Archive for the ‘Comets’ Category

And THIS is a Sun-grazing comet!

Wednesday, May 11th, 2011

The solar neighborhood is busy this week, with a fantastic solar eruption on Monday and now a sun-grazing “Kreutz” comet on Tuesday! These images were compiled from the SOHO/LASCO C2 database:

SOHO’s LASCO instrument is a set of two coronagraphs that image the solar corona from about 462-thousand to about 13.4-million miles. A coronagraph is a telescope that blocks light from the solar disk, and the corona is the plasma atmosphere surrounding the Sun. C2 has a 3-degree field of view and C3 has a 16-degree field of view. The Sun, by comparison, is 0.5-degrees across – you can see it as the white outlined circle in the center of the LASCO images.

Click here to see SOHO launching from Cape Canaveral in December 1995. Click here to see the latest SOHO images. Click here to learn more about Kreutz and other sungrazing comets.

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.

Another one bites the (star)dust

Thursday, October 21st, 2010

SOHO has captured another Kreutz Sungrazer comet plunging towards the Sun this week.  Kreutz Sungrazers, named for astronomer Heinrich Kreutz and the comets’ “sun-grazing” orbits, are believed to be the fragments of a super-comet that broke apart some 2,000 years ago.

While most of these fragments can be measured in meters, there are the rare “Great Comets”  that are visible even in the daytime sky.  This particular comet was not one of those larger fragments, nor did it actually dive “into” the Sun as it appears to in the movie; rather, it is passing within such close proximity as to be completely disintegrated.

Many of the Kreutz Sungrazers are discovered by amateur astronomers.  This particular fragment was discovered by Chinese comet-hunter Bo Zhou.  Click here to learn how you can use SOHO images to discover your own sungrazing comets!

(*Credit Note: Fragmentation hierarchy of bright sungrazing comets and the birth and orbital evolution of the Kreutz system. I. Two-superfragment model: http://hdl.handle.net/2014/39288)

Now Available On-Demand

Thursday, August 12th, 2010

Our special Perseids #Meteorwatch presentation, When Planets and Particles Collide – Part II, is now available for on-demand play.  Click here to watch and listen.  NOTE: The slides may take a moment to load.

Planets, Particles, and the Perseids!

Wednesday, August 11th, 2010

WHAT: When Planets and Particles Collide – Part II

WHEN: Thursday, August 12, 9:00 pm EDT

WHERE: AFM*Radio

Join us Thursday night on AFM*Radio for a fun slideshow presentation featuring the Perseid Meteor Shower!  Adapting last year’s When Planets and Particles Collide, we’ll  focus on the Perseids as we talk about the differences between meteoroids, meteors, and meteorites; the mechanisms of meteor showers; and the night sky surrounding constellation Perseus.  Science and Fun, all rolled into one!

NOTE: This special feature will be presented in Adobe Connect.  Log-in here as a “guest”. You can then listen to the audio through the Adobe room, or mute the Adobe sound and listen via AFM*Radio.

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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