Marsbugs is published on a weekly to monthly basis as warranted by the number of articles and announcements. Copyright of this compilation exists with the editor, except for specific articles, in which instance copyright exists with the author/authors. Opinions expressed in this newsletter are those of the authors, and are not necessarily endorsed by the editor or by Lyon College. E-mail subscriptions are free, and may be obtained by contacting the editor. Information concerning the scope of this newsletter, subscription formats and availability of back-issues is available at http://www.lyon.edu/projects/marsbugs. The editor does not condone "spamming" of subscribers. Readers would appreciate it if others would not send unsolicited e-mail using the Marsbugs mailing lists. Persons who have information that may be of interest to subscribers of Marsbugs should send that information to the editor.
BOEING DELIVERS JIMO SPACECRAFT DESIGN PROPOSAL
Boeing release
19 July 2004
Boeing delivered its conceptual design proposal Friday, July 16, for the Jupiter Icy Moons Orbiter (JIMO), a spacecraft that could become the nation’s first nuclear-fission-powered exploration vehicle with technologies applicable to future Mars and lunar missions. The JIMO reactor would provide more than 100 times more usable onboard power than has been available to previous science probes and demonstrate nuclear reactors can be operated safely and reliably in space to provide electrical power needed for propulsion and scientific exploration.
A Boeing-led team of engineers and program planners is working with JPL on a groundbreaking initiative that heralds a new era in space science and exploration. The Jupiter Icy Moons Orbiter (JIMO) spacecraft would be the nation’s first nuclear fission reactor-powered scientific spacecraft. It is part of NASA’s Project Prometheus, the space agency’s endeavor to develop safe nuclear power and high-efficiency electric propulsion to open the solar system. With the planet Jupiter as its backdrop, this artist's rendering shows JIMO orbiting the ice-covered Jovian satellites Callisto, Ganymede and Europa. One purpose of the mission is to begin studying the subsurface water ocean suspected to exist on Europa, which could harbor simple extraterrestrial life. JIMO would be the first probe to have the power to orbit multiple planetary objects for weeks at a time. John J. Rankin, artist.
"Through Project Prometheus, NASA is developing space nuclear power and electric propulsion technologies that have the potential to revolutionize space exploration. As envisioned, JIMO would change how humans
explore the solar system," said Mike Mott, Boeing NASA Systems vice president and general manager. "The Boeing team has the large-scale systems integration capability and experience to make it a success."
Boeing submitted the proposal in conjunction with its ongoing $11.8 million Phase A study contract with Jet Propulsion Laboratory (JPL), one of three awarded last year to study options for the reactor, power conversion, electric propulsion and other JIMO subsystems. The orbiter’s proposed mission is to explore Jupiter’s three ice-covered Galilean moons Ganymede, Callisto and Europa and would launch no earlier than 2015, as outlined in the national Vision for Space Exploration.
Boeing’s analysis of the proposed mission would have the JIMO spacecraft embark on a direct five- to eight-year interplanetary journey to reach the icy moons avoiding the time intensive gravity assists often used to sling chemically propelled space probes toward their final destinations. Once at Jupiter, the available power and propulsion systems would give JIMO the capability to explore each icy moon extensively for 30 days or more, providing unprecedented science data about the frozen worlds. The spacecraft would extensively explore the moons’ composition, history and potential for sustaining life. The venture supports the Vision for Space Exploration and NASA’s main goal to explore the universe and search for life.
"Boeing believes that the prudent use of nuclear power is one key to safely and reliably conducting the exploration initiatives NASA is undertaking for America’s future," said Joe Mills, Boeing vice president leading the company’s JIMO efforts. "The Boeing team has a long heritage of successful nuclear power programs and brings technical and management expertise to support the government in this critical area."
The Boeing JIMO program is being led by Phantom Works in partnership with Boeing NASA Systems along with support from Electron Dynamic Devices Inc., for electric propulsion research; Boeing Satellite Systems for spacecraft engineering; and Rocketdyne Propulsion and Power for power conversion and management technologies.
Boeing’s partners include BWX Technologies Inc., Ball Aerospace & Technologies Corp., and General Dynamics Electric Boat. A JIMO spacecraft contractor is expected to be selected in the fall of 2004. Phase B would include the development of system requirements and a preliminary design of the spacecraft. Phase C/D would follow next for the full-scale design, fabrication, integration and test of the space system. Phase E would include launch and post-launch operations. NASA may then contract for up to three additional spacecraft for missions to other outer planet destinations.
Phantom Works is the advanced research and development unit and catalyst of innovation for Boeing. Through its Integrated Defense Advanced Systems group, it provides leading edge systems and technology solutions to Boeing Integrated Defense Systems (IDS), one the world's largest space and defense businesses.
For more information about
the Boeing JIMO initiative, visit http://www.boeing.com/defense-space/space/prometheus/.
Contacts:
Tanya E. Deason-Sharp
Boeing NASA Systems
Phone: 281-226-6070
E-mail: tanya.e.deason-sharp@boeing.com
Glen Golightly
Boeing Phantom Works
Phone: 714-372-4742
E-mail: glen.golightly@boeing.com
Regina W. Carter
BWX Technologies, Inc.
Phone: 434-522-5158
E-mail: rwcarter@bwxt.com
Emilia Reed
Ball Aerospace Technologies & Corp
Phone: 303-939-6551
E-mail: ereed@ball.com
Neil Ruenzel
General Dynamics Electric Boat
Phone: 860-433-8556
An additional article on this subject is available at http://spaceflightnow.com/news/n0407/27jimo/.
INSIDE THE GIANTS: PUZZLING DIFFERENCES IN JUPITER AND SATURN
By Robert Roy Britt
From Space.com
20 July 2004
Scientists aren't sure what the interiors of Jupiter and Saturn look like or how the planets formed. But a new study of their insides suggests they took different paths to giant status. Researchers modeled 50,000 what-ifs of internal structure using real data from the two planets and lab experiments that show how material behaves under extreme pressure. They found Saturn has a huge core and Jupiter may have none.
"Heavy elements are concentrated in Saturn's massive core, while those same elements are mixed throughout Jupiter, with very little or no central core at all," said Didier Saumon of the Los Alamos National Laboratory.
The result, published last week in the Astrophysical Journal, agrees with similar studies but is far more comprehensive. "These conclusions are now very firm," Saumon said in a telephone interview.
Read the full article at http://www.space.com/scienceastronomy/planet_formation_040720.html.
UNIQUE OBSERVATIONS OF NEWBORN STAR PROVIDE INFORMATION ON SOLAR SYSTEM'S ORIGIN
Vanderbilt University release
21 July 2004
A new study has caught a newborn star similar to the sun in a fiery outburst. X-ray observations of the flare-up, which are the first of their kind, are providing important new information about the early evolution of the sun and the process of planet formation. The study, which was conducted by a team of astronomers headed by Joel Kastner of the Rochester Institute of Technology and included David Weintraub from Vanderbilt, is reported in the July 22 issue of the journal
Nature.
Last January, Jay McNeil, an amateur astronomer in West Kentucky, discovered a new cloud of dust and gas in the Orion region. Previously the cloud, now named the McNeil nebula, was not visible from earth. But a new star inside the dark cloud had flared up in brightness, lighting up the surrounding nebula. Looking back at the images taken of this part of the sky revealed that a young star about the size of the sun had burst into visibility last November. Despite the fact that hundreds of telescopes scan the sky nightly, the discovery of a new star is an extremely rare event, having occurred only twice in the last century. What made this star even more special was the fact that it appears to be an extremely young star-far less than a million years old-that is about the same mass as the sun. Astronomers know of fewer
than a dozen of these stars, which they call FU-Orionis-type. Although this is the third FU-Orionis that has been caught in the act of flaring, it is the first that has occurred in modern times when its behavior could be monitored not only in visible light, but also in radio, infrared and X-ray wavelengths.
"In FU-Orionis stars, these outbursts are very brief," says Weintraub, associate professor of astronomy. "They brighten by as much as 100 thousand times in a few months and then fade away over a number of months."
In this X-ray image taken with the Chandra X-ray Observatory in early March, the small orange object near the center is v1647. Photo courtesy of David Weintraub.
Knowing that time was short, Kastner and Weintraub submitted an emergency request for viewing time on the orbiting Chandra X-ray observatory. Because X-rays are generated by extremely violent events, they provide a critical window for observing extreme stellar flare-ups of this sort. The astronomers were granted two viewing times in early and late March. Using Chandra, the astronomers discovered that the star, which has been officially named V1647 Ori, was a very bright X-ray source in early March, but its X-ray brightness had decreased substantially by the end of the month before the star disappeared from view behind the sun. At the same time, the new star was fading in visible and infrared wavelengths.
In
addition, the astronomers learned that Ted Simon from the Institute for Astronomy in Hawaii had taken some serendipitous X-ray images of the same area in 2002 for another purpose. These showed no X-rays coming from the V1647 Ori's location at that time, supporting the idea that the recent X-ray production was directly associated with the star's flare-up. Kastner and Weintraub propose a novel mechanism to explain their observations. Many stars, including the sun, produce X-rays by a mechanism that depends on the star's rotation rate and convection depth. But the astronomers calculate that the temperature of the gas that is producing the X-rays at V1647 ORI is substantially higher than can be explained by this traditional mechanism.
Observations of V1647 Ori indicate that it possesses a "protoplanetary" disk-a thin disk extending out from a star's equator that contains dust and gas left over from the star's formation and from which planets form. Kastner and Weintraub argue that the flare was touched off by a sudden avalanche of disk material falling onto the surface of the star and that this was the source of the intense X-rays as well as the other forms of radiation. If their hypothesis is correct, X-ray observations may help discriminate between young stars that possess protoplanetary disks and those that don't, Weintraub says.
There is a disagreement among astronomers about whether FU-Orionis stars undergo outbursts of this sort only once, several times or dozens of times before they settle into maturity. Other astronomers who have looked further back in the astronomical records for V1647 Ori have found that it also flared up in 1965, which provides added support for the multiple outburst theories.
Other participants in the study were Michael Richmond at the Rochester Institute of Technology, Nicolas Grosso and H. Ozawa at the Laboratoire d'Astrophysique de Grenoble, A. Frank at the University of Rochester, Kenji Hamaguchi at NASA's Goddard Space Flight Center and Arne Henden at the U.S. Naval Observatory.
Kastner and Weintraub have been awarded time to conduct additional observations on Chandra so that they can measure the X-ray activity of the new star beginning in October when it becomes visible once again.
Read the original news release at http://www.vanderbilt.edu/news/releases?id=13096.
An additional article on this subject is available at http://spaceflightnow.com/news/n0407/22newbornstar/.