Category Archives: Solar Science

Space sciences roundup – May.10.2019

A sampling of recent articles, videos, and images from space-related science news items:

** Experiments designed and built by students were among the 38 R&D payloads on the recent Blue Origin New Shepard flight to 106 km:

For example, the UCLA team of 11 students designed and built an experimental magnetic pump named Blue Dawn that will work in zero-gravity:

“The goal was to see if we could design an efficient fluid pump without any moving parts to work in zero-gravity, which has never been done before,” said Alexander Gonzalez, fourth-year physics major and undergrad science lead on the project. Such a low-maintenance pump would be ideal for moving various liquids on the International Space Station, and could reduce the risk of motorized pump failures for rovers and even future bases on the moon or Mars.

** Living tissues embedded in 3D electronics chips were among the research projects on the recent SpaceX Dragon Cargo mission to the ISS. The company Emulate, Inc. sent “organs-on-chips” to the ISS to study the Effects of Microgravity on Human Physiology including

the effect of microgravity and other space-related stressors on the brain blood barrier. It uses fully automated tissue chip technology, a Brain-Chip, consisting of living neuronal and vascular endothelial cells in a micro-engineered environment. Results may provide insight into the relationship between inflammation and brain function and a better understanding of neurodegenerative diseases such as Alzheimer’s and Parkinson’s.

More about tissue chip research in microgravity:

** The latest sunspot count: Sunspot update April 2019: Not quite minimum | Behind The Black

As the Sun ramps down to minimum it will have months where there is no activity, as happened in February 2019, and months, such as in March and April, where more sunspots appear.

Eventually the quiet months will become dominate, and soon thereafter, when activity increases again (assuming it does), the solar science community will then announce the date of true minimum.

We are not there. Normally it can take a year or more for the Sun to settle down. If activity declines as indicated by the red curve, it could take as long four years, which would be a record-long minimum. The difference will tell us whether the eleven-year solar cycle is continuing, or the Sun is heading into a grand minimum, with no significant sunspots for decades.

** Measuring the magnetism of Mars and Jupiter were discussed on the recent TMRO.tv episode Orbit 12.15:

NASA’s MAVEN Magnetometer Instrument Lead Dr. Jared Espley joins us to talk about MAVEN, Juno and how we measure the magnetism of planets in our local system. More information on MAVEN can be found here: https://www.nasa.gov/mission_pages/ma… And more information on Juno can be found here: https://www.nasa.gov/mission_pages/ju…

** The mystery of Mars water remains unsolved: Mars Used to Have Water, But We Can’t Explain How | The Planetary Society

Mars has been the most extensively studied planet in the Solar System, except of course Earth. For the last 25 years, these missions have focused on the search for life by “following the water.” Although we have acquired compelling evidence of flowing liquid water on early Mars, the fundamental question about how water could be stable under Martian atmospheric conditions remains unsolved. Everything we have learned about Mars points towards a freezing cold Martian climate that would be incapable of stabilizing liquid water throughout Mars’ history.

** Even dry asteroids contain water in our wet solar system: Water has been found in dust of an asteroid thought to be bone-dry | Science News

Grains of dust from the asteroid Itokawa actually contain a surprising amount of water, two cosmochemists from Arizona State University in Tempe report May 1 in Science Advances.

“We didn’t really expect water to be there in Itokawa at all,” says study coauthor Maitrayee Bose. But if similar asteroids have similar amounts of water, the space rocks could have been a major source of water for the early Earth.

** More cave openings spotted on Mars and analyzed by Bob Zimmerman: The many pits of Arsia Mons | Behind The Black

Arsia Mons pits 2019. Credits Behind-the-Black

The many pits surrounding Arsia Mons highlight a far greater mystery about Martian geology. Some geologists believe that the many meandering channels we see on Mars could have formed not from surface flow as generally assumed but by underground drainage that washed out voids below the ground which in turn caused the surface to subside, forming those meandering channels.

Yet, as far as I can tell, the only place where scientists have been able to identify a significant number of potential cave openings are on the volcanic slopes of Arisa Mons and its neighboring giant volcanos. There are exceptions, such as this spectacular pit at the head of a channel in the transition zone between the southern highlands and the northern lowlands, as well as two different pits, here and here, that are located in the lowlands in Utopia Basin. Overall however the bulk of pits imaged by MRO appear to be on the slopes of the giant volcanoes, with the majority so far found near Arsia Mons.

** Insight lander images sunrise and sunset on Mars: InSight Captures Sunrise and Sunset on Mars | NASA

A camera on the spacecraft’s robotic arm snapped the photos on April 24 and 25, the 145th Martian day, or sol, of the mission. In local Mars time, the shots were taken starting around 5:30 a.m. and then again starting around 6:30 p.m. As a bonus, a camera under the lander’s deck also caught clouds drifting across the Martian sky at sunset.

Insight captures a sunset.
“NASA’s InSight lander used the Instrument Deployment Camera (IDC) on the end of its robotic arm to image this sunset on Mars on April 25, 2019, the 145th Martian day, or sol, of the mission. This was taken around 6:30 p.m. Mars local time.” Credits: NASA/JPL-Caltech. Full image and caption

** NASA orbiter measures the temperature of Mars moon Phobos: Why This Martian Full Moon Looks Like Candy – NASA JPL

For the first time, NASA’s Mars Odyssey orbiter has caught the Martian moon Phobos during a full moon phase. Each color in this new image represents a temperature range detected by Odyssey’s infrared camera, which has been studying the Martian moon since September of 2017. Looking like a rainbow-colored jawbreaker, these latest observations could help scientists understand what materials make up Phobos, the larger of Mars’ two moons.

Odyssey is NASA’s longest-lived Mars mission. Its heat-vision camera, the Thermal Emission Imaging System (THEMIS), can detect changes in surface temperature as Phobos circles Mars every seven hours. Different textures and minerals determine how much heat THEMIS detects.

Phobos temperature

Such measurements can help determine the composition of the moon, particularly the minerals and metals:

Iron and nickel are two such metals. Depending on how abundant the metals are, and how they’re mixed with other minerals, these data could help determine whether Phobos is a captured asteroid or a pile of Mars fragments, blasted into space by a giant impact long ago.

These recent observations won’t definitively explain Phobos’ origin, Bandfield added. But Odyssey is collecting vital data on a moon scientists still know little about – one that future missions might want to visit. Human exploration of Phobos has been discussed in the space community as a distant, future possibility, and a Japanese sample-return mission to the moon is scheduled for launch in the 2020s.

** Hubble telescope images assembled into a giant mosaic of 265k galaxies: Hubble Assembles Wide View of the Distant Universe | ESA/Hubble

Astronomers developed a mosaic of the distant Universe that documents 16 years of observations from the NASA/ESA Hubble Space Telescope. The image, called the Hubble Legacy Field, contains roughly 265,000 galaxies that stretch back to just 500 million years after the Big Bang.

The wavelength range of this image stretches from ultraviolet to near-infrared light, capturing all the features of galaxy assembly over time. The faintest and farthest galaxies in the image are just one ten-billionth the brightness of what the human eye can observe.

“Now that we have gone wider than in previous surveys, we are harvesting many more distant galaxies in the largest such dataset ever produced,” said Garth Illingworth of the University of California, Santa Cruz, leader of the team that assembled the image. “No image will surpass this one until future space telescopes like James Webb are launched.”

This video “takes the viewer on a journey into the Hubble Legacy Field”:

** Tracking Gaia precisely to get precise locations of a billion stars: Pinpointing Gaia to Map the Milky Way | ESO

This image, a composite of several observations captured by ESO’s VLT Survey Telescope (VST), shows the ESA spacecraft Gaia as a faint trail of dots across the lower half of the star-filled field of view. These observations were taken as part of an ongoing collaborative effort to measure Gaia’s orbit and improve the accuracy of its unprecedented star map.

This image, a composite of several observations captured by ESO’s VLT Survey Telescope (VST), shows the space observatory Gaia as a faint trail of dots across the lower half of the star-filled field of view. These observations were taken as part of an ongoing collaborative effort to measure Gaia’s orbit and improve the accuracy of its unprecedented star map.

Gaia, operated by the European Space Agency (ESA), surveys the sky from orbit to create the largest, most precise, three-dimensional map of our Galaxy. One year ago, the Gaia mission produced its much-awaited second data release, which included high-precision measurements — positions, distance and proper motions — of more than one billion stars in our Milky Way galaxy. This catalogue has enabled transformational studies in many fields of astronomy, addressing the structure, origin and evolution the Milky Way and generating more than 1700 scientific publications since its launch in 2013.

In order to reach the accuracy necessary for Gaia’s sky maps, it is crucial to pinpoint the position of the spacecraft from Earth. Therefore, while Gaia scans the sky, gathering data for its stellar census, astronomers regularly monitor its position using a global network of optical telescopes, including the VST at ESO’s Paranal Observatory [1]. The VST is currently the largest survey telescope observing the sky in visible light, and records Gaia’s position in the sky every second night throughout the year.

** A Galaxy Grouping in 2D and 3D: Stephan’s Quintet;

In 1877, Edouard Stephan discovered a tight visual grouping of five galaxies located in the constellation Pegasus. The galaxies of Stephan’s Quintet are both overlapping and interacting, and have become the most famous among the compact groups of galaxies. Astronomers have long known that four of the galaxies (all of which are yellowish-white in this video) form a physical group in space, while the fifth (bluish) is a foreground galaxy. In addition, a sixth galaxy (yellowish-white and on the far left) is likely to be part of the physical grouping. Hence, this 2D quintet that is a 3D quartet may actually be a 2D sextet that is a 3D quintet.

This visualization makes apparent the spatial distribution of these galaxies. The video starts with a view that matches our 2D perspective. As the sequence travels in 3D, the foreground blue spiral, NGC 7320, quickly passes by the camera. The possible sixth galaxy member on the left, NGC 7320C, is seen at roughly the same distance as the remaining four galaxies. The camera turns to pass between two strongly interacting galaxies, NGC 7319 (left) and NGC 7318B (right), with each galaxy’s spiral structure distorted by the gravitational interaction. In contrast, NGC 7318B overlaps in 2D with the more distant elliptical NGC 7318A, but does not have a strong interaction. The other elliptical, NGC 7317, is also seen as more distant than the strongly interacting pair. In 3D, the four or five galaxies in this group are gathered together by their mutual gravity, and may collide and merge together in the future.

Credits: G. Bacon, J. DePasquale, F. Summers, Z. Levay (STScI)

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Outpost in Orbit: A Pictorial & Verbal History of the Space Station

Space sciences roundup – March.7.2019

A sampling of recent articles, videos, and images related to space related sciences:

** Video shows Hayabusa2 landing on asteroid Ryuga and firing a projectile that stired up material from the surface to allow for capturing samples of the asteroid to return to earth: Watch Hayabusa2’s incredible touchdown on asteroid Ryugu | The Planetary Society

The video was shot with Hayabusa2’s small monitoring camera, CAM-H, which points downward from the side of the main spacecraft bus. Incredibly, the camera was funded by donations from the public!

There’s so much to like about the video: The reflection of Ryugu on Hayabusa2’s shiny surface. The white target marker containing names of Planetary Society members, visible in the lower-left corner for the first part of the video. And, of course, the incredible spray of debris when Hayabusa2 hits the surface and fires its tantalum bullet.

With so much material flying around, the team says “the potential for sample collection is high.” That hopefully includes some larger pieces that either floated directly into the sample catcher or were caught on the inner lip of the sample horn, giving them a chance to tumble up into the catcher later. JAXA also confirmed some debris stuck to the lens of one of the optical navigation cameras.

** NASA’s InSight Mars lander’s drill slowed by hard rock. Mars InSight Lander’s ‘Mole’ Pauses Digging – NASA’s InSight Mars Lander

NASA’s Mars InSight lander has a probe designed to dig up to 16 feet (5 meters) below the surface and measure heat coming from inside the planet. After beginning to hammer itself into the soil on Thursday, Feb. 28, the 16-inch-long (40-centimeter-long) probe — part of an instrument called the Heat and Physical Properties Package, or HP3 — got about three-fourths of the way out of its housing structure before stopping. No significant progress was seen after a second bout of hammering on Saturday, March 2. Data suggests the probe, known as a “mole,” is at a 15-degree tilt.

Scientists suspect it hit a rock or some gravel. The team had hoped there would be relatively few rocks below ground, given how few appear on the surface beside the lander. Even so, the mole was designed to push small rocks aside or wend its way around them. The instrument, which was provided for InSight by the German Aerospace Center (DLR), did so repeatedly during testing before InSight launched.

“The team has decided to pause the hammering for now to allow the situation to be analyzed more closely and jointly come up with strategies for overcoming the obstacle,” HP3 Principal Investigator Tilman Spohn of DLR wrote in a blog post. He added that the team wants to hold off from further hammering for about two weeks.

HP3 on the Martian Surface: NASA’s InSight lander set its heat probe, called the Heat and Physical Properties Package (HP3), on the Martian surface on Feb. 12. Image Credit: NASA/JPL-Caltech/DLR. Full image and caption ›

** Israeli Beresheet lunar probe sends selfie as it moves closer to the Moon: Been here, done that: SpaceIL sends its first selfie from space – ISRAEL21c

The SpaceIL Beresheet lunar lander spacecraft takes a picture of itself along with the Earth in the background.

More background info on the selfie:

** View the Moon in the colors of its minerals in this image created by A James Mccarthy (u/ajamesmccarthy) and posted on Reddit


See also:

** The Chinese Chang’e 4 lander & rover on the far side of the Moon is busy on its third lunar day (equal to 14 earth days):  Yutu-2 Rocks On into Lunar Day 3 for Chang’e-4 mission | The Planetary Society

Yutu-2 awakened for lunar day 3 of the mission at 02:51 UTC on 28 February, with the lander following later the same day at 23:52. A few days later, the rover stood down for its ‘noon nap’ to avoid heating issues from a high solar incidence angle, at 10:25 UTC on March 3. It will resume its activities early on 10 March, before entering a sleep state around 02:00 UTC on 13 March, when the Sun is low in the sky over Von Kármán crater in preparation for the lunar nighttime.

According to a release by the China Lunar Exploration Program (CLEP) on 4 March, Yutu-2 has so far travelled 127 meters, adding 7 meters to the total of 120 meters driven on lunar days 1 (44.185 m) and 2 (75.815 m).

The apparent relatively low distance is believed to be due to Yutu-2 taking time to image nearby rocks and features in the regolith. Analysis of the images from the Visible and Near-Infrared Imaging Spectrometer (VNIS) and Panoramic camera is expected to provide insight into the origin and composition of the rocks and development of the lunar far side itself.

Yutu-2 observes some Moon rocks during the rover’s third Lunar Day since landing on the far side.

** NASA will pay companies with lunar spacecraft for delivery of scientific instruments and experiments to the Moon as soon as their spacecraft are ready to go: NASA Selects Experiments for Possible Lunar Flights in 2019 – NASA

NASA has selected 12 science and technology demonstration payloads to fly to the Moon as early as the end of this year, dependent upon the availability of commercial landers. These selections represent an early step toward the agency’s long-term scientific study and human exploration of the Moon and, later, Mars.

** NASA MAVEN Mars orbiter to support communications with Mars 2020 rover:

NASA’s 4-year-old atmosphere-sniffing Mars Atmosphere and Volatile Evolution (MAVEN) mission is embarking on a new campaign today to tighten its orbit around Mars. The operation will reduce the highest point of the MAVEN spacecraft’s elliptical orbit from 3,850 to 2,800 miles (6,200 to 4,500 kilometers) above the surface and prepare it to take on additional responsibility as a data-relay satellite for NASA’s Mars 2020 rover, which launches next year.

“The MAVEN spacecraft has done a phenomenal job teaching us how Mars lost its atmosphere and providing other important scientific insights on the evolution of the Martian climate,” said Jim Watzin, director of NASA’s Mars Exploration Program. “Now we’re recruiting it to help NASA communicate with our forthcoming Mars rover and its successors.”

While MAVEN’s new orbit will not be drastically shorter than its present orbit, even this small change will significantly improve its communications capabilities. “It’s like using your cell phone,” said Bruce Jakosky, MAVEN principal investigator from the University of Colorado, Boulder. “The closer you are to a cell tower, the stronger your signal.”

Aerobraking plan for MAVEN. (left) Current MAVEN orbit around Mars: 6,200 kilometers (~3,850 miles) at highest altitude, and an orbit period of about 4.5 hours. (center) Aerobraking process: MAVEN performs a series of “deep dip” orbits approaching to within about 125 kilometers (~78 miles) of Mars at lowest altitude, causing drag from the atmosphere to slow down the spacecraft. Over roughly 360 orbits spanning 2.5 months, this technique reduces the spacecraft’s altitude to about 4,500 kilometers (~2,800 miles) and its orbit period to about 3.5 hours. (right) Post-aerobraking orbit, with reduced altitude and shorter orbit period. Credits: NASA’s Scientific Visualization Studio/Kel Elkins and Dan Gallagher. Download in high resolution from the Scientific Visualization Studio

** More Mars caving via images from the Mars Reconnaissance Orbiter (MRO) camera : Another batch of caves/pits found on Mars | Behind The Black

Images from the MRO showing pits, located north and west of Arsia Mons. Credits Bob Zimmerman

The November release imaged three pits found on the southern flanks of Arsia Mons. The January 2019 release found several north of the volcano, two of which are very close to the two middle new pits highlighted above. The February release, which is the focus of this post, included four more pits, shown above, all located north and west of Arsia Mons, as shown in the overview map [shown below in image from Behind the Black].

MRO images of Arsia Mons with notation by Bob Zimmerman.

** Our sun is spotless as it reaches a zero minimum in the current phase of the solar cycle. We will have to wait and see how long it remains in that state. Sunspot update February 2019: The Sun flatlines again | Behind The Black

The number of sunspots in the current cycle since 2008. Annotated by Bob Zimmerman.

** And our solar system is very bigAstronomers discover solar system’s most distant object, nicknamed ‘FarFarOut’ – AAAS

For most people, snow days aren’t very productive. Some people, though, use the time to discover the most distant object in the solar system.

That’s what Scott Sheppard, an astronomer at the Carnegie Institution for Science in Washington, D.C., did this week when a snow squall shut down the city. A glitzy public talk he was due to deliver was delayed, so he hunkered down and did what he does best: sifted through telescopic views of the solar system’s fringes that his team had taken last month during their search for a hypothesized ninth giant planet.

That’s when he saw it, a faint object at a distance 140 times farther from the sun than Earth—the farthest solar system object yet known, some 3.5 times more distant than Pluto. The object, if confirmed, would break his team’s own discovery, announced in December 2018, of a dwarf planet 120 times farther out than Earth, which they nicknamed “Farout.” For now, they are jokingly calling the new object “FarFarOut.” “This is hot off the presses,” he said during his rescheduled talk on 21 February.

** Juno’s Jupiter images never get old: Dramatic Jupiter | NASA

Jupiter’s northern hemisphere as seen by Jupiter in an image enhanced by citizen scientist Kevin M. Gill.

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Chasing New Horizons: Inside the Epic First Mission to Pluto

Videos: TMRO.tv: Space weather, Asgardia, and space news

The latest TMRO.tv Space episode examined space weather:

This week we bring on Dr. Tamitha Skov to talk about Space Weather and it’s impact on your daily life. We also go over how she got started and her journey to becoming the Space Weather Woman.

The previous show dealt with the Asgardia space nation project:

This week we welcome on Lena De Winne, the Deputy Head of Administration of Asgardia to talk about what Asgardia is, what they hope to accomplish and how they will get there. Asgardia is the first Space Nation and you can get more information at asgardia.space.

And here are two TMRO space news videos:

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Space 2.0: How Private Spaceflight, a Resurgent NASA,
and International Partners are Creating a New Space Age

Space science roundup – Feb.9.2019

A sampling of items regarding planetary science, astronomy, and solar science:

** A solar cycle update from Bob Zimmerman:  Sunspot update January 2019: The early solar minimum | Behind The Black

January saw a slight uptick in sunspot activity, but the overall activity remains comparable to mid-2008, when the last prolonged solar minimum began. If you go to my October 2018 update, you can see the graph when it included data going back to 2000 and see the entire last minimum.

That last minimum started in the last half of 2007, and lasted until mid-2009, a full two years. If you look at the red line prediction of the solar science community, it appears that they are expecting this coming minimum to last far longer, almost forever. I expect this is not really true, but that they have simply not agreed on a prediction for the next cycle. Some in that solar science community have hypothesized that we are about to enter a grand minimum, with no sunspots for decades and thus no solar maximum. Others do not agree.

** Mark Showalter,  New Horizons Hazard team lead and SETI Institute Senior Scientist, discusses “the spacecraft’s flyby of Ultima Thule, what it’s like working on the Hazards team, and even the naming of some of Pluto’s surface features” with SETI Institute chief Bill Diamond:

*** Ultima Thule has flat lobes according to further analysis of the image data from the fly-by of the Kuiper Belt object: New Horizons’ Evocative Farewell Glance at Ultima Thule: Images Confirm the Kuiper Belt Object’s Highly Unusual, Flatter Shape – New Horizons

This animation depicts a shape model of Ultima Thule created by the New Horizons science team based on its analysis of all the pre-flyby images sent to Earth so far. The first half of the movie mimics the view from the New Horizons spacecraft as it approached Ultima Thule and has the “snowman” shape that was so frequently mentioned in the days surrounding the New Year’s 2019 flyby.

The movie then rotates to a side-view that illustrates what New Horizons might have seen had its cameras been pointing toward Ultima Thule only a few minutes after closest approach. While that wasn’t the case, mission scientists have been able to piece together a model of this side-view, which has been at least partially confirmed by a set of crescent images of Ultima Thule (link). There is still considerable uncertainty in the sizes of “Ultima” (the larger section, or lobe) and “Thule” (the smaller) in the vertical dimension, but it’s now clear that Ultima looks more like a pancake than a sphere, and that Thule is also very non-spherical.

** Mars:

NASA’s Curiosity Mars Rover has already descended from Vera Rubin Ridge, a region of Mount Sharp that it has been exploring for more than a year. But before it left, the rover took a 360-degree panorama of the area depicting its last drill hole on the ridge (at a location called “Rock Hall”), a new region it will spent the next year exploring (the clay unit) and its last view of Gale Crater’s floor until it starts ascending in elevation again.

At high resolution there does not appear to be much difference between the darker and lighter areas. The lighter areas in general seem less rough and at a slightly lower elevation, but both areas are dominated by ridges and dunes trending southwest-to-northeast.

Why is this slightly higher region darker? Let’s assume that this darker material was a lava flow overlaying the surface. Over eons wind erosion, trending southwest-to-northwest, roughly eroded both it and the lower layers around it, leaving behind this rough corroded terrain. The different make-up of the darker material allows it to erode in a rougher manner.

While possibly correct, I would not bet much money on this guess. It is not clear it is lava. It is not clear that it is a flow. It does not explain why there are two areas of different darkness. And it certainly not clear what the make-up of any of this stuff is.

This is simply another cool mystery on the Martian surface.

Martian southern highlands region showing contrast between lighter and darker tinted areas.

** Moon:

Chang’e-4 lander as seen from the Yutu-2 rover.

** Uranus and Neptune are more interesting than we thought, new images show | Berkeley News

NASA’s Hubble Space Telescope has snapped the latest weather pictures of our solar system’s frigid outer planets, and UC Berkeley astronomers have jumped in to interpret them.

Giant polar cap dominates Uranus; dark tempest is raging on Neptune.

The new images, taken as part of a yearly monitoring program, show that a dark storm has appeared in Neptune’s northern hemisphere, the fourth seen on the planet since 1993, all of which appear and fade within a few years. UC Berkeley undergraduate student Andrew Hsu, who led a study of the latest images with associate research astronomer Michael Wong, estimates that the dark spots appear every four to six years at different latitudes and disappear after about two years.

It’s unclear how the storms form, Hsu said, but like Jupiter’s Great Red Spot, the dark vortices swirl in an anti-cyclonic direction and seem to dredge up material from deeper levels in the ice giant’s atmosphere. The latest storm was captured by Hubble in September 2018 and is roughly 6,800 miles across.

The new snapshot of Uranus gives a fresh look at a long-lived storm circling around the north-pole region of Uranus, a planet that is usually thought of as featureless and boring.

More at Hubble Reveals Dynamic Atmospheres of Uranus and Neptune – HubbleSite

** Asteroids – The DART mission will smack an asteroid with a spacecraft to test deflection capabilities:  The DART Mission: Learning How to Swat Dangerous Asteroids | The Planetary Society

Why did the dinosaurs die? They didn’t have a space program! The upcoming DART mission will test our best thinking about how we may someday deflect a Near Earth Object that is speeding toward fiery Armageddon on Earth. Nancy Chabot of the JHU Applied Physics Lab is the mission’s Coordination Lead.

** Science news is included in the latest TMRO.tv space news report: SpaceX Engine Tests, ISRO Spaceflight, Lunar Craters and SpaceIL

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Space science roundup – Feb.2.2019

A sampling of space and solar science items of interest:

** Parker Solar Probe update:  All Systems Go As Parker Solar Probe Begins Second Sun Orbit – Parker Solar Probe

On Jan. 19, 2019, just 161 days after its launch from Cape Canaveral Air Force Station in Florida, NASA’s Parker Solar Probe completed its first orbit of the Sun, reaching the point in its orbit farthest from our star, called aphelion. The spacecraft has now begun the second of 24 planned orbits, on track for its second perihelion, or closest approach to the Sun, on April 4, 2019.

Parker Solar Probe’s position, speed and round-trip light time as of Jan. 28, 2019. Track the spacecraft online.

** Caves and lava tubes on Mars could provide good locations for early settlements:  The many pits/caves of Mars | Behind The Black

That these pits are all in a line, and that they also in line with a shallow straight depression, strongly suggests that they are skylights into a lava tube below. Located to the northwest of Arsia Mons, the southeast-to-northwest trend of the line reinforces this conclusion, suggesting that we are looking at surface evidence of an underground lava tube that flowed down from Arsia Mons, when that giant volcano was active, eons ago.

Pits Near Arsia Mons. HiRISE on Mars Reconnaissance Orbiter

** Watch a storm on Jupiter as captured by the Juno probe: Jupiter Storm Tracker | NASA

A giant, spiraling storm in Jupiter’s southern hemisphere is captured in this animation from NASA’s Juno spacecraft. The storm is approximately 5,000 miles (8,000 kilometers) across.

The counterclockwise motion of the storm, called Oval BA, is clearly on display. A similar rotation can be seen in the famous Great Red Spot at the top of the animation.

Juno took the nine images used to produce this movie sequence on Dec. 21, between 9:24 a.m. PST (12:24 p.m. EST) and 10:07 a.m. PST (1:07 p.m. EST). At the time the images were taken, the spacecraft was between approximately 15,400 miles (24,800 kilometers) and 60,700 miles (97,700 kilometers) from the planet’s cloud tops above southern latitudes spanning about 36 to 74 degrees.

Citizen scientists Gerald Eichstädt and Seán Doran created this animation using data from the spacecraft’s JunoCam imager.

JunoCam’s raw images are available for the public to peruse and to process into image products at: http://missionjuno.swri.edu/junocam.   

More information about Juno is at: http://www.nasa.gov/juno and http://missionjuno.swri.edu.

** Curiosity sensors measure local gravity and researchers use the data to estimate local ground densities: ‘Mars Buggy’ Curiosity Measures a Mountain’s Gravity | NASA

In a new paper in Science, the researchers detail how they repurposed sensors used to drive the Curiosity rover and turned them into gravimeters, which measure changes in gravitational pull. That enabled them to measure the subtle tug from rock layers on lower Mount Sharp, which rises 3 miles (5 kilometers) from the base of Gale Crater and which Curiosity has been climbing since 2014. The results? It turns out the density of those rock layers is much lower than expected.  

Just like a smartphone, Curiosity carries accelerometers and gyroscopes. Moving your smartphone allows these sensors to determine its location and which way it’s facing. Curiosity’s sensors do the same thing but with far more precision, playing a crucial role in navigating the Martian surface on each drive. Knowing the rover’s orientation also lets engineers accurately point its instruments and multidirectional, high-gain antenna.

A Mars Buggy and a Moon Buggy: Side-by-side images depict NASA’s Curiosity rover (left) and a moon buggy driven during the Apollo 16 mission. Credit: NASA/JPL-Caltech. Full image & caption ›

By happy coincidence, the rover’s accelerometers can be used like Apollo 17’s gravimeter. The accelerometers detect the gravity of the planet whenever the rover stands still. Using engineering data from the first five years of the mission, the paper’s authors measured the gravitational tug of Mars on the rover. As Curiosity ascends Mount Sharp, the mountain adds additional gravity — but not as much as scientists expected.

“The lower levels of Mount Sharp are surprisingly porous,” said lead author Kevin Lewis of Johns Hopkins University. “We know the bottom layers of the mountain were buried over time. That compacts them, making them denser. But this finding suggests they weren’t buried by as much material as we thought.”

** Sounding rocket flies through the Aurora Borealis after launch from Norway:  To Catch a Wave, Rocket Launches From Top of World | NASA

On Jan. 4, 2019, at 4:37 a.m. EST the CAPER-2 mission launched from the Andøya Space Center in Andenes, Norway, on a 4-stage Black Brant XII sounding rocket. Reaching an apogee of 480 miles high before splashing down in the Arctic Sea, the rocket flew through active aurora borealis, or northern lights, to study the waves that accelerate electrons into our atmosphere.

CAPER-2, short for Cusp Alfvén and Plasma Electrodynamics Rocket-2, is a sounding rocket mission — a type of spacecraft that carries scientific instruments on short, targeted trips to space before falling back to Earth. In addition to their relatively low price tags and quick development time, sounding rockets are ideally suited for launching into transient events — like the sudden formation of the aurora borealis, or northern lights.

An animation of the CAPER-2 sounding rocket flight into the aurora borealis.

For CAPER-2 scientists, flying through an aurora provides a peek into a process as fundamental as it is complex: How do particles get accelerated throughout space? NASA studies this phenomenon in an effort to better understand not only the space environment surrounding Earth — and thus protect our technology in space from radiation — but also to help understand the very nature of stars and atmospheres throughout the solar system and beyond.

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