Seen here with its robotic arm extended studying a rock called “Athens”, the Mars Exploration Rover Opportunity is still actively involved in science even after 3,970 days on Mars!
A couple of weeks before checking out “Athens” the rover took four images with the Pancam of the area called Marathon Valley located on the western rim of Endeavour Crater from its vantage point overlooking the valley.
The scene spans from east to southeast and the image was taken on 13 March 2015. The view is very close to the true color.
Crew: NASA astronaut Scott Kelly, Russian cosmonauts Mikhail Kornienko and Gennady Padalka
Launch Day / Time: 27 March 2015 at 19:42 UTC / 15:42 EDT
Launch site: Baikonur Cosmodrome, Kazakhstan
Note: Crew members Kelly and Kornienko will be aboard the ISS until March 2016. The long duration is to study how the body reacts and adapts to life in space. The research is needed for future missions say to Mars and may have implications for helping patients here on Earth recovering from long terms of bed rest to helping those with poor immune systems.
Scott Kelly has a twin brother, retired NASA astronaut Mark Kelly who will participate in a number of comparative genetic studies.
From NASA: There are seven key elements of research on the one-year mission. Functional studies will examine crew member performance during and after the 12-month span. Behavioral studies will monitor sleep patterns and exercise routines. Visual impairment will be studied by measuring changes in pressure inside the human skull. Metabolic investigations will examine the immune system and effects of stress. Physical performance will be monitored through exercise examinations. Researchers will also monitor microbial changes in the crew, as well as the human factors associated with how the crew interacts aboard the station.
NASA-TV coverage is scheduled to begin at 18:30 UTC / 14:30 EDT
Last week we had a beautiful display of the aurora courtesy of a solar storm. Other planets are known to have auroral activity. Jupiter included, however the giant planet has auroral activity that isn’t always due to solar storms
The Japan Aerospace Exploration Agency (JAXA) using their Hisaki satellite detected flare-ups get started by the interaction with the Jupiter moon Io and the planet. The results of two months observing Jupiter with Hisaki were published in a paper by Tomoki Kimura of JAXA and his colleagues in Geophysical Research Letters, a journal of the American Geophysical Union.
A Rosetta NAVCAM image of Comet 67P/Churyumov-Gerasimenko from 81.4 km / 50.6 miles. ESA did a nice job of processing the image in order to bring out some of the outflow. The outflow should become more evident over time and give 67P/G-C the classic comet look.
In the mean time Rosetta is intermittently sending radio signals to the Philae lander to establish contact. So far nothing has been heard from the little lander. Possibly the solar panels have not built up enough power in the systems to function or maybe it is just too cold. The lander remains in hibernation.
Philae needs an internal temperature above -45 C / -49 F and five watts of power to turn on – which is pretty impressive. The lander needs to be able to generate 19 watts in order to send signals to Rosetta.
ESA is choosing when to send signals to Philae so the alignment between it and Rosetta and presumably the sun to have the best chance for success. The first half of April will be the next best opportunity to contact.
If you click the image above you will see a version with some of the craters labeled.
This is what Saturn looks like to the Very Large Array or VLA. The VLA “sees” in a part of the spectrum we can’t see – the radio spectrum.
Here’s the NRAO description of the image:
Note the bright disk of the planet with a gradual fading toward the edge, called limb darkening. This illustrates a gradual cooling outward in Saturn’s atmosphere. The rings are seen in emission outside the disk but then in front of the planet they absorb the radiation from the bright disk behind, appearing as a dark band. In visual light they appear bright everywhere because they reflect the incident sunlight but at radio wavelengths the sunlight is fainter and we see the actual emission from Saturn.
Here’s an orthographic look at the north polar region from the Messenger spacecraft. The view is colored by the maximum biannual surface temperature. The temperature ranges from over 400 K / 127 C / 260 F for the red colors down to 50 K / -223 C /-370 F for the purple colors. Temperatures on Mercury do exceed 350 C / 660 F in places.
The largest crater shown is called Prokofiev and it is centered at 85.77 degrees latitude. The interior of the purple colored craters are easily cold enough for water ice to be stable – hard to imagine but true.
There is big news coming in the Messenger mission. The spacecraft is orbiting closer and closer to the surface of the planet being boosted by thrusters when necessary. One orbit brought Messenger to within 11.6 km / 7.2 miles of the surface of Mercury. The Thrusters increased the speed of the spacecraft by 3.07 meters per second or 6.87 miles per hour and increased the minimum close-approach altitude of 34 km / 21.4 miles.
The problem is the propellant is about gone and this means the Messenger spacecraft will end its mission by crashing into the surface of Mercury. There is another thruster maneuver on 02 April, this will probably be the last such event. Messenger is expected to impact the surface of Mercury later in April, May at the latest.
Europe will visit the inner-most planet with the launch of BepiColumbo in 2016 and a trip of 7 years.
The bright flash of a meteor impact was seen on the moon a couple of years ago on 17 March 2013. The flash was some 10 times any flash recorded before. NASA recorded the flash at lunar coordinates 20.6°N, 336.1°E.
The Lunar Reconnaissance Orbiter was able to image the location before and after and it turns out it has found a few more.
The video and a really cool before/after image is located at the NASA site.`