Friday, December 2, 2011

Astromers Discovery: Some Ancient Stars Have Huge Heavy Metal Deposits

A new study revealed that some ancient stars in the outer reaches of the Milky Way were found to have an unusually large amounts of heavy metals like gold, platinum and uranium.

This discovery has puzzled astronomers as it is the younger generations of stars that typically have an abundance of heavy metals, scientists said.

Researchers tried to unravel the mystery by observing these ancient stars for several years using the European Southern Observatory's fleet of telescopes in Chile, training the telescopes on 17 "abnormal" stars in the Milky Way that were found to be rich in the heaviest chemical elements.

"In the outer parts of the Milky Way there are old 'stellar fossils' from our own galaxy's childhood," the study's lead author Terese Hansen, an astrophysicist at the Niels Bohr Institute at the University of Copenhagen.

"These old stars lie in a halo above and below the galaxy's flat disc. In a small percentage - approximately 1-to-2 percent of these primitive stars - you find abnormal quantities of the heaviest elements relative to iron and other 'normal' heavy elements."

According to the researchers, there are two possible theories to explain these discoveries about ancient stars and both are about supernova explosions.

One theory focuses on the formation of the first stars shortly after the universe was created. The universe then was dominated by light elements like hydrogen and helium and the first stars were formed as clouds of these gasses gathered and collapsed under their own gravity.

The hydrogen and helium in the stars then merged together and formed the first heavy elements like carbon, nitrogen and oxygen.

Supernova explosions cause these stars to die, and the newly formed elements are spread as gas clouds into space, which eventually formed into new stars containing heavier elements.

This process have made the newer generations of stars more abundant with heavy elements.

A second theory is that early supernovas disperse these elements in different directions, which eventually formed some of the stars in the Milky Way. This explains how many of the old stars became abnormally rich in heavy elements, the researchers said.

"In the supernova explosion the heavy elements like gold, platinum and uranium are formed and when the jets hit the surrounding gas clouds, they will be enriched with the elements and form stars that are incredibly rich in heavy elements," Hansen said.

The study was published in the Astrophysical Journal Letters.

Thursday, December 1, 2011

ESA Proba-1 Images of Earth from Space

The Pyramids of Giza, nearby Cairo in Egypt.

The Mysterious and Mystical Uluru or Ayres Rock in Australia.

The Milky Way by ESO Photo Ambassador Yuri Beletsky

An incredible image of the Milky Way by ESO Photo Ambassador Yuri Beletsky.

See 12 more Photos from this series here.

Professor Stephen Hawking welcomes you to YouTube Space Lab - YouTube



"Humanity's future relies on moving beyond Earth. As long as we are confined to one planet, the existence of our species will always be in question. Realising this goal will require an entrepreneurial spirit and a new generation of scientists and astronauts. YouTube Space Lab is a wonderful initiative that will help inspire young minds around the world to take a greater interest in science and the future of space exploration."

- Professor Stephen Hawking, YouTube Space Lab judge.

ESA SOHO: Two Solar Storms

When we combine the narrower and broader fields of view of SOHO's coronagraphs, we can easily track in one image the path of two solar storms (likely coronal mass ejections) as they expand into space (Jan. 13-14, 2011). 

This combining of images is quite easy to do with the newly released JHelioviewer software, described in the recent Hot Shots web area here. 

Before that was released, the effort to overlay images was time-consuming and took a considerable level of skill. 

Both of these storms were identified as events from the far side of the Sun that were not headed toward Earth.

NASA Astronaut Tests SAFER Backpack

Astronaut Mark Lee tests the new backpack called Simplified Aid for EVA Rescue (SAFER), a system designed for use in the event a crew member becomes untethered while conducting an EVA.

The Lidar-In-Space Technology Experiment (LITE) is shown in the foreground. 

The LITE payload employs lidar, which stands for light detection and ranging, a type of optical radar using laser pulses instead of radio waves to study Earth's atmosphere. 

Unprecedented views were obtained of cloud structures, storm systems, dust clouds, pollutants, forest burning, and surface reflectance.

The STS-64 mission marked the first untethered U.S. EVA in 10 years, and was launched on September 9, 1994, aboard the Space Shuttle Orbiter Discovery.

Image Credit: NASA

NASA's NanoSail-D Completes Mission: 240 days

NASA nanosatellite that deployed the agency's first-ever solar sail in low-Earth orbit has successfully completed its Earth Orbiting Mission.

The NanoSail-D, which was launched on Nov. 19, 2010 as a payload on NASA's FASTSAT, has completed more than 240 days "sailing" around the Earth to demonstrate and test the deorbiting capabilities of a large low mass high surface area sail.

"The NanoSail-D mission produced a wealth of data that will be useful in understanding how these types of passive deorbit devices react to the upper atmosphere," said Joe Casas, FASTSAT project scientist at NASA's Marshall Space Flight Center in Huntsville, Ala.


Casas added that the data collected from the mission is being evaluated in relation to data from FASTSAT science experiments which are intended to better understand the drag influences of Earth's upper atmosphere on satellite orbital re-entry.

The FASTSAT science experiments are led by NASA's Goddard Space Flight Center in Greenbelt, Md. and sponsored by the Department of Defense Space Experiments Review Board which is supported by the Department of Defense Space Test Program.

According to the space agency's initial assessment, NanoSail-D exhibited the predicted cyclical deorbit rate behavior that was only previously theorized by researchers.

"The final rate of descent depended on the nature of solar activity, the density of the atmosphere surrounding NanoSail-D and the angle of the sail to the orbital track," said Dean Alhorn, principal investigator for NanoSail-D at Marshall Space Flight Center.

"It is astounding to see how the satellite reacted to the sun's solar pressure. The recent solar flares increased the drag and brought the nanosatellite back home quickly."