Wednesday, October 17, 2012
Planetary collision resulted in moon we see
Thursday, June 14, 2012
Science News, the 'Golden Corral' Buffet
[ I didn't read the above post--- I was miffed my essay"God will smite the climate change deniers" didn't even make the first round, of candidates]
Thursday, June 7, 2012
So how did the climate change in the Miocene Era?
Scientists are puzzled today by the discovery that millions of years ago levels of carbon dioxide in the atmosphere were lower [than they are today] - and yet,[the water] temperatures [then] were higher than today's [are].
So begins a writeup about a paper in Nature just published. If you don't have access to the magazine the writeup I reference still contains information about how they determined what the temperature in the miocene era WAS, and how surprised they were to find that apparently the levers of climatic change were different in the miocene than the mechanisms of global change today.
Monday, June 4, 2012
Mind body connection progress perhaps
Nature, June 3
—Washington University in St. Louis
Thursday, May 31, 2012
No traffic lights in the early solar system
Thursday, April 19, 2012
Dark Matter Getting Cloudy
"(Phys.org) -- The most accurate study so far of the motions of stars in the Milky Way has found no evidence for dark matter in a large volume around the Sun. According to widely accepted theories, the solar neighbourhood was expected to be filled with dark matter, a mysterious invisible substance that can only be detected indirectly by the gravitational force it exerts. But a new study by a team of astronomers in Chile has found that these theories just do not fit the observational facts. This may mean that attempts to directly detect dark matter particles on Earth are unlikely to be successful."
Tuesday, April 17, 2012
The stellar source of the elements that compose us
Friday, April 13, 2012
Thursday, April 12, 2012
Unidentifiable spectral lines
The colors of the universe
"If you point a telescope to the sky, you see spectral lines that are very specific to a certain molecule or atom," said Pavanello. Different moleculesemit photons at different wavelengths, which result in different spectral lines that allow astronomers to determine the chemical composition of stars. But the more these telescopes get accurate and precise, the more spectral lines we see."
"We are at a point in which we see many, many more spectral lines than we can possibly identify, and we don't know what these lines mean," said Pavanello.
Knowing the vibrational levels, and therefore the spectral lines of H3+, will allow astronomers and astro-chemists to sift through the inundation of spectral lines and further identify the elemental composition of objects in space.