Robonaut 2 (on left) became the first nonhuman to visit the International Space Station
Space is as hostile as environments come. Astronauts encounter temperatures that swing from 248 F (120 C) to -148 F (-100 C), and that’s just near Earth. The temperature of deep space plummets to -454 F (-270 C). Even the relative comfort of a space station—with its carefully regulated temperature, pressure and mix of gases—offers no escape from the ravages of prolonged exposure to microgravity.
If ever a setting called for robotic assistance, space is that place; but working in place of and, particularly, alongside humans requires a combination of strength, gentleness and dexterity unequaled by robots found anywhere else. Let’s take a look at …
Exoplanet visualization by Supportstorm via Wikimedia Commons
Although astronomers and cosmologists long believed in the existence of planets outside our solar system, such worlds remained purely theoretical until as recently as the early 1990s. Since then, the ever-quickening pace of discovery has filled the roster of possible and confirmed planetary candidates with first tens, then hundreds and now thousands of distant worlds.
In this article, I’ll take you on a tour through the history of planet hunting and into its future. Along the way, we’ll take a look at some of the most significant discoveries, including the candidates most suitable for life as we know it.
More than just skyline blight, smog is an ozone-filled haze packed with the power to inflict or exacerbate ailments in even healthy adults, to say nothing of small children and the elderly. Unfortunately, although scientists know how it forms and even how to detect it, they cannot always predict where it will strike. Now, researchers at Arizona State University and University of California at Berkeley have embarked upon a project that uses NASA satellites to detect smog precursors over a much wider area than before. The research could enable scientists to spot an ozone plume in time to help communities prepare for its health effects.
Infant stars (pink) in the Serpens region, captured by NASA's Spitzer Space Telescope (only somewhat relevant, but still cool).
Using NASA’s Hubble and Spitzer Space Telescopes, an international team of astronomers have found nine of the smallest, faintest, most compact galaxies ever observed in the early universe–the building blocks of today’s larger, older galaxies. Composed of millions of brilliant blue stars, each infantile galaxy is one-hundredth to one-thousandth as large as our Milky Way galaxy. They formed about 12.5 billion years ago – just 1 billion years after the “Big Bang.”
Such galaxies are consistent with the conventional model of galactic formation, which holds that larger galaxies are formed when younger, smaller, less-massive galaxies merge. The sighting thus offers some much-needed support for the “hierarchical model,” which has become ever more contentious in recent years.
