Updates MESSENGER Mission News

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True, but they cheated with Nelson, I think his statue is about 5? times life size. Look a bit daft otherwise, small chap on top of a big plinth.

We do have a version of the Washington Monument:

http://en.wikipedia.org/wiki/Cleopatra's_Needle#London

Napoleon has a lot to answer for...

N.
 

N_Molson

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:rofl:

We have the Egyptian brand of it in Paris, too. Behind the "Assemblée Nationale" (more or less the Congress equivalent).

P1020407_Paris_VIII_Place_de_la_Concorde_Obelisque_rwk.JPG


Back on topic, very interesting data about a place we knew nearly nothing about. :thumbup:
 

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Universe Today: New Features Discovered On Mercury Could Be Evidence Of Hydrogen Geysers And Metallic Iron:
{...}

According to Marvin Herndon, an independent scientist based in San Diego, Mercury formed under great pressure and high temperature – enough to leave iron in a molten state. If so, it should be responsible for absorbing large amounts of hydrogen. As it cools and transforms to a solid state, the hydrogen is then released, forming a type of “geyser” on the planet’s surface.

“These hydrogen geysers could certainly have caused the rimless depressions that MESSENGER sees.” says Herndon, a self-proclaimed maverick in the world of planetary geology.

As the hydrogen is released from below the planet’s surface, it would also react with other elements it would encounter – possibly iron sulphide, commonly found on Mercury’s surface. This would cause a reduction to metallic iron. From there it would form a light “dust” which could account for the bright, new features seen by MESSENGER.

{...}

Technology Review - The Physics arXiv Blog: Hydrogen Geysers And Metallic Iron Could Explain Puzzling Hollows on Mercury
 

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http://messenger.jhuapl.edu/news_room/details.php?id=188

NASA Extends MESSENGER Mission
NASA has announced that it will extend the MESSENGER mission for an additional year of orbital operations at Mercury beyond the planned end of the primary mission on March 17, 2012. The MESSENGER probe became the first spacecraft to orbit the innermost planet on March 18, 2011.
 

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Universe Today: Incredible ‘Sideways’ Look at Mercury’s Limb

Click on images to enlarge​
A mosaic of nine oblique views from the MESSENGER spacecraft of Mercury's limb, looking towards the horizon. Click for larger, more amazing view.
Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington​
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Correlation of features between the limb mosaic and an overhead view.
Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington​
 

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MESSENGER Among Discover Magazine’s Top 100 Stories of 2011

Discover magazine has named the MESSENGER mission one of the top 100 stories of 2011. “The 100 stories here capture scientific curiosity in all its stages: provocative early results, long-sought confirmation, and many steps in the iterative process of testing theory against observation and vice versa,” wrote Discover Editor-in-Chief Corey Powell in the Editor’s Note for the January/February 2012 issue of the magazine.



MESSENGER came in at 25 among the 100. This honor caps off a year of accomplishment for the spacecraft, which entered orbit around Mercury on March 18, 2011, and has since sent back images and other data that have transformed our scientific understanding of the planet closest to the Sun.



The magazine’s article on MESSENGER, entitled “Mercury’s New Face,” was written by noted author Dava Sobel. Sobel was among the visitors to the Johns Hopkins University Applied Physics Laboratory in Laurel, Md., on the occasion of Mercury orbit insertion, and she wrote her story as a first-hand account of that evening.



“The MESSENGER team is honored to be recognized by Discover magazine for our spacecraft’s amazing year,” says MESSENGER Principal Investigator Sean Solomon, of the Carnegie Institution of Washington. “It was particularly special that Discover assigned a writer with the story-telling ability of Dava Sobel to cast the mission’s challenges and opportunities in compelling terms. With NASA’s recent approval of a MESSENGER Extended Mission, we can look forward to another year of scientific surprises at Mercury.”



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MESSENGER (MErcury Surface, Space ENvironment, GEochemistry, and Ranging) is a NASA-sponsored scientific investigation of the planet Mercury and the first space mission designed to orbit the planet closest to the Sun. The MESSENGER spacecraft launched on August 3, 2004, and entered orbit about Mercury on March 18, 2011 (UTC), to begin its primary mission – a one-year study of its target planet. Dr. Sean C. Solomon, of the Carnegie Institution of Washington, leads the mission as Principal Investigator. The Johns Hopkins University Applied Physics Laboratory built and operates the MESSENGER spacecraft and manages this Discovery-class mission for NASA.

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Notebook

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Odd thing, I can normaly paste the content to here, but I get a very strange response from the original:

https://aplive.jhuapl.edu/dana-na/auth/url_default/welcome.cgi

Either way, its honest!


Software Enables Efficient Planning of MESSENGER Observations



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.




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MESSENGER Co-Investigator Named AGU Fellow



James A. Slavin, a MESSENGER Co-Investigator and Chair of the Department of Atmospheric, Oceanic, and Space Sciences at the University of Michigan, has been elected a Fellow of the American Geophysical Union (AGU) for his fundamental contributions to the understanding of solar-wind interactions with the planets and the structure and dynamics of Earth's magnetosphere. He joins a select group of scientists who have been elected by their peers as an AGU Fellow.



Slavin is a leading expert on planetary magnetospheres and how they interact with atmospheres and the solar wind. He has authored more than 300 scientific articles about planetary magnetospheres, magnetic reconnection and substorms, and solar-wind interaction with non-magnetized planets and comets.



He has served on 19 magnetic field investigations (including the Cluster, WIND, Magnetospheric Multiscale, and BepiColombo missions) and five NASA missions. He participated in the development of MESSENGER’s Magnetometer and is leading the analysis of the magnetospheric magnetic field measurements.



Slavin worked at the Jet Propulsion Laboratory, NASA Headquarters, and NASA’s Goddard Space Flight Center before moving to the University of Michigan last year. He has received seven NASA Group Achievement Awards, two NASA Medals for Exceptional Achievement, and the University of California Regent's Fellowship in Space Physics.




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MESSENGER (MErcury Surface, Space ENvironment, GEochemistry, and Ranging) is a NASA-sponsored scientific investigation of the planet Mercury and the first space mission designed to orbit the planet closest to the Sun. The MESSENGER spacecraft launched on August 3, 2004, and entered orbit about Mercury on March 18, 2011 (UTC), to begin a yearlong study of its target planet. Dr. Sean C. Solomon, of the Carnegie Institution of Washington, leads the mission as Principal Investigator. The Johns Hopkins University Applied Physics Laboratory built and operates the MESSENGER spacecraft and manages this Discovery-class mission for NASA.




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Universe Today: Bright Peaks, Dark Shadows

EN0236873588M_web.png

MESSENGER image of Mercury's Amaral crater


Amaral_detail.jpg

Amaral's "blue" peaks seen in a color-enhanced global image acquired Jan. 14, 2008.​
 

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Universe Today: Mercury Down Under

EW0223018028G.3band.nomap_.png

MESSENGER wide-angle camera image of Mercury's southern hemisphere.​
 

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MESSENGER Modifies Orbit to Prepare for Extended Mission



MESSENGER successfully completed an orbit-correction maneuver this evening to lower its periapsis altitude — the lowest point of MESSENGER’s orbit about Mercury relative to the planet’s surface — from 405 to 200 kilometers (251 to 124 miles). This is the first of three planned maneuvers designed to modify the spacecraft’s orbit around Mercury as science operations transition from MESSENGER’s primary orbital mission to its extended mission.



MESSENGER’s orbit around Mercury is highly eccentric, taking it from 200 kilometers (124 miles) above Mercury’s surface to 15,200 kilometers (9,445 miles) altitude every 12 hours. Since orbit insertion nearly one year ago, spacecraft operators at the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland, conducted five earlier maneuvers to counter the perturbing forces that pull MESSENGER away from its preferred observing geometry, including those arising from solar gravity and Mercury’s slight oblateness (the flattening of its spherical shape at the planet’s poles).



For this latest orbit adjustment, MESSENGER was 148 million kilometers (92 million miles) from Earth when the 171-second maneuver, which used all four of the medium-sized monopropellant thrusters on the deck opposite most of the science instruments, began at 8:44 p.m. EST. APL mission controllers verified the start of the maneuver 8 minutes and 12 seconds later, when the first signals indicating spacecraft thruster activity reached NASA’s Deep Space Network tracking station near Canberra, Australia.



In mid-April the team will conduct two additional maneuvers designed to reduce the period of MESSENGER’s orbit around Mercury from 12 to eight hours. According to MESSENGER Principal Investigator Sean Solomon, of the Carnegie Institution of Washington, “This reduction in orbital period will mean that MESSENGER spends a greater fraction of its time close to Mercury’s surface than during the primary mission that is now nearing a successful completion. Moreover, the accomplishment of the global mapping carried out during the primary mission will free many of MESSENGER’s instruments for a new mix of measurements to address a fresh set of scientific objectives that address questions raised by the findings from orbital observations to date.”



“The eight-hour orbit will provide 50% more low-altitude observation opportunities of Mercury’s north polar regions, including permanently shadowed craters,” explains MESSENGER Mission Design Lead Jim McAdams of APL. “A one-third reduction in maximum altitude relative to the 12-hour orbit will enable higher-resolution imaging of the southern hemisphere.”


http://messenger.jhuapl.edu/



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MESSENGER (MErcury Surface, Space ENvironment, GEochemistry, and Ranging) is a NASA-sponsored scientific investigation of the planet Mercury and the first space mission designed to orbit the planet closest to the Sun. The MESSENGER spacecraft launched on August 3, 2004, and entered orbit about Mercury on March 18, 2011 (UTC), to begin its primary mission – a yearlong study of its target planet. MESSENGER’s extended mission begins on March 18, 2012. Dr. Sean C. Solomon, of the Carnegie Institution of Washington, leads the mission as Principal Investigator. The Johns Hopkins University Applied Physics Laboratory built and operates the MESSENGER spacecraft and manages this Discovery-class mission for NASA.


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