An international project to make the world’s most productive ground-based telescope 10 times more capable has reached its halfway mark and is on schedule to provide astronomers with an extremely powerful new tool for exploring the Universe.
In the thin, dry air of northern Chile’s Atacama Desert, at an altitude of 16,500 feet, an amazing new telescope system is taking shape, on schedule to provide the world’s astronomers with unprecedented views of the origins of stars, galaxies, and planets.
A giant cloud of hydrogen gas is speeding toward a collision with our Milky Way Galaxy, and when it hits — in less than 40 million years — it may set off a spectacular burst of stellar fireworks.
A composite radio-optical image shows five new clouds of hydrogen gas discovered using the National Science Foundation’s Green Bank Telescope.
Astronomers have produced a scientific gold mine of detailed, high-quality images of nearby galaxies that is yielding important new insights into many aspects of galaxies, including their complex structures, how they form stars, the motions of gas in the galaxies, the relationship of normal matter to unseen dark matter, and many others.
Having the sharpest pictures always is a big advantage, and a sophisticated radio-astronomy technique using continent-wide and even intercontinental arrays of telescopes is yielding extremely valuable scientific results in a wide range of specialties. That’s the message delivered to the American Astronomical Society’s meeting in Austin, Texas, by Mark Reid of the Harvard-Smithsonian Center for Astrophysics, a leading researcher in the field of ultra-precise astronomical position measurements.
