Vega, ESA’s new launch vehicle, is ready to operate alongside the Ariane 5 and Soyuz launchers after a successful qualification flight this morning from Europe’s Spaceport in Kourou, French Guiana.(read more)
Source: ESO Photo Release eso1208
ESO’s Very Large Telescope has delivered the most detailed infrared image of the Carina Nebula stellar nursery taken so far. Many previously hidden features, scattered across a spectacular celestial landscape of gas, dust and young stars, have emerged. This is one of the most dramatic images ever created by the VLT. (learn more)
Source: NASA Chandra
The giant black hole at the center of the Milky Way may be vaporizing and devouring asteroids, which could explain the frequent flares observed, according to astronomers using data from NASA's Chandra X-ray Observatory.
For several years Chandra has detected X-ray flares about once a day from the supermassive black hole known as Sagittarius A*, or "Sgr A*" for short. The flares last a few hours with brightness ranging from a few times to nearly one hundred times that of the black hole's regular output. The flares also have been seen in infrared data from ESO's Very Large Telescope in Chile. (read more)
Source: MESSENGER Press Release
SciBox, a scientific planning software package, has proven critical to the success of the MESSENGER mission to Mercury. With completion of the design of all primary-mission observations — including more than 70,000 images and millions of spectral observations — the SciBox software tool has substantially increased, relative to original expectations, the scientific return from the first year of Mercury orbital observations. The spacecraft team is now adapting the system to develop the best plan for MESSENGER’s extended mission, which begins next month.
Software engineers at the Johns Hopkins University Applied Physics Laboratory (APL) in Laurel, Md., designed SciBox for the simulation and planning of mission scientific operations and for the generation of spacecraft and instrument commands. “It is a flexible, adjustable suite of mission-simulation and command-generation tools that models spacecraft performance with high fidelity,” explains APL’s Teck Choo, the creator and architect of SciBox.
SciBox developers worked with the scientists responsible for MESSENGER’s investigations to insert the requirements for all scientific observations into the software’s decision routines. During a planning run, SciBox examines the entire mission, locating the best opportunity for each scientific observation. Then, using a set of intertwined priorities constructed to minimize interference among observations, SciBox schedules the full set of observations for the entire mission.
Once the science and engineering teams verify the plan, SciBox produces the instrument commands, which are combined with telecommunication and power commands and then converted to binary format for transmission to the spacecraft. Because spacecraft pointing is integral to the observation plan, SciBox also plans attitude control maneuvers and produces those commands.
The SciBox planning system has increased the scientific return from MESSENGER in several ways. First, it has reduced the complexity involved in combining the more than 30 different sets of observations from the seven instruments and radio science. “By hand, this intractable problem—to find a fully integrated schedule that accommodates all observations — would be nearly impossible to solve,” states Mark Perry, the science lead for SciBox development. “With SciBox, the scientists can levy any and all types of requirements and constraints on the observations, no matter how intricate, and the SciBox implementation team can create an observing sequence to satisfy them.”
SciBox also helped the team evaluate options. “With SciBox, scientists and planners can modify the observational parameters and evaluate the effect on the entire mission schedule,” Perry says. “Part of SciBox’s output is an extensive set of reports that includes detailed lists, summary statistics, and hundreds of plots that facilitate evaluation of improvements and modifications. With that valuable information, MESSENGER scientists can conduct trades to identify the best approach.”
SciBox can also respond quickly to changes in the mission or requirements. “SciBox can re-plan an entire mission in three hours, including the re-integration of all observations, the generation of commands, and the completion of reports,” says Choo. “If the orbit is slightly different from that expected, or if an instrument’s optimal observing parameters change during the course of the mission, then we modify SciBox and re-run it.”
These same SciBox features have also reduced the risks involved in achieving overall mission objectives. “By planning all the mission observations at once, scientists need not estimate the long-range effects of their requirements,” Perry says. Many of the observing variables are run-time parameters, enabling trade studies without modifying the SciBox code, he explains. With SciBox, planners can also easily investigate the effects of problems and then modify SciBox to develop a plan that is less sensitive to such problems. This rapid response capability minimizes the effect of mission changes by quick re-planning of the full mission.
The SciBox tool continues to evolve. Indeed, one of its advantages is the ease with which it accommodates changes. During MESSENGER’s yearlong primary mission, as the science team has identified new observing opportunities, capability has been added to generate new and improved observations.
For the extended mission, the team developed a version of SciBox that incorporates all of the extended-mission observing requirements defined by MESSENGER’s science team. The SciBox developers examined strategies for accomplishing the new observations and then worked with the scientists to resolve conflicts and ensure that all requirements are met. The result, endorsed by the science team and scheduled to go into effect in March, is a packed plan that achieves a scientific return that exceeds extended mission requirements.
The NASA/ESA Hubble Space Telescope has taken a picture of the barred spiral galaxy NGC 1073, which is found in the constellation of Cetus (The Sea Monster). Our own galaxy, the Milky Way, is a similar barred spiral, and the study of galaxies such as NGC 1073 helps astronomers learn more about our celestial home. (read more)
G350.1-0.3 is a supernova remnant located about 14,700 light years from Earth toward the center of the Milky Way.Vital clues about the devastating ends to the lives of massive stars can be found by studying the aftermath of their explosions.In its more than twelve years of science operations, NASA's Chandra X-ray Observatory has studied many of these supernova remnants sprinkled across the Galaxy.Vital clues about the devastating ends to the lives of massive stars can be found by studying the aftermath of their explosions. In its more than twelve years of science operations, NASA's Chandra X-ray Observatory has studied many of these supernova remnants sprinkled across the Galaxy. (learn more)
Source: ESO Photo Release eso1207
The star formation region NGC 3324. Image credits: ESO.
This new view shows a stellar nursery called NGC 3324. It was taken using the Wide Field Imager on the MPG/ESO 2.2-metre telescope at the La Silla Observatory in Chile. The intense ultraviolet radiation from several of NGC 3324's hot young stars causes the gas cloud to glow with rich colours and has carved out a cavity in the surrounding gas and dust. (read more)
A camera aboard one of NASA's twin Gravity Recovery And Interior Laboratory (GRAIL) lunar spacecraft has returned its first unique view of the far side of the moon. MoonKAM, or Moon Knowledge Acquired by Middle school students, will be used by students nationwide to select lunar images for study.
GRAIL consists of two identical spacecraft, recently named Ebb and Flow, each of which is equipped with a MoonKam. The images were taken as part of a test of Ebb's MoonKam on Jan. 19. The GRAIL project plans to test the MoonKAM aboard Flow at a later date.