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KECK, HUBBLE IMAGES SHOW CONTINUED TURBULENCE IN JUPITER’S ATMOSPHERE
Berkeley (May 22nd, 2008) Increased turbulence and storms first observed on Jupiter more than two years ago are still raging, according to astronomers from the University of California, Berkeley, and the W. M. Keck Observatory in Hawaii, who snapped high-resolution pictures of the planet earlier this month. Captured with NASA’s Hubble Space Telescope (HST) and […]
Read More >COMPACT GALAXIES IN EARLY UNIVERSE PACK A BIG PUNCH
Baltimore, Md. (April 29th, 2008) Imagine receiving an announcement touting the birth of a baby 20 inches long and weighing 180 pounds. After reading this puzzling message, you would immediately think the baby’s weight was a misprint. Astronomers using NASA’s Hubble Space Telescope and the W. M. Keck Observatory on Mauna Kea, Hawaii, received a […]
Read More >NOVA PHENOMENON EXPLAINED WITH NULLING MODE AT KECK OBSERVATORY
MAUNA KEA (January 28th, 2008) First results from a new scientific instrument at W. M. Keck Observatory are helping scientists understand the physics behind recurrent novae, a type of cataclysmic star system. The results are overturning long-standing assumptions about powerful explosions called novae and have produced the first unified model for a nearby nova called […]
Read More >NASA Mega-Telescope Gears Up to Study Cosmos
(December 5th, 2007) NASA has selected three teams of scientists to begin studying disks of dust around nearby stars starting in February 2008, using the Keck Interferometer in Mauna Kea, Hawaii. This sophisticated new system combines the observing power of the two large Keck telescopes into a single mega-telescope. The announcement follows completion of the […]
Read More >Keck Helps Discover Record Fifth Planet
Berkeley (November 6th, 2007) A team of American astronomers announced the discovery of a record-breaking fifth planet around the nearby star 55 Cancri, making it the only star aside from the sun known to have five planets. The discovery comes after 19 years of observations of 55 Cancri and represents a milestone for the California […]
Read More >Morning forecast on Titan calls for widespread methane drizzle off Xanadu, according to Keck, VLT im
(October 11th, 2007) Berkeley — Noted for its bizarre hydrocarbon lakes and frozen methane clouds, Saturn’s largest moon, Titan, also appears to have widespread drizzles of methane, according to a team of astronomers at the University of California, Berkeley. New near-infrared images from Hawaii’s W. M. Keck Observatory and Chile’s Very Large Telescope show for […]
Read More >Scientists ‘Weigh’ Tiny Galaxy Halfway Across Universe
(October 4th, 2007) Santa Barbara, California –– A tiny galaxy, nearly halfway across the universe, the smallest in size and mass known to exist at that distance, has been identified by an international team of scientists led by two from the University of California, Santa Barbara. The scientists used data collected by NASA’s Hubble Space […]
Read More >Dark, but Light: Smallest Galaxies Ever Seen Solve a Big Problem
Mauna Kea (September 12th, 2007) Mauna Kea scientists may have solved a discrepancy between the number of extremely small, faint galaxies predicted to exist near the Milky Way and the number actually observed. In an attempt to resolve the “Missing Dwarf Galaxy” problem, two astronomers used the W. M. Keck Observatory to study a population […]
Read More >‘One Of The Most Curious Objects In The Sky’ Delights Astronomers Again
Mauna Kea (August 29th, 2007) Edwin Hubble once called IC 10 “one of the most curious objects in the sky,” and new observations of the extremely faint, lightweight dwarf galaxy are giving scientists new clues about how populations of stars are born. Though the properties of stars is one of the most well-studied topics in […]
Read More >Scientists Study Changes In Planets Rings
Berkeley (August 23rd, 2007) As the rings of Uranus swing edge-on to Earth – a short-lived view we get only once every 42 years – astronomers observing the event are getting an unprecedented, glare-free view of the rings and the fine dust that permeates them. The rings were discovered in 1977, so this is the […]
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