Asteroid 87 Sylvia, known since 2001 to be part of a double system, has just gotten more interesting. A team of astronomers at the University of California at Berkeley and the Observatoire de Paris have now established that the asteroid is actually part of a triple system, the first ever discovered. Using data from the European Southern Observatory's Very Large Telescope array in Chile, the team found two small moons in nearly circular orbits. Astronomical names are always a challenge, but in this case naming comes easy. 87 Sylvia was named for Rhea Sylvia, the mother of the founders of Rome. Thus it made perfect sense for Berkeley's Franck Marchis to propose Romulus and Remus as the names of the moons. The suggestion has already been approved by the International Astronomical Union. Image: Artist's conception shows twin moonlets, Romulus and Remus, orbiting the large main-belt asteroid 87 Sylvia. Credit: European Southern Observatory. Calling them 'moons' should not obscure the fact...
New Data on Catastrophic Asteroid Impacts
The recent images from Cassini's flyby of Mimas remind us how violent the history of the early Solar System was. Now a study at the Australian National University shows that three huge asteroids -- between 20 and 50 kilometers across and traveling as a cluster -- collided with the Earth some 3.2 billion years ago. The result: volcanic eruptions, the creation of major fault lines, earthquakes and a variety of disruptive effects deep inside Earth's crust. This work grows out of evidence of extraterrestrial impact deposits from this era discovered in South Africa and extends the effects of those impacts to the Pilbara region of Western Australia. According to an ANU news release, the materials studied in the eastern Transvaal had indicated that impact craters several hundreds of kilometers in diameter had been created in oceanic parts of the Earth. In the Australian studies, the impacts coincide with the formation of fault escarpments and fault troughs and a major volcanic episode....
Finding the Sun’s Twin
A star in the constellation Serpens may be a close match for our own Sun. HD 143436 (also known as HIP 78399, from its listing in the Hipparcos survey) is an 8th magnitude star that's 140 light years from Earth and visible with binoculars. According to a recent article on the star by astronomer Ken Croswell, both its spectral type and its absolute magnitude are closely similar to Sol, and the star appears to be equally hot, with a temperature of 5768 Kelvin vs. the Sun's 5777 K. In terms of mass, HD 143436 is the Sun's twin. Finds like this are intriguing because they raise the possibility that similar stars have similar solar systems, within which may lurk a terrestrial world. No one knows whether this star has a planet like Earth around it -- or any planets at all, for that matter -- but we do know that the close stellar match calls for further work. Exactly how old HD 143436 is remains conjectural, with an uncertainty either way of 2.9 billion years. The star may be as old as the...
Mimas: A Tortured History, and a Warning
Can any other surface in the Solar System be this battered? The twin views below show Saturn's moon Mimas as imaged by Cassini on August 2. Note how the false-color brings out the variation across this tortured surface -- at left is an enhanced clear-filter image, at right a color composite of ultraviolet, infrared and clear-filter images. The most prominent feature in both is the 140-kilometer wide Herschel Crater, an ancient strike that is today filled with landslide material. Close study reveals numerous other craters and long grooves similar to those found on asteroids. Are these grooves related to the enormous impact that created the Herschel crater? No one knows, but study of this moon's turbulent history may help scientists understand how many impactors have moved through the Saturn system, a reminder of how dangerous a place the Solar System can be when you're in the crosshairs of an approaching piece of space debris. Mimas is a tiny place, measuring just 397 kilometers...
A Theory of Interstellar Migration
A continuing preoccupation at Centauri Dreams is long-term thinking. What can we as a species do to extend our time-frame beyond the infuriating short-term outlook of today, so that we can start thinking realistically about shaping a future beyond our own lifetimes? This kind of thinking will be necessary when we build our first interstellar probes, traveling journeys that will surely take decades and may involve centuries. What will drive us to think and plan within the millennial time frames that would allow humans to expand into and throughout the galaxy? Novelist Stephen Baxter addresses this question in a recent paper in the Journal of the British Interplanetary Society. Baxter points out the enormity of the time challenge: Voyager 1, the fastest human object ever built, travels at some 17.3 kilometers per second. It would reach Alpha Centauri (if headed in that direction) in 73,000 years. But starships that can reach 0.1c are not beyond possibility. If we can develop them, it's...
The Search for Missing Quasars
Quasars remain a mystery in several key areas. These massive black holes that live at the center of distant galaxies are voracious, and we know that they can consume the equivalent mass of a thousand stars every year. Surrounded by rings of dust and gas, they light up as they pull in this material to become the fantastically bright objects we observe not just in visible light, but in infrared and x-ray light as well. And that's the problem. To get a count on how many quasars are out there, astronomers have measured the cosmic x-ray background, where quasars outshine everything in the universe. It should be possible to predict how many quasars there are using this method, but it doesn't seem to work. In fact, the estimated number derived from the x-ray background doesn't match the figures derived from x-ray and optical observations of known quasars. In other words, something is hiding many of the universe's quasars from our view. Now the Spitzer Space Telescope has used its infrared...
Life’s Potential in the Early Universe
Complex carbon-based molecules are considered the building blocks of life. Now the Spitzer Space Telescope has detected evidence for molecules made up of hydrogen and carbon in galaxies some 10 billion light years from Earth. The organic compounds -- polycyclic aromatic hydrocarbons, known as 'PAHs' -- are common on Earth and in galaxies like the Milky Way, but no instrument has found them as far back in time as Spitzer. PAHs are called 'organic' because of their carbon atoms. That doesn't translate to 'life-bearing,' for any molecule containing carbon is considered 'organic,' whether or not biology is involved. But find organic compounds and you find at least the potential for life. "This is 10 billion years further back in time than we've seen them before," said Dr. Lin Yan of the Spitzer Science Center at the California Institute of Technology in Pasadena, Calif. Yan and team will publish their findings in the August 10 issue of the Astrophysical Journal. What makes the Spitzer...
Thinking About Cosmos 2
Regular readers of Centauri Dreams will know James Benford as the scientist who showed that microwaves could move a sail in a vacuum. That experiment, performed at the Jet Propulsion Laboratory, involved a 10-kilowatt microwave beam and a 10 sq cm sail in a vacuum chamber. The material used was a carbon fiber material commonly called carbon-carbon, in which carbon molecules are fused together in a structure called a 'microtruss.' Developed by San Diego's Energy Science Research Laboratories, carbon-carbon is terrifically interesting as a possible material for early solar and beamed sail work. The president of Microwave Sciences in Lafayette CA, Benford wrote in a recent e-mail about the failed Cosmos 1 solar sail launch. He had hoped to oversee a microwave experiment using the Deep Space Network's Goldstone facilities to test the effects of a microwave beam on a sail in operational conditions, but that was not to be. At least, not this time. Benford's message is worth quoting, and is...
Sharpening Our View of the 10th Planet
Over the weekend, more news came in about 2003 UB313, the soon to be renamed new planet discovered at Palomar Observatory. As discussed in astronomer Mike Brown's page on the discovery, 2003 UB313 is the largest object found orbiting the Sun since Neptune and its moon Triton in 1846. There seems to be no doubt that it is larger than Pluto and, like that planet, a member of the Kuiper Belt, a vast band of icy objects beyond Neptune. Remarkably, the 2003 UB313 team has found 80 bright Kuiper Belt objects since beginning its survey of the outer Solar System in 2001, but none so newsworthy as this one. Artist2003 UB313 takes twice as long to orbit the Sun as Pluto, and it is currently more than three times more distant, although it moves in an elliptical orbit that can bring it within Pluto's orbit and close to that of Neptune. Size limits can now be set ranging from 2210 to 3550 kilometers, depending on the nature of the surface and how it reflects light. Hubble measurements, already...