Nola Taylor Redd, Author at żěè¶ĚĘÓƵ Science news and science articles from żěè¶ĚĘÓƵ Fri, 12 Aug 2016 11:09:45 +0000 en-US hourly 1 https://wordpress.org/?v=7.0.1 242057827 Canadian meteorite may be first visitor from the Kuiper belt /article/2100887-canadian-meteorite-may-be-first-visitor-from-the-kuiper-belt/?utm_campaign=RSS|NSNS&utm_content=currents&utm_medium=RSS&utm_source=NSNS /article/2100887-canadian-meteorite-may-be-first-visitor-from-the-kuiper-belt/#respond Fri, 12 Aug 2016 09:57:01 +0000 /?post_type=article&p=2100887 cxvxvxvxcv
Rock of ages: pristine sample from beyond Neptune
Michael Holly; Creative Services; University of Alberta.

A fireball that streaked through the sky over a decade ago may have brought the first meteorite from the outskirts of the solar system.

Most meteorites found on Earth are thought to start out in the asteroid belt, which lies between Mars and Jupiter, but the makeup of the Tagish Lake meteorite, which fell on an icy lake in Canada’s British Columbia in 2000, bears little resemblance to other space rocks.

That might be because it formed much further out in the Kuiper belt, the ring of icy bodies beyond Neptune that has Pluto as its most famous member. NASA recently approved an extension of the New Horizons mission to visit a Kuiper-belt object called 2014 MU69, so having a sample of similar material on Earth could help us understand how this region of the solar system formed.

of the Southwest Research Institute in Boulder, Colorado, and his colleagues suggest that in the early solar system the shifting of the giant planets – Jupiter, Saturn, Uranus and Neptune – may have hurled debris from the outskirts into the asteroid belt. And some rocks, including the Tagish Lake meteorite, might then have travelled onwards to Earth.

Giant  planets

“For a short time in the solar system’s history, you have giant planets encountering one another while surrounded by this big sea of comets,” Bottke says. The team studied how this dance of giants may have hurled smaller objects inward, including asteroids born from comets. “Things were very dramatic for a short time.”

One theory of the early solar system suggests there was once a fifth giant planet, later ejected from our cosmic neighbourhood. The team suggest that the gravitational pull of this fifth giant could have helped seed the asteroid belt with primitive objects from the Kuiper belt.

That seeding could explain the origins of the Tagish Lake meteorite, which previous studies suggested might be a small class of objects known as D-type asteroids. Only a handful of the unusual class of rock lurks in the asteroid belt, though the dark samples are abundant around gas giants.

Samples from the Kuiper belt could provide clues to how planets formed, something that could help solve the mystery of where Earth’s water came from, Bottke says. Most researchers think it was deposited on the planet from elsewhere in the solar system, but they’re still not sure what brought it.

“[Their research is] pretty convincing and it makes a lot of sense that those objects are implanted from this distant region which was the initial Kuiper belt,” says at the Marseille Observatory in France. He isn’t quite convinced that surface observations of D-type asteroids match them with Tagish Lake meteorite, though he tentatively suggests the object could have come from the heart of one of the rare rocks. “For now, we don’t have the observations to establish that it is possible.”

Bottke remains confident, pointing out that the five-planet model still works if the meteorite comes from either the surface or the heart of the unusual asteroids. Either way, the object that crashed on to Tagish Lake may provide the first direct sample from the outermost edges of the solar system to help us understand its early history.

The Astronomical Journal

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Hot Jupiters may have formed through planetary billiards /article/2064415-hot-jupiters-may-have-formed-through-planetary-billiards/?utm_campaign=RSS|NSNS&utm_content=currents&utm_medium=RSS&utm_source=NSNS Fri, 06 Nov 2015 17:00:00 +0000 http://dn28459 Planetary ping-pong might have built the strange worlds known as hot Jupiters. Fresh research suggests that collisions between young planets could have formed the cores of these massive gas giants, challenging the long-held idea that they migrated in from the outer edges of their systems. Most of the first exoplanets identified were hot Jupiters, gas giants that orbit their stars in days or even hours. “The presence of hot Jupiters has been a major surprise with planet-hunting, and their existence has immediately challenged planet-formation theory,” says of the University of British Columbia in Vancouver, Canada. Early theories suggested that these worlds must have formed at least as far from their stars as Earth is from our sun, before moving inward. But the influx of planets discovered with NASA’s Kepler telescope challenged that idea. Kepler has spotted large, rocky planets called super-Earths and mini-Neptunes orbiting near their stars. Such planets should have gathered gas and dust as they travelled inward, ultimately becoming gas giants. The fact that they remained rocky suggested they could have formed closer to their stars.

Tightly packed

In addition, the telescope has turned up systems where several rocky planets are packed closely with their star, which researchers call systems of tightly packed inner planets (STIPs). Most of these systems will eventually become unstable and send their planets crashing into one another. If those collisions happened slowly enough, the planets could stick together and form the core of a new planet. And if they happened before the material around the star dissipated, which takes about 10 million years, that core could grab on to enough gas and dust to become a hot Jupiter. To test this idea, Boley and his colleagues added instabilities to a computer model of Kepler-11, a system that contains six rocky planets orbiting closer to their star than Mercury does to the sun. Their simulations produced several warm Jupiters – gas giants just a bit further from their stars than hot Jupiters. The team attributed this difference to the particular arrangement of Kepler-11’s planets, and say different configurations should result in the overheated gas giants. This doesn’t mean that planets never migrate in towards their stars, Boley adds – but it might not be the dominant method of building warm and hot Jupiters. “It fits in really nicely with the idea of STIPs becoming unstable,” says of the University of Arizona in Tucson. “This is a totally different way of thinking about [hot Jupiter] formation.” Reference: (Image credit: NASA, ESA & G. Bacon)]]>
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Explosive meteors may have seasonal peaks /article/2074601-explosive-meteors-may-have-seasonal-peaks/?utm_campaign=RSS|NSNS&utm_content=currents&utm_medium=RSS&utm_source=NSNS Fri, 10 Oct 2014 14:02:00 +0000 http://dn26361 Out of a clear blue sky, a meteor explodes over Chelyabinsk, Russia, last year
Out of a clear blue sky, a meteor explodes over Chelyabinsk, Russia, last year
(Image: Ria Novosti/SPL)

Heads up – it’s explosive-meteorite season. A new analysis suggests that powerful incoming meteors like the rock responsible for last year’s explosion over Chelyabinsk, Russia, may not be completely random.

Brothers at Complutense University of Madrid in Spain used data from the infrasound sensors of the – which were designed to detect nuclear detonations on Earth – to measure 26 explosions from with energy of up to 1 kilotonne of TNT between 2000 and 2014. Seven other events were taken from published literature.

They found that several explosions occurred within a handful of days as similar explosions in previous years. For instance, the Chelyabinsk impact was on 15 February, 2013, while a meteorite over the South China Sea was recorded on 18 February, 2000, at almost the same latitude. The number of meteors in the study is admittedly very small, but a statistical analysis suggests that rather than being random events, there may be a seasonal aspect to explosive meteorites.

A seasonal peak was discernible in the southern hemisphere, where explosions clustered between September and December. In the northern hemisphere, blasts seemed evenly distributed throughout the year, although some individual events appeared to be linked.

Seasonal showers

We already know about seasonal meteor showers caused by debris from comets entering Earth’s atmosphere when the comets cross our planet’s path. But while comets shed centimetre-scale particles to create ordinary meteor showers, explosive impacts may be caused by streams of metre-scale objects. These might be the remnants of large asteroids ripped apart by gravitational encounters with other bodies, like Jupiter, or objects kicked out of the asteroid belt and trapped in orbits that regularly carry them into the vicinity of Earth’s path.

Unfortunately, it is hard to compare the material of meteorites from two potentially linked explosions, as in many cases, no samples are recovered. But the authors hope their work will inspire further examination of existing meteorites.

“Although based on a small sample – lucky for us, these relatively big things are not falling often – our work is intended to spawn multidisciplinary research that may eventually help us all to better deal with this problem,” says Carlos de la Fuente Marcos.

at the Space Science Institute in Boulder, Colorado, is not inspired by the new research. He points out that astronomers would not change their strategy and stop searching the skies during a supposedly low-probability month – and for small, local explosions, advanced knowledge of a significant meteor could actually make the situation worse.

“Evacuations are not harmless,” he says, adding that they typically result in a death rate of about 1 in 100,000 people. While no deaths were attributed to the 2013 explosion over Russia when it came without warning, “emptying out Chelyabinsk might kill 10 or so people. We run a serious risk of overreacting.”

Journal reference:

Article amended on 1 January 1970

When first published, this story mistakenly suggested a seasonality of explosive events in the northern hemisphere.

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