QueSST Update: NASA's Next X-Plane Briefly Gets Its Nose...

Lockheed Martin

X-59 Nose Makes an Appearance (News Release - September 22)

The X-59 Quiet SuperSonic Technology (QueSST) aircraft is taking shape at the Lockheed Martin Skunk Works facility in Palmdale, California. The team positioned the X-59 QueSST's nose at the front of the aircraft.

As one of the more recognizable features of the X-59, the nose makes up almost a third of the aircraft length and will be essential in shaping shock waves during supersonic flight, resulting in quiet sonic thumps instead of loud sonic booms. The nose was attached and then removed from the front of the aircraft in preparation for its shipment to Fort Worth, Texas where it will undergo additional testing.

The X-59 will fly at supersonic speeds above communities as part of the Low-Boom Flight Demonstration mission, during which NASA will gather community feedback to the sound of quiet supersonic flight. These findings will be shared with regulators to inform decisions on current restrictions of supersonic flight over land.

Source: NASA.Gov

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NASA

Happy First Day of Autumn: A New Discovery Has Been Made by the InSight Mars Lander...

NASA / JPL - Caltech

NASA’s InSight Finds Three Big Marsquakes, Thanks to Solar-Panel Dusting (News Release)

The lander cleared enough dust from one solar panel to keep its seismometer on through the summer, allowing scientists to study the three biggest quakes they’ve seen on Mars.

On Sept. 18, NASA’s InSight lander celebrated its 1,000th Martian day, or sol, by measuring one of the biggest, longest-lasting marsquakes the mission has ever detected. The temblor is estimated to be about a magnitude 4.2 and shook for nearly an hour-and-a-half.

This is the third major quake InSight has detected in a month: On Aug. 25, the mission’s seismometer detected two quakes of magnitudes 4.2 and 4.1. For comparison, a magnitude 4.2 quake has five times the energy of the mission’s previous record holder, a magnitude 3.7 quake detected in 2019.

The mission studies seismic waves to learn more about Mars’ interior. The waves change as they travel through a planet’s crust, mantle, and core, providing scientists a way to peer deep below the surface. What they learn can shed light on how all rocky worlds form, including Earth and its Moon.

The quakes might not have been detected at all had the mission not taken action earlier in the year, as Mars’ highly elliptical orbit took it farther from the Sun. Lower temperatures required the spacecraft to rely more on its heaters to keep warm; that, plus dust buildup on InSight’s solar panels, has reduced the lander’s power levels, requiring the mission to conserve energy by temporarily turning off certain instruments.

The team managed to keep the seismometer on by taking a counterintuitive approach: They used InSight’s robotic arm to trickle sand near one solar panel in the hopes that, as wind gusts carried it across the panel, the granules would sweep off some of the dust. The plan worked, and over several dust-clearing activities, the team saw power levels remain fairly steady. Now that Mars is approaching the Sun once again, power is starting to inch back up.

“If we hadn’t acted quickly earlier this year, we might have missed out on some great science,” said InSight’s principal investigator, Bruce Banerdt of NASA’s Jet Propulsion Laboratory in Southern California, which leads the mission. “Even after more than two years, Mars seems to have given us something new with these two quakes, which have unique characteristics.”

Temblor Insights

While the Sept. 18 quake is still being studied, scientists already know more about the Aug. 25 quakes: The magnitude 4.2 event occurred about 5,280 miles (8,500 kilometers) from InSight – the most distant temblor the lander has detected so far.

Scientists are working to pinpoint the source and which direction the seismic waves traveled, but they know the shaking occurred too far to have originated where InSight has detected almost all of its previous large quakes: Cerberus Fossae, a region roughly 1,000 miles (1,609 kilometers) away where lava may have flowed within the last few million years. One especially intriguing possibility is Valles Marineris, the epically long canyon system that scars the Martian equator. The approximate center of that canyon system is 6,027 miles (9,700 kilometers) from InSight.

To the surprise of scientists, the Aug. 25 quakes were two different types, as well. The magnitude 4.2 quake was dominated by slow, low-frequency vibrations, while fast, high-frequency vibrations characterized the magnitude 4.1 quake. The magnitude 4.1 quake was also much closer to the lander – only about 575 miles (925 kilometers) away.

That’s good news for seismologists: Recording different quakes from a range of distances and with different kinds of seismic waves provides more information about a planet’s inner structure. This summer, the mission’s scientists used previous marsquake data to detail the depth and thickness of the planet’s crust and mantle, plus the size of its molten core.

Despite their differences, the two August quakes do have something in common other than being big: Both occurred during the day, the windiest – and, to a seismometer, noisiest – time on Mars. InSight’s seismometer usually finds marsquakes at night, when the planet cools off and winds are low. But the signals from these quakes were large enough to rise above any noise caused by wind.

Looking ahead, the mission’s team is considering whether to perform more dust cleanings after Mars solar conjunction, when Earth and Mars are on opposite sides of the Sun. Because the Sun’s radiation can affect radio signals, interfering with communications, the team will stop issuing commands to the lander on Sept. 29, though the seismometer will continue to listen for quakes throughout conjunction.

Source: Jet Propulsion Laboratory

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NASA / JPL - Caltech

A Lunar Landing Site Has Finally Been Chosen for the VIPER Rover, Which Is Scheduled to Launch in Late 2023...

NASA Ames / Daniel Rutter

NASA’s Artemis Rover to Land Near Nobile Region of Moon’s South Pole (Press Release)

In 2023, NASA’s Volatiles Investigating Polar Exploration Rover (VIPER) will land near the western edge of the Nobile Crater at the Moon’s South Pole to map and explore the region’s surface and subsurface for water and other resources. Part of Artemis, VIPER will launch on a SpaceX Falcon Heavy rocket for delivery to the Moon by Astrobotic’s Griffin lander under NASA’s Commercial Lunar Payload Services initiative.

The Moon’s South Pole is one of the coldest areas in our solar system. No prior missions to the Moon’s surface have explored it – scientists have thus far only studied the region using remote sensing instruments, including those on NASA’s Lunar Reconnaissance Orbiter and the Lunar Crater Observation and Sensing Satellite.

Data from these and other missions helped scientists conclude that ice and other potential resources exist in permanently shadowed areas of the Moon near the poles. After an extensive landing site selection process, the mountainous area west of Nobile Crater was chosen as VIPER’s landing site due to its rover-accessible terrain and array of nearby sites of scientific interest, including permanently shadowed areas.

“Once on the lunar surface, VIPER will provide ground truth measurements for the presence of water and other resources at the Moon’s South Pole, and the areas surrounding Nobile Crater showed the most promise in this scientific pursuit,” said Thomas Zurbuchen, associate administrator for science at NASA Headquarters. “The data VIPER returns will provide lunar scientists around the world with further insight into our Moon’s cosmic origin, evolution, and history, and it will also help inform future Artemis missions to the Moon and beyond by enabling us to better understand the lunar environment in these previously unexplored areas hundreds of thousands of miles away.”

Nobile Crater is an impact crater that was formed through a collision with another smaller celestial body, and is almost permanently covered in shadows, allowing ice to exist there. Smaller, more accessible craters surrounding Nobile’s perimeter, will also provide VIPER with ideal locations to investigate in its search for ice and other resources.

“Selecting a landing site for VIPER is an exciting and important decision for all of us,” Daniel Andrews, VIPER project manager, said. “Years of study have gone into evaluating the polar region VIPER will explore. VIPER is going into uncharted territory—informed by science—to test hypotheses and reveal critical information for future human space exploration.”

Landing Site Selection

NASA’s team evaluated viable rover traverse paths, taking into account where VIPER could use its solar panels to charge and stay warm during its 100-day journey. The area near Nobile Crater provided a lot of flexibility.

VIPER’s currently planned trajectory allows the rover to visit at least six sites of scientific interest, with additional time to spare.

“Our evaluation of the landing site was driven by science priorities,” said Anthony Colaprete, VIPER lead project scientist at NASA's Ames Research Center in Silicon Valley, California. “We seek answers to some pretty complex questions and studying these resources on the Moon that have stood the test of time will help us answer them.”

The VIPER team aims to address how frozen water and other resources arrived on the Moon in the first place. They also plan to identify where they came from, how they remained preserved for billions of years, how they escape, and where they go.

VIPER’s Journey Across the Nobile Region

The area VIPER will study in the Nobile region covers an approximate surface area of 36 square miles (93 square kilometers), 10 to 15 miles (16 to 24 km) of which VIPER is expected to traverse through during the course of its mission. During this time, the rover will visit carefully chosen areas of scientific interest that will provide further insight into a wide array of different kinds of lunar environments. The VIPER team will look to characterize ice and other resources in these areas using VIPER’s sensors and drill.

As VIPER moves among each area of scientific interest, it will collect samples from at least three drill locations. Analysis of these samples from a variety of depths and temperatures will help scientists to better predict where else ice may be present on the Moon based on similar terrain, allowing NASA to produce a global resource map. This map, and the other science VIPER will produce, will allow scientists to better understand the distribution of resources on the Moon and help inform future crewed missions to establish a long-term presence on the lunar surface.

Source: NASA.Gov

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NASA

20 YEARS LATER...

It was two decades ago on this day that the world was changed by immense tragedy that struck on the east coast of the United States. We will never forget the fallen...

Here's hoping that we remain vigilant, and don't allow history to repeat itself that will cause us to return our brave service members to distant lands—specifically Afghanistan—in the name of the war on terror.

May God bless America, and may God protect our troops.

ABOVE: Photo by Jesse Mills

Perseverance Update: More Info Is Revealed About the Rock the Robotic Rover Extracted Its First Core Samples From...

NASA / JPL - Caltech

NASA’s Perseverance Rover Collects Puzzle Pieces of Mars’ History (Press Release)

NASA’s Perseverance Mars rover successfully collected its first pair of rock samples, and scientists already are gaining new insights into the region. After collecting its first sample, named “Montdenier,” Sept. 1, the team collected a second, “Montagnac,” from the same rock Sept. 7.

Analysis of the rocks from which the Montdenier and Montagnac samples were taken and from the rover’s previous sampling attempt may help the science team piece together the timeline of the area’s past, which was marked by volcanic activity and periods of persistent water.

“It looks like our first rocks reveal a potentially habitable sustained environment,” said Ken Farley of Caltech, project scientist for the mission, which is led by NASA’s Jet Propulsion Laboratory (JPL) in Southern California. “It’s a big deal that the water was there a long time.”

The rock that provided the mission’s first core samples is basaltic in composition and may be the product of lava flows. The presence of crystalline minerals in volcanic rocks is especially helpful in radiometric dating. The volcanic origin of the rock could help scientists accurately date when it formed. Each sample can serve as part of a larger chronological puzzle; put them in the right order, and scientists have a timeline of the most important events in the crater’s history. Some of those events include the formation of Jezero Crater, the emergence and disappearance of Jezero’s lake, and changes to the planet’s climate in the ancient past.

What’s more, salts have been spied within these rocks. These salts may have formed when groundwater flowed through and altered the original minerals in the rock, or more likely when liquid water evaporated, leaving the salts. The salt minerals in these first two rock cores may also have trapped tiny bubbles of ancient Martian water. If present, they could serve as microscopic time capsules, offering clues about the ancient climate and habitability of Mars. Salt minerals are also well-known on Earth for their ability to preserve signs of ancient life.

The Perseverance science team already knew a lake once filled the crater; for how long has been more uncertain. The scientists couldn’t dismiss the possibility that Jezero’s lake was a “flash in the pan”: floodwaters could have rapidly filled the impact crater and dried up in the space of 50 years, for example.

But the level of alteration that scientists see in the rock that provided the core samples – as well as in the rock the team targeted on their first sample-acquisition attempt – suggests that groundwater was present for a long time.

This groundwater could have been related to the lake that was once in Jezero, or it could have traveled through the rocks long after the lake had dried up. Though scientists still can’t say whether any of the water that altered these rocks was present for tens of thousands or for millions of years, they feel more certain that it was there for long enough to make the area more welcoming to microscopic life in the past.

“These samples have high value for future laboratory analysis back on Earth,” said Mitch Schulte of NASA Headquarters, the mission’s program scientist. “One day, we may be able to work out the sequence and timing of the environmental conditions that this rock’s minerals represent. This will help answer the big-picture science question of the history and stability of liquid water on Mars.”

Next Stop, ‘South Séítah’

Perseverance is currently searching the crater floor for samples that can be brought back to Earth to answer profound questions about Mars’ history. Promising samples are sealed in titanium tubes the rover carries in its chassis, where they’ll be stored until Perseverance drops them to be retrieved by a future mission. Perseverance will likely create multiple “depots” later in the mission, where it will drop off samples for a future mission to bring to Earth. Having one or more depots increases the likelihood that especially valuable samples will be accessible for retrieval to Earth.

Perseverance’s next likely sample site is just 656 feet (200 meters) away in “South Séítah,” a series of ridges covered by sand dunes, boulders, and rock shards that Farley likens to “broken dinner plates.”

The rover’s recent drill sample represents what is likely one of the youngest rock layers that can be found on Jezero Crater’s floor. South Séítah, on the other hand, is likely older, and will provide the science team a better timeline to understand events that shaped the crater floor, including its lake.

By the start of October, all Mars missions will be standing down from commanding their spacecraft for several weeks, a protective measure during a period called Mars solar conjunction. Perseverance isn’t likely to drill in South Séítah until sometime after that period.

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NASA / JPL - Caltech

Hubble's Successor Is Now Scheduled to Launch Exactly One Week Before Christmas...

NASA / Chris Gunn

NASA Readies James Webb Space Telescope for December Launch (Press Release)

NASA plans to launch the James Webb Space Telescope into orbit Dec. 18, 2021, to serve as the premier deep space observatory for the next decade.

The agency set the new target launch date in coordination with Arianespace after Webb recently and successfully completed its rigorous testing regimen – a major turning point for the mission. The new date also follows Arianespace successfully launching an Ariane 5 rocket in late July and scheduling a launch that will precede Webb. The July launch was the first for an Ariane 5 since August 2020.

Webb, an international program led by NASA with its partners ESA (European Space Agency) and the Canadian Space Agency, will launch on an Ariane 5 from Europe's Spaceport in French Guiana on the northeastern coast of South America. ESA is providing the Ariane 5.

The highly complex space telescope is currently resting in its final stow configuration at Northrop Grumman’s facilities in Redondo Beach, California.

“Webb is an exemplary mission that signifies the epitome of perseverance,” said Gregory L. Robinson, Webb’s program director at NASA Headquarters in Washington. “I am inspired by our dedicated team and our global partnerships that have made this incredible endeavor possible. Together, we’ve overcome technical obstacles along the way as well as challenges during the coronavirus pandemic. I also am grateful for the steadfast support of Congress. Now that we have an observatory and a rocket ready for launch, I am looking forward to the big day and the amazing science to come.”

The Webb team is preparing for shipment operations, during which the observatory will undergo final closeout procedures and packing for its journey to the launch site. The major elements of the Ariane 5 rocket that will carry Webb into space have safely arrived in Kourou, French Guiana, from Europe.

The Webb telescope’s revolutionary technology will explore every phase of cosmic history – from within our solar system to the most distant observable galaxies in the early universe, and everything in between. Webb will reveal new and unexpected discoveries, and help humankind understand the origins of the universe and our place in it.

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Photos of the Day: Celestial Wonders Above My Street in Los Angeles County...

Happy Tuesday, everyone! Just thought I'd share these images of Jupiter, Saturn and the Big Dipper that I took with my Google Pixel 4A smartphone last week.

Ever since the COVID-19 pandemic began about 18 months ago, I've been taking evening walks around my street in Pomona, California almost every other day. Two of the cool things that I enjoyed looking at during my 1-plus-hour walk were Jupiter and Saturn as these two gas giants were visible in the night sky for much of 2020...until they dipped below the horizon last December.

I even took photos of Jupiter and Saturn (using my Nikon D3300 DSLR camera) a little over a year ago.

It wasn't until recent weeks that Jupiter and Saturn were visible in the evening sky above Southern California once more—and I celebrated their return by taking these photos with my smartphone.

And last Friday, I decided to take pictures of the Big Dipper...which I just found out isn't a constellation itself (it's part of the constellation Ursa Major), but a group of stars known as an asterism. Pretty interesting.

I should go to areas with much darker skies since my Pixel 4A does such an awesome job taking photos in its Night Sight mode. Of course, I also intend on shooting nocturnal images with the Nikon D3300 when I have the chance. I didn't buy a new tripod for it using the stimulus money provided by President Biden and the Democrats earlier this year for nothing!

Carry on.

Perseverance Update: The First Rock Specimen Is Officially Sealed Aboard the Mars Rover...

NASA / JPL - Caltech

NASA’s Perseverance Rover Collects First Mars Rock Sample (Press Release)

NASA’s Perseverance rover today completed the collection of the first sample of Martian rock, a core from Jezero Crater slightly thicker than a pencil. Mission controllers at NASA’s Jet Propulsion Laboratory (JPL) in Southern California received data that confirmed the historic milestone.

The core is now enclosed in an airtight titanium sample tube, making it available for retrieval in the future. Through the Mars Sample Return campaign, NASA and ESA (European Space Agency) are planning a series of future missions to return the rover’s sample tubes to Earth for closer study. These samples would be the first set of scientifically identified and selected materials returned to our planet from another.

“NASA has a history of setting ambitious goals and then accomplishing them, reflecting our nation’s commitment to discovery and innovation,” said NASA Administrator Bill Nelson. “This is a momentous achievement and I can’t wait to see the incredible discoveries produced by Perseverance and our team.”

Along with identifying and collecting samples of rock and regolith (broken rock and dust) while searching for signs of ancient microscopic life, Perseverance’s mission includes studying the Jezero region to understand the geology and ancient habitability of the area, as well as to characterize the past climate.

“For all of NASA science, this is truly a historic moment,” said Thomas Zurbuchen, associate administrator for science at NASA Headquarters in Washington. “Just as the Apollo Moon missions demonstrated the enduring scientific value of returning samples from other worlds for analysis here on our planet, we will be doing the same with the samples Perseverance collects as part of our Mars Sample Return program. Using the most sophisticated science instruments on Earth, we expect jaw-dropping discoveries across a broad set of science areas, including exploration into the question of whether life once existed on Mars.”

First Sample

The sample-taking process began on Wednesday, Sept. 1, when the rotary-percussive drill at the end of Perseverance’s robotic arm cored into a flat, briefcase-size Mars rock nicknamed “Rochette.”

After completing the coring process, the arm maneuvered the corer, bit, and sample tube so the rover’s Mastcam-Z camera instrument could image the contents of the still-unsealed tube and transmit the results back to Earth. After mission controllers confirmed the cored rock’s presence in the tube, they sent a command to complete processing of the sample.

Today, at 12:34 a.m. EDT, Perseverance transferred sample tube serial number 266 and its Martian cargo into the rover’s interior to measure and image the rock core. It then hermetically sealed the container, took another image, and stored the tube.

“With over 3,000 parts, the Sampling and Caching System is the most complex mechanism ever sent into space,” said Larry D. James, interim director of JPL. “Our Perseverance team is excited and proud to see the system perform so well on Mars and take the first step for returning samples to Earth. We also recognize that a worldwide team of NASA, industry partners, academia, and international space agencies contributed to and share in this historic success.”

First Science Campaign

Perseverance is currently exploring the rocky outcrops and boulders of “Artuby,” a ridgeline of more than a half-mile (900 meters) bordering two geologic units believed to contain Jezero Crater’s deepest and most ancient layers of exposed bedrock.

“Getting the first sample under our belt is a huge milestone,” said Perseverance Project Scientist Ken Farley of Caltech. “When we get these samples back on Earth, they are going to tell us a great deal about some of the earliest chapters in the evolution of Mars. But however geologically intriguing the contents of sample tube 266 will be, they won’t tell the complete story of this place. There is a lot of Jezero Crater left to explore, and we will continue our journey in the months and years ahead.”

The rover’s initial science foray, which spans hundreds of sols (Martian days), will be complete when Perseverance returns to its landing site. At that point, Perseverance will have traveled between 1.6 and 3.1 miles (2.5 and 5 kilometers) and may have filled as many as eight of its 43 sample tubes.

After that, Perseverance will travel north, then west, toward the location of its second science campaign: Jezero Crater’s delta region. The delta is the fan-shaped remains of the spot where an ancient river met a lake within the crater. The region may be especially rich in clay minerals. On Earth, such minerals can preserve fossilized signs of ancient microscopic life and are often associated with biological processes.

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NASA / JPL - Caltech

Perseverance Update: The Mars Rover Has Successfully Collected Its First Rock Specimen!

NASA / JPL - Caltech / ASU / MSSS

NASA’s Perseverance Rover Successfully Cores Its First Rock (News Release - September 2)

Perseverance will obtain additional imagery of the sample tube before potentially completing the process of collecting its first scientifically-selected Mars sample.

Data received late Sept. 1 from NASA’s Perseverance rover indicate the team has achieved its goal of successfully coring a Mars rock. The initial images downlinked after the historic event show an intact sample present in the tube after coring. However, additional images taken after the arm completed sample acquisition were inconclusive due to poor sunlight conditions. Another round of images with better lighting will be taken before the sample processing continues.

Obtaining additional imagery prior to proceeding with the sealing and storing of Mars rock sample is an extra step the team opted to include based on its experience with the rover’s sampling attempt on Aug. 5. Although the Perseverance mission team is confident that the sample is in the tube, images in optimal lighting conditions will confirm its presence.

Perseverance’s Sampling and Caching System uses a rotary-percussive drill and a hollow coring bit at the end of its 7-foot-long (2-meter-long) robotic arm to extract samples slightly thicker than a pencil. Within the bit during coring is a sample tube. After completing yesterday’s coring, Perseverance maneuvered the corer, bit, and open end of the sample tube in order to be imaged by the rover’s Mastcam-Z instrument. The target for the sample collection attempt was a briefcase-size rock belonging to a ridgeline that is more than half-a-mile (900 meters) long and contains rock outcrops and boulders.

The initial set of images from Mastcam-Z showed the end of a cored rock within the sample tube. After taking these images, the rover began a procedure called “percuss to ingest,” which vibrates the drill bit and tube for one second, five separate times. The movement is designed to clear the lip of the sample tube of any residual material. The action can also cause a sample to slide down farther into the tube. After the rover finished the percuss-to-ingest procedure, it took a second set of Mastcam-Z images. In these images, the lighting is poor, and internal portions of the sample tube are not visible.

“The project got its first cored rock under its belt, and that’s a phenomenal accomplishment,” said Jennifer Trosper, project manager at NASA’s Jet Propulsion Laboratory in Southern California. “The team determined a location, and selected and cored a viable and scientifically valuable rock. We did what we came to do. We will work through this small hiccup with the lighting conditions in the images and remain encouraged that there is sample in this tube.”

Commands uplinked to the rover earlier today will result in images of the corer and tube to be acquired tomorrow, Sept. 3, at times of day on Mars when the Sun is angled in a more favorable position. Photos will also be taken after sunset to diminish point-sources of light that can saturate an image. The photos will be returned to Earth early in the morning of Sept. 4.

If the results of this additional imaging remain inconclusive, the Perseverance team still has several options to choose from going forward, including using the Sampling and Caching System’s volume probe (located inside the rover’s chassis) as a final confirmation of the sample being in the tube.

The Sept. 1 coring is the second time that Perseverance has employed its Sampling and Caching System since landing in Jezero Crater on Feb. 18, 2021.

Source: Jet Propulsion Laboratory

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NASA / JPL - Caltech / ASU / MSSS


NASA / JPL - Caltech / ASU / MSSS