The Sky is Waiting.
Why yes, we HAVE seen the ISS!
You just never know when you’ll come face-to-face with Woo.
We recently wrote about Comet ISON on Universe Today and how conspiracy crackpots are already lining up to capitalize on the projected “Comet of the Century.” It’s really win-win for them; if the comet lives up to expectations, there’ll be lots to hype, and if it’s a fizzle, hey, NASA’s “secret mission” must’ve taken it out…
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Quantum physics is perhaps the most arcane field of research out there today. It’s a field where particles pop in and out of existence, actions happen at a distance, and cats in boxes appear to be both alive and dead depending on the actions of the observer. Although there has been much written on the odd world of quantum physics, there are very few books out there for the curious layperson. [Read more...]
Staring into STAR. (Credit: From the Brookhaven National Laboratories’ Flickr stream).
The menagerie of bizarre sub-atomic particles just got stranger, as scientists at Long Islands Relativistic Heavy Ion Collider recently unveiled the discovery of the heaviest anti-particle yet discovered. Dubbed the antihypertriton, this strange beast sits at 200 milli-electron volts (for comparison, an electron volt about 1.602 x 10-19 joules), beating out old fashioned anti-helium. [Read more...]
Out Now from Princeton University Press!
One of the crucial questions in modern cosmology is: why is there anything at all? Why are we here to admire the cosmos, and create books and blogs about how clever we are to figure it all out? Why didn’t the early universe promptly annihilate itself in a massive matter/anti-matter collision? [Read more...]
Hickson Compact Group 31. (Credit: NASA/HST/ESA/S. Gallagher/J. English).
Astronomers may have found a cosmological missing link in the realm of galactic evolution. The early universe was a crowded place; galaxy mergers must have been much more common in the primeval universe than they are today. But studying those early collisions has been problematic; the immense distances involved over time and space mean that resolving clusters and individual stars are out of the question. Now, a team from the University of Western Ontario led by Sara Gallagher has published a study of an object which may serve as a “living fossil” of those early times; Hickson Compact Group 31. A cluster of irregular galaxies “only” 166 million light years away in the constellation Eridanus, this merger has somehow escaped coalescence over 10 billion years of cosmic history to just begin merging. “Because HCG 31 is so nearby,” Gallagher notes, “we can indentify individual star clusters.” In fact, two main components of HCG 31 approach visual magnitude +13 and have been snared by amateur instruments. HCG 31 is approximately 75,000 light years in diameter, and will probably one day form one huge elliptical galaxy. To conduct this study, Gallagher utilized time and instruments that spanned the spectrum, from Hubble in visible light to Spitzer in infrared to Galex and Swift in the ultraviolet. It is amazing that astronomers now have such capabilities in their bag of tricks at their ready disposal!
The LIGO detector at Hanford. (Credit:NSF/LIGO).
Astronomers have added a key tool to their arsenal in probing the very early universe. LIGO, the Laser Interferometer Gravitational wave Observatory, is a pair of “observatories” one in Hanford, Washington, and one in Livingston, Louisiana that monitor the universe for that most exotic of beasts; gravity waves. Each L-shaped detector is comprised of two 2.25 mile long arms and by monitoring the minute changes in length as measured by laser beam, LIGO can detect changes as small as 1/1,000th of the width of an atomic nucleus. By comparing the measurements from the two observatories and its sister companion, a European detector known as Virgo, directional magnitude of cosmic gravity waves can be measured. LIGO saw first “gravity light” in 2002. Late last year, data was released comprising two years’ worth of observations, and a sort of “all-sky map” in gravity waves is emerging. Unlike microwave energy, which can only probe the universe back to an age of about 380,000 years old, gravity waves were generated just moments after the Big Bang, and promise to paint a picture of that youthful era of our universe. LIGO may also prove to be one of the very few testable platforms for string theory, a theory that is very much in need of observational data. And be sure to keep an eye out in 2014 for Advanced LIGO, a detector to go online with 10x the present accuracy… can’t wait? YOU can join the citizen science brigade in the hunt for gravity waves before bedtime; checkout Einstein@home!
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Pictured is a Delta IV rocket launch from Cape Canaveral on November 21st, 2010. The image is a 20 second exposure taken at dusk, shot from about 100 miles west of the launch site. The launch placed a classified payload in orbit for the United States Air Force.
Difficult but not impossible to catch against the dawn or dusk sky, spotting an extreme crescent moon can be a challenge. The slender crescent pictured was shot 30 minutes before sunrise when the Moon was less than 20 hours away from New. A true feat of visual athletics to catch, a good pair of binoculars or a well aimed wide field telescopic view can help with the hunt.
The Sun is our nearest star, and goes through an 11-year cycle of activity. This image was taken via a properly filtered telescope, and shows the Sun as it appeared during its last maximum peak in 2003. This was during solar cycle #23, a period during which the Sun hurled several large flares Earthward. The next solar cycle is due to peak around 2013-14.
Located in the belt of the constellation Orion, Messier 42, also known as the Orion Nebula is one of the finest deep sky objects in the northern hemisphere sky. Just visible as a faint smudge to the naked eye on a clear dark night, the Orion Nebula is a sure star party favorite, as it shows tendrils of gas contrasted with bright stars. M42 is a large stellar nursery, a star forming region about 1,000 light years distant.
Orbiting the planet in Low Earth Orbit (LEO) every 90 minutes, many people fail to realize that you can see the International Space Station (ISS) from most of the planet on a near-weekly basis. In fact, the ISS has been known to make up to four visible passes over the same location in one night. The image pictured is from the Fourth of July, 2011 and is a 20 second exposure of a bright ISS pass.
Next to the Sun, the two brightest objects in the sky are the Moon and the planet Venus. In fact, when Venus is favorably placed next to the Moon, it might just be possible to spot the two in the daytime. Another intriguing effect known as earthshine or ashen light is also seen in the image on the night side of the Moon; this is caused by sunlight reflected back off of the Earth towards our only satellite.
A mosaic of three images taken during the total lunar eclipse of December 21st, 2010. The eclipse occurred the same day as the winter solstice. The curve and size of the Earth’s shadow is apparent in the image.
Review: Brilliant Blunders by Mario Livio
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Many scientific discoveries often come out of left field.
The history of science (if we learn any of the history of science at all in school) is often depicted as a neat, tidy progression from ignorance to enlightenment. How could Isaac Newton not have formulated his laws of gravity and motion, or Einstein not have stumbled on his Theory of Relativity? It all seems foreordained in hindsight. [Read more...]