Why Saturn’s rings are so sharp

January 5th, 2009

outer-b-ring

Here’s a conundrum for you: why do Saturn’s rings have such sharp edges?

It’s question that has puzzled planetary scientists for many years. Various ideas have been put forward but none adequately explain the structure we see today.

To understand just  how sharp the edges are consider this: pictures from Cassini show that the density of particles at the edge of the outer B ring, for example, drops by an order of magnitude over a distance of only 10 metres or so.

That’s extraordinary given that the ring is 25580 kilometres wide.

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Flash ‘n’ cash

January 3rd, 2009

The best of the rest from the physics arXiv:

The Hydrodynamics of Swimming Microorganisms

Trapping Ccold Atoms Using Surface-Grown Carbon Nanotubes

Solution of Peter Winkler’s Pizza Problem

Innovative In Silico Approaches to Address Avian Flu Using Grid Technology

Quantum Generalized Reed-Solomon Codes: Unified Framework for Quantum MDS Codes

First stars “powered by dark matter”

January 2nd, 2009

dark-stars

“95% of the mass in galaxies and clusters of galaxies is in the form of an unknown type of dark matter,” say Katherine Freese at the University of Michigan, Ann Arbor, and buddies. What effect might this huge amount of stuff have on star formation?

The answer according to these guys is astounding. In the early universe, the first stars would have been powered by dark matter.

Here’s the thinking: the concentration of dark matter at that time would have been extremely high meaning that any ordinary stars would naturally contain large amounts of dark matter. Freese and co have calculated the effect of this stuff and say tit would have radically altered the evolution of these stars forming so-called “dark stars”.

Dark stars would have been driven by the annihilation of dark matter particles releasing heat but only in stars larger than 400 solar masses. That turns out to be quite feasible since stars containing smaller amounts of dark matter would naturally grow as they swept up dark matter from nearby space.

When the dark matter runs out, they simply collapse to form black holes

Interestingly, we should soon be able to to see these stars with forthcoming generations of telescopes. And if they are found, that would be further proof of the existence of dark matter.

Keep ‘em peeled!

Ref: arxiv.org/abs/0812.4844: Dark Stars: the First Stars in the Universe May be Powered by Dark Matter Heating

Flashback: First test of exotic space thruster ends in explosion

January 1st, 2009

Over the holiday period the arXivblog is re-running the most popular posts from 2008

23 May 2008: First test of exotic space thruster ends in explosion

In 2006, Mason Peck at Cornell University in Ithaca dreamt up with an entirely new way to control satellites orbiting planets that have a magnetic field. The idea is based on the Lorentz force: that a charged particle moving through a magnetic field experiences a force perpendicular to both its velocity and the field.

Read on…

Flashback: Forget black holes, could the LHC trigger a “Bose supernova”?

December 31st, 2008

Over the holiday period, the arXivblog is running a selection of the most popular posts from 2008

29 September 2008 : Forget black holes, could the LHC trigger a “Bose supernova”?

The fellas at CERN have gone to great lengths to reassure us all that they won’t destroy the planet (who says physicists are cold hearted?).

Read on…

Flashback: Cloaking objects at a distance

December 30th, 2008

Over the holiday period, the arXivblog is running a selection of the most popular posts from 2008

5 November 2008: Cloaking objects at a distance

One of the disadvantages of invisibility cloaks is that anything placed inside one is automatically blinded, since no light can get in.

Now Yun Lai and colleagues from The Hong Kong University of Science and Technology have come up with a way round this using the remarkable idea of cloaking at a distance. This involves using a “complementary material” to hide an object outside it.

Read on…

Flashback: Quantum communication: when 0 + 0 is not equal to 0

December 29th, 2008

Over the holiday period, the arXivblog is running a selection of the most popular posts from 2008

5 August 2008: Quantum communication: when 0 + 0 is not equal to 0

One of the lesser known cornerstones of modern physics is Claude Shannon’s mathematical theory of communication which he published in 1948 while juggling and unicycling his way around Bell Labs.

Shannon’s theory concerns how a message created at one point in space can be reproduced at another point in space. He calls the conduit for such a process a channel and the limits imposed by the universe on this process the channel capacity.

Read on…

Flashback: Do nuclear decay rates depend on our distance from the sun?

December 28th, 2008

Over the holiday period, the arXivblog is running a selection of the most popular posts from 2008

29 August 2008: Do nuclear decay rates depend on our distance from the sun?

Here’s an interesting conundrum involving nuclear decay rates.

We think that the decay rates of elements are constant regardless of the ambient conditions (except in a few special cases where beta decay can be influenced by powerful electric fields).

So that makes it hard to explain the curious periodic variations in the decay rates of silicon-32 and radium-226 observed by groups at the Brookhaven National Labs in the US and at the Physikalisch-Technische Bundesandstalt in Germany in the 1980s.

Read on…

Flashback: Feline ballistics

December 27th, 2008

Over the holiday period, the arXivblog is running a selection of the most popular posts from 2008

1 February 2008: Feline ballistics

Here’s a straightforward question in ballistics:

What velocity do you need to launch a 350 pound object over a 12.5 foot barrier that is 33 feet away?

Read on…

Flashback: First superheavy element found in nature

December 26th, 2008

Over the holiday period, the arXivblog is running a selection of the most popular posts from 2008

28 April 2008: First superheavy element found in nature

The hunt for superheavy elements has focused banging various heavy nuclei together and hoping they’ll stick. In this way, physicists have extended the periodic table by manufacturing elements 111, 112, 114, 116 and 118, albeit for vanishingly small instants. Although none of these elements is particularly long lived, they don’t have progressively shorter lives and this is taken as evidence that islands of nuclear stability exist out there and that someday we’ll find stable superheavy elements.

Read on…