dinsdag 2 augustus 2011

Non-zero sum transitions in the human past | Gene Expression

Non-zero sum transitions in the human past | Gene Expression: "

A few people have pointed me to the recent paper in Science, Tenfold Population Increase in Western Europe at the Neandertal–to–Modern Human Transition. The basic result is obvious, and not totally revolutionary: anatomically modern humans may simply have demographically absorbed the Neandertals (the word “absorbed” has many connotations here obviously). The results are clear in this figure:



This is not surprising, even though I have only a glancing familiarity with the guts of paleontology I was aware that there’s a lot of inferential evidence that Neandertals were not as efficient at extracting resources from any given piece of territory as modern humans. In The Dawn of Human Culture the paleoanthropologist Richard Klein offered a straightforward biological explanation for why and how the neo-African populations so rapidly marginalized Neandertals: some sort of macromutation which allowed for language and so the protean flexibility of human culture.




Implicitly this was the conventional wisdom until the likelihood of Neandertal admixture was discovered, and earlier the fact that Neandertals seemed to share the derived FOXP2 variant (the “language gene”). The earlier inferences of human demography using mtDNA, and later ancient ...

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Europe's Plan to Move An Asteroid

Europe's Plan to Move An Asteroid: "

If we ever need to prevent an asteroid hitting Earth, we'll have to deflect it somehow. To practice, the European Space Agency is planning a game of asteroid billiards



If astronomers ever spot an asteroid coming our way, the world will have to decide pretty quickly what to do.


One idea is to knock it off course. But although that sounds pretty straightforward, it hides a multitude of challenges. The most obvious of these is to determine how big an impact would be necessary and how this could be delivered.


In 2002, the European Space Agency began a program called Don Quijote to find out how best to perform such a deflection.


Don Quijote involves sending two spacecraft to a near Earth asteroid; one to smash into it and the other to watch while in orbit above the impact crater. The goal is to change the asteroid's semimajor axis by more than 100 metres and to measure the change with an accuracy greater than 1 per cent.


But the question is how best to monitor what's going on in a way that is relevant to other asteroids. After all, the ultimate plan is to use the information from this mission to move some other asteroid with our name on it.


Now, Stephen Wolters at the Open University in the UK and a few friends have published a new analysis of the mission saying that measuring the change in orbit is not enough. Instead, the spacecraft needs to characterise the impact in detail, determining the density of the material near the asteroid's surface, the size of the surface grains as well as the mass and speed distribution of the impact ejecta.


Only with this information will it be possible to work out exactly how the momentum from the impactor was transferred to the asteroid.


That significantly changes the mission. In addition to an on-board radio transmitter that will allow space scientists back on Earth to work out its distance exactly, the spacecraft will need a sophisticated imaging suite capable of photographing the damage and carrying out infrared spectroscopy to determine the asteroid's mineral content.


The thermal cameras will also pick up any changes in temperature. That's important because of the small but potentially significant force from the way the asteroid emits heat.


If the asteroid emits thermal photons equally in all directions, their force cancels out. But if it emits more in some directions than others, then this force will slowly push an asteroid. That can happen if the asteroid tends to cool down at a rate that matches its speed of rotation--so that all the thermal photons emitted after the surface has been in the Sun, travel in the same direction.


This force, called the Yarkovsky effect, could make the difference between whether an impact with Earth occurs or not. So knowing its value is crucial, particularly if the impactor changes the asteroid's rate of rotation.


So that should make Don Quijote a better mission but it also makes it a more expensive one. And that raises a question mark over whether the European Space Agency will want to pay for it on its own.


But then again, why should it? There's a good argument that the international community as a whole should shoulder the burden and the cost of planetary protection.


The only question then is how badly we need Don Quijote to keep our planet safe.


Ref: arxiv.org/abs/1107.4229: Measurement Requirements For A Near-Earth Asteroid Impact Mitigation Demonstration Mission





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Download DivX Converter 2.0.1 for Linux - A simple Mencoder GUI to Produce DivX Player Compatible video format with subtitle attach - Softpedia

Download DivX Converter 2.0.1 for Linux - A simple Mencoder GUI to Produce DivX Player Compatible video format with subtitle attach - Softpedia

This program works like a charm, was searching the whole weekend for something like this in ubuntu. Great work.

Twitter, Facebook & Google+ Propaganda PostersAaron Wood...

Twitter, Facebook & Google+ Propaganda Posters
Aaron Wood...
: "





Twitter, Facebook & Google+ Propaganda Posters


Aaron Wood criou uma série muito legal de poster com propagandas fictícias do Twitter, Facebook e Google.

"

maandag 1 augustus 2011

Vesta in breathtaking detail | Bad Astronomy

Vesta in breathtaking detail | Bad Astronomy: "

NASA’s Dawn mission team just revealed the first full-frame image of the giant main-belt asteroid Vesta, and it’s really, really cool:



Yegads! [Click to asteroidenate.]


Vesta is about 500 km (300 miles) across, but is clearly non-spherical, so take that as an average. That’s roughly the size of Colorado! So it’s a big rock, and we’re now seeing it in exquisite detail. This image was taken on July 24, from a distance of about 5000 km (3000 miles).


Man, there’s nothing like being there.


There’s a lot to see. The surface of Vesta is varied, with craters of various sizes (as expected) and depths. I’m very curious to see that there are some darker spots (like in this image) that look like material dredged up from under the surface from impacts; we see this on the Moon and other bodies as well. Some preliminary mineralogical maps show varied distributions of minerals on the surface as well.


An animation of Vesta rotating has also been put together, and really shows how odd this little world is:



[Make sure to set the resolution to at least 720p!]


Look at how the surface changes: you can see ...

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Wat gebeurt als de tijd stopt?

Wat gebeurt als de tijd stopt?: "

Wat zou er gebeuren als van het ene op het andere moment de tijd plotseling stil zou komen te staan? Tot nu toe was dat metafysische speculatie, maar natuurkundige Igor Smolyaninov is er in geslaagd het Einde van de Tijd na te bootsen. In een onverwacht alledaags materiaal. Wat gebeurt er als de tijd letterlijk opraakt?


Universum nabootsen in grafeen

Natuurkundigen vinden steeds meer fysische systemen die gebruikt kunnen worden als model van ruimtetijd. Zo kunnen ze spelen met de algemene relativiteitstheorie in een systeem dat wiskundig gezien erg lijkt op ruimtetijd. Een paar voorbeelden: elektronen in grafeen, het kippengaas van koolstofatomen dat de ontdekkers een Nobelprijs opleverde, gedragen zich bij afkoelen ongeveer zo als het universum vlak na de Big Bang waardoor natuurkundigen in staat zijn, door grafeen te koelen meer te weten te komen van het vroege heelal.


Elektromagnetische ruimte


Wat zou er gebeuren als de tijd ophoudt te bestaan?

Wat zou er gebeuren als de tijd ophoudt te bestaan?


Een ander voorbeeld is de wiskundige gelijkenis tussen licht in een elektromagnetische ruimte (doorzichtig medium) en in ruimtetijd. Fysici hebben kort geleden ontdekt hoe ze in deze elektromagnetische ruimte dingen kunnen aanleggen als kwantumschuim, de Big Bang, zwarte gaten en zelfs het hele multiversum. Moeilijk te overtreffen, maar Igor Smolyanov is er nu toch in geslaagd. Hij heeft in zijn nieuwste experiment het einde van de tijd gemodelleerd.


Experimenteren met het einde van de tijd

Smolyaninov’s techniek maakt gebruik van metamaterialen. Metamaterialen kunnen zo worden samengesteld dat ze zich gedragen als een tweedimensionale ruimte met een tijddimensie. Overigens kan andersom ook: twee tijddimensies en één ruimtedimensie, bijvoorbeeld. Metamaterialen zijn veelzijdig.

Volgens Smolyaninov ontstaat een interessante situatie als de twee materialen tegen elkaar worden gezet. Als de tijddimensie loodrecht op de ruimtedimensie staat, eindigt de tijd domweg plotseling, aldus Smolyaninov. Hij noemt deze situatie het Einde der Tijden.


In hun experiment lieten de experimentatoren ruimtetijd overgaan in een Euclidische ruimte (dus zonder tijd). Ze bouwden dit scenario na in metamaterialen met optische eigenschappen die lijken op de eigenschappen van ruimtetijd. Hiervoor gebruikten ze de plasticsoort polymethyl methacrylaat (PMMA), beter bekend als perspex of plexiglas. Dit materiaal werd in stroken op een goudlaagje aangebracht. Het licht beweegt zich in de vorm van plasmons (een soort energievibraties die langs een oppervlak reizen) langs dit oppervlak. Er werden twee kosmologische situaties nagebootst: het einde van de ruimte en het einde van de tijd.

Het einde van de ruimte leidt tot een Rindler-horizon, iets dat veel weg heeft van een waarnemingshorizon, en liet de door Hawking al voorspelde Hawkingstraling zien.


Maar wat gebeurt er aan het einde van de tijd?

Volgens Smolyaninov divergeert het elektromagnetische veld aan het einde van de tijd (m.a.w. waaiert uit). Volgens het Physics Blog van MIT Technology Review een vrij saaie ontwikkeling, maar wie weet is dat precies wat er nu gebeurt. Immers, er lijkt een geheimzinnige invloed, de donkere energie, het heelal steeds sneller uiteen te rukken. Zou het einde der tijden steeds sneller naderen? Kunnen we op tijd uit dit heelal ontsnappen? De zaak blijft interessant.


Bron

Igor I. Smolyaninov et al., Hyperbolic Metamaterial Interfaces: Hawking Radiation From Rindler Horizons And The “End Of Time”, 2011

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Problem Banks: Comparing Official and Unofficial Counts

Problem Banks: Comparing Official and Unofficial Counts: "The following graph compares the weekly count of banks on the 'unofficial problem bank list' with the number from the FDIC's Quarterly Banking Profile.



We started posting the Unofficial Problem Bank list in early August 2009 (credit: surferdude808).



The FDIC's official problem bank list is comprised of banks with a CAMELS rating of 4 or 5, and the list is not made public (just the number of banks and assets every quarter). Note: Bank CAMELS ratings are also not made public.



CAMELS is the FDIC rating system, and stands for Capital adequacy, Asset quality, Management, Earnings, Liquidity and Sensitivity to market risk. The scale is from 1 to 5, with 1 being the strongest.



As a substitute for the CAMELS ratings, surferdude808 is using publicly announced formal enforcement actions, and also media reports and company announcements that suggest to us an enforcement action is likely, to compile a list of possible problem banks in the public interest.



Problem Banks

The red dots are the number of banks on the official problem bank list as announced in the FDIC quarterly banking profile for Q1 2009 through Q1 2011. The dots are lagged one month because of the delay in announcing formal actions. Here is a graph from the FDIC back to Q1 2006.



On August 7, 2009, we listed 389 institutions with $276 billion in assets, and the list now has 995 institutions and $415 billion in assets.



For Q1 2011, the FDIC listed 888 institutions and $390 billion in assets (somewhat less than the unofficial list a month later). The FDIC Q2 2011 Quarterly Banking Profile will be released in a few weeks.



The unofficial count is close, but is somewhat higher than the official count.



Yesterday:

• Summary for Week ending July 29th

• Schedule for Week of July 31st

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Khan Academy

Khan Academy

Free education!

Muziek helpt bij depressie

Muziek helpt bij depressie: "Nieuw onderzoek bewijst dat mensen met een depressie veel baat kunnen hebben bij muziektherapie. De onderzoekers verzamelden 79 mensen met een...



Lees verder op Scientias.nl >>


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De grote vraag blijft of muziektherapie met alcohol ook baat heeft.

davidup:Don’t play me.

davidup:

Don’t play me.
: "

davidup:



Don’t play me.


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