Half a dozen press releases from NASA this morning, but two in particular caught my eye:
Astronomers are surprised to find the debris belt is wider than previously known, spanning a section of space from 14 to nearly 20 billion miles from the star. Even more surprisingly, the latest Hubble images have allowed a team of astronomers to calculate the planet follows an unusual elliptical orbit that carries it on a potentially destructive path through the vast dust ring.
NASA’s Hubble Reveals Rogue Planetary Orbit for Fomalhaut B.
The discovery of an asteroid belt-like band of debris around Vega makes the star similar to another observed star called Fomalhaut. The data are consistent with both stars having inner, warm belts and outer, cool belts separated by a gap. This architecture is similar to the asteroid and Kuiper belts in our own solar system.
NASA, ESA Telescopes Find Evidence for Asteroid Belt Around Vega.
The more planetary systems we discover and study, the more we find structures that are similar to our own solar system. Here’s a thought: the bigger a star is, the wider it’s habitable zone is.
NASA continues to progress towards a deep space launch vehicles with their Orion spacecraft and capsule:
Recent engineering advances by NASA and its industry partners across the country show important progress toward Exploration Flight Test-1 (EFT-1), the next step to launching humans to deep space. The uncrewed EFT-1 mission, launching from NASA’s Kennedy Space Center in Florida in 2014, will test the re-entry performance of the agency’s Orion capsule, the most advanced spacecraft ever designed, which will carry astronauts farther into space than ever before.
Roemer knew that the true orbital period of Io could have nothing to do with the relative positions of the Earth and Jupiter. In a brilliant insight, he realized that the time difference must be due to the finite speed of light. That is, light from the Jupiter system has to travel farther to reach the Earth when the two planets are on opposite sides of the Sun than when they are closer together. Romer estimated that light required twenty-two minutes to cross the diameter of the Earth’s orbit. The speed of light could then be found by dividing the diameter of the Earth’s orbit by the time difference.
The Dutch scientist Christiaan Huygens, who first did the arithmetic, found a value for the speed of light equivalent to 131,000 miles per second. The correct value is 186,000 miles per second. The difference was due to errors in Roemer’s estimate for the maximum time delay (the correct value is 16.7, not 22 minutes), and also to an imprecise knowledge of the Earth’s orbital diameter. More important than the exact answer, however, was the fact that Roemer’s data provided the first quantitative estimate for the speed of light, and it was in the right ballpark.
What’s interesting was that at the time the true distance from the Earth to the Sun was unknown, making this measurement either incredibly lucky or incredibly insightful.
Excerpt from Cosmic Horizons from the American Museum of Natural History.
If the weather clears up at all this week, there’s a good chance of catching some meteors during the Geminid meteor shower:
This week is a great chance to watch a great meteor shower: the Geminids, so named because they appear to shoot away from the constellation of Gemini. This is a really reliable shower, generally putting out as many as 100 meteors per hour! It peaks on the evening to morning of Dec. 13/14, but usually has a decent showing for a couple of days before and after the peak.
First things first: In November, I posted a how-to guide on watching a meteor shower for the Leonids, another nice annual shower. The instructions for the Geminids are essentially the same. Just replace “Leo” with “Gemini” in your head when you read the guide, and you’ll be fine. Gemini rises in the east around 7:00 p.m. local time, but the best time to observe is after local midnight (see #3 in the how-to guide).
Just remember: if you’re anywhere close to a major city, you’ll have a much better time if you drive somewhere darker. This dark sky map is a good way of finding suitable viewing areas near you: Dark Sky Finder.
via Bad Astronomy.
A brief history of the gas discharge tube, and the first public demonstration of the neon discharge tube 102 years ago today.
Claude’s associate, Jacques Fonseque, sold the first neon-advertising sign to a Paris barber in 1912. The next year saw a breakthrough, as boulevardiers gazed upon 3.5-foot neon letters spelling “CINZANO.”
Claude had applied for a U.S. patent Nov. 9, 1911, and Patent 1,125,476 was awarded Jan. 9, 1915. Claude then sold licenses to the new invention in other countries.
via This Day In Tech | Wired.com.