NASA – Suzaku ‘Post-mortem’ Yields Insight into Kepler’s Supernova

This composite of images from NASA's Chandra X-ray Observatory shows the remnant of Kepler's supernova in low (red), intermediate (green) and high-energy  (blue) X-rays.

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This composite of images from NASA’s Chandra X-ray Observatory shows the remnant of Kepler’s supernova in low (red), intermediate (green) and high-energy (blue) X-rays. The background is an optical star field taken from the Digitized Sky Survey. The distance to the object is uncertain, with estimates ranging from 13,000 to 23,000 light-years, but recent studies favor the maximum range. This image spans 12 arcminutes or about 80 light-years at the greatest distance.Credit: X-ray: NASA/CXC/NCSU/M.Burkey et al.; optical: DSS

 

An exploding star observed in 1604 by the German astronomer Johannes Kepler held a greater fraction of heavy elements than the sun, according to an analysis of X-ray observations from the Japan-led Suzaku satellite. The findings will help astronomers better understand the diversity of type Ia supernovae, an important class of stellar explosion used in probing the distant universe.

“The composition of the star, its environment, and the mechanism of the explosion may vary considerably among type Ia supernovae,” said Sangwook Park, an assistant professor of physics at the University of Texas at Arlington. “By better understanding them, we can fine-tune our knowledge of the universe beyond our galaxy and improve cosmological models that depend on those measurements.”

The best way to explore the star’s makeup is to perform a kind of post-mortem examination on the shell of hot, rapidly expanding gas produced by the explosion. By identifying specific chemical signatures in the supernova remnant, astronomers can obtain a clearer picture of the composition of the star before it blew up.

via NASA – Suzaku ‘Post-mortem’ Yields Insight into Kepler’s Supernova.

NASA – Remaining Martian Atmosphere Still Dynamic

This image shows the first holes into rock drilled by NASA's Mars rover Curiosity

This image shows the first holes into rock drilled by NASA’s Mars rover Curiosity, with drill tailings around the holes plus piles of powdered rock collected from the deeper hole and later discarded after other portions of the sample had been delivered to analytical instruments inside the rover. Image credit: NASA/JPL-Caltech/MSSS

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VIENNA — Mars has lost much of its original atmosphere, but what’s left remains quite active, recent findings from NASA’s Mars rover Curiosity indicate. Rover team members reported diverse findings today at the European Geosciences Union 2013 General Assembly, in Vienna.

Evidence has strengthened this month that Mars lost much of its original atmosphere by a process of gas escaping from the top of the atmosphere.

Curiosity’s Sample Analysis at Mars (SAM) instrument analyzed an atmosphere sample last week using a process that concentrates selected gases. The results provided the most precise measurements ever made of isotopes of argon in the Martian atmosphere. Isotopes are variants of the same element with different atomic weights. “We found arguably the clearest and most robust signature of atmospheric loss on Mars,” said Sushil Atreya, a SAM co-investigator at the University of Michigan, Ann Arbor.

SAM found that the Martian atmosphere has about four times as much of a lighter stable isotope (argon-36) compared to a heavier one (argon-38). This removes previous uncertainty about the ratio in the Martian atmosphere from 1976 measurements from NASA’s Viking project and from small volumes of argon extracted from Martian meteorites. The ratio is much lower than the solar system’s original ratio, as estimated from argon-isotope measurements of the sun and Jupiter. This points to a process at Mars that favored preferential loss of the lighter isotope over the heavier one.

Curiosity measures several variables in today’s Martian atmosphere with the Rover Environmental Monitoring Station (REMS), provided by Spain. While daily air temperature has climbed steadily since the measurements began eight months ago and is not strongly tied to the rover’s location, humidity has differed significantly at different places along the rover’s route. These are the first systematic measurements of humidity on Mars.

via NASA – Remaining Martian Atmosphere Still Dynamic.

What Is Yuri’s Night?

GLogo

This Friday April 12 at 7:00 pm, join the SIUE STEM Center’s CosmoQuest

and the River Bend Astronomy Club in celebrating Yuri’s Night at Annie’s Frozen Custard in Edwardsville (original location on Buchanan St.)! Yuri’s Night is a global celebration of humanity’s past, present, and future in space. This world wide space party commemorates April 12, 1961, the day of cosmonaut Yuri Gagarin’s first manned spaceflight, and April 12, 1981, the inaugural launch of NASA’s Space Shuttle.

View the night sky through telescopes and binoculars, learn how to find your way around the constellations, and just hang out with other space and astronomy (and frozen custard) enthusiasts!

 If you’d like to help or want last-minute go/cancel information if things are looking stormy, please contact Georgia at gbracey@siue.edu. Unless we’re faced with big storms, we’ll be there. Hope to see you there, too.
 

Blog about last year’s Yuri’s night… use anything you like from that:

http://cosmoquest.org/blog/2012/04/yuris-night-in-edwardsville-who-needs-dark-or-clear-skies/