its closest pass missing Earth’s orbit by a mere 2-million miles.

Although most meteor showers do originate from comets, 3200 Phaethon is not a typical comet, nor does it appear to be a usual asteroid.  While some scientists originally thought that Phaethon may be a “dormant” comet, a more recent study proposes an entirely new kind of object – a “rock comet” possibly even born of an impact event with the large main belt asteroid, Pallas.

A better understanding of Phaethon’s peculiar comet/asteroid characteristics and possible Pallas relationship might also help scientists make more learned determinations about other similar peculiar events, such as the recent comet-like coma detected around the asteroid (596) Sheila.

Near-Earth-Object 2010 RF12 in Aquarius

Wednesday, September 8th, 2010

Two small space rocks, discovered just three days ago, are passing between our planet and the Moon today. Last night, I managed to grab a picture of the closer one, 2010 RF12, as it passed through the constellation Aquarius.

In this image (click for larger version,) the NEO appears as a faint segmented line. That’s because it is a small object moving quickly through multiple exposures of a fixed field of view.  Several galaxies are also apparent, including NGC 7364 which hosted a supernova in 2006.

Location: Slooh Remote Observatory, 954, Mt. Teide, Tenerife, Canary Islands
Scope: 0.5 meter f6.8 Corrected Dall Kirkham
Coordinates: RA 22 44 48 DEC -00 06 06 (Aquarius)
Time: 2010 Sept 08, 0440 UTC
Magnitude: 15.58
NEO: 2010 RF12 / 5.8m – 13m Aten object
Close Approach: 0.2 LD (48,000 miles) 2010 Sept 08 at 21:12 UTC
Discovery: 2010 Sept 05, Andrea Boattini, Mt. Lemmon, Arizona, Catalina Sky Survey

Visualizing Our Busy Neighborhood

Sunday, August 29th, 2010

It’s one thing to read about the discovery history of asteroids; it is another to visualize it.  Astronomer Scott Manley has created a fantastic animation illustrating the known positions of all asteroids discovered in the past three decades.  Each new discovery appears as a white object and then evolves to either yellow or red for near-Earth-asteroids, or green for all others.

While the animation is not to scale – Space is not so crowded as it appears in the video – it does offer a great comprehension of how frequently we are discovering new objects, especially in the last decade, and of just how busy our inner solar system really is.  Hundreds of thousands of asteroids have already been discovered, more than seven-thousand of which pass near or across our own planet’s orbit.  Scientists estimate that there are probably millions of undiscovered asteroids residing in the Main Belt, with about 750,000 measuring greater than one kilometer, and hundreds of thousands of which are likely near-Earth asteroids.

The most interesting thing about Manley’s animation is the discovery pattern.  As noted in Manley’s You Tube description, most discoveries are made in the region directly opposite the Sun and many are obviously related to specific missions and surveys, such as the automated sky surveys, the more recent WISE mission, and even past searches for Jovian satellites.

Kudos to Scott Manley for this creative way of bringing the more intricate details of solar system discovery down to Earth!

*Click the full-screen option and turn up your sound.

1 Dusty Determination + 1 Serendipitous Solution = 2 Mysteries Solved!

Saturday, April 17th, 2010

An exhaustive study, led by the SETI Institute’s Peter Jenniskens and planetary scientist David Nesvorny of Colorado’s Southwest Research Institute, has solved two long-standing mysteries.   Interestingly, it was the study of one well-known phenomenon that serendipitously solved a second, lesser-known mystery.

The primary focus of the NASA-funded study was to determine the true origins of zodiacal light.  Originally attributed to the scattering of sunlight by solar system dust – an explanation recently refined to specify asteroid dust – the zodiacal light extends as a glowing cone up from the sunset or sunrise horizon to the ecliptic.  Although this ethereal light is so tenuous as to be rendered invisible by moonlight and light pollution, it is readily apparent in darker skies and even bright enough to be followed across the ecliptic in the very darkest conditions.

In their paper, Cometary Origin of the Zodiacal Cloud and Carbonaceous MicroMeteorites – Implications for Hot Debris Disks, Jenneskins and Nesvorny confirm the zodiacal cloud mass as originating primarily, not from asteroids, but from the past violent and repeated disruptions of Jupiter Family comets.  Moreover, these disruptions likely resulted in twenty-trillion-tons of dust, with hundreds-of-thousands of tons impacting our planet every day!

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Of Fusion Crusts and Strewn Fields: Science Channel’s “Meteorite Men” Make an Impact

Tuesday, March 2nd, 2010

PHOTO CREDIT: Photograph by Caroline Palmer © Aerolite Meteorites www.aerolite.org

Join us Sunday, March 7 at 9pm EST (March 8 at 0200 UTC), for a special AFM*Radio presentation featuring Geoffrey Notkin of the Science Channel’s Meteorite Men!

In a pre-recorded interview, we speak with Geoff about all things Meteorite Men, including how the show came to be, some surprising results of the show, and his remarkable fourteen-year friendship with Meteorite Men co-host, Steve Arnold.  Geoff also discusses some of world’s more fascinating impact sites, the intricacies of meteorite hunting,  and his own passions for science, meteorites, and music.

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Webcast Archive: “MoonWalking with Rob Self-Pierson”

Friday, December 18th, 2009

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12/23/2009 Update: Video archive of this webcast can be found here.

Throughout billions of years, the Moon has held an intrinsic practical and emotional bond with our planet.  Sadly, we are losing the human connection as we keep our eyes fixed on the material and social noise of today’s world.

Every once in a while, something special comes along to remind us to pause and look up at Luna, to consider that constant, though oft-forgot, guidepost for all living things on Earth.

We are proud to announce our next AFM*Radio special event, an audio/visual presentation, Moon-Walking with Rob Self-PiersonJoin us next Tuesday night, Dec. 23 0100 UTC (Dec. 22 8pm ET), when Rob Self-Pierson stops by to discuss his “MoonWalking” experiences and his upcoming Blue Moon Walk.  We’ll feature images, video, an interactive chatroom, and details about how you can participate in commemorating the last Blue Moon of this decade!