Monday, July 31, 2023

Europe's Dark Matter-Detecting Space Telescope Has Opened Its Eye on the Universe...

A first-light image of the universe that was taken by Europe's Euclid space telescope.
ESA / Euclid / Euclid Consortium / NASA, CC BY- SA 3.0 IGO

Euclid Mission to Study Dark Universe Takes First Test Images (News Release)

The telescope took a picture of a glittering field of stars, indicating that it is doing well after a million-mile journey from Earth.

The two instruments aboard Euclid, an ESA (European Space Agency) spacecraft with NASA contributions, have captured their first test images. The results indicate that the space telescope will achieve the scientific goals that it has been designed for – and possibly much more.

The mission will delve into some of the biggest mysteries about our universe, including the nature of dark matter and why the universe’s expansion is accelerating. Scientists call the force behind this accelerated expansion “dark energy.”

Euclid launched on July 1 from Cape Canaveral, Florida. It has arrived at its destination about 1 million miles (1.5 million kilometers) from Earth, a vantage point known as the Second Lagrange Point (L2).

“We are thrilled to see that the NASA-supplied detectors and other hardware are working as expected and are incredibly excited about the scientific results that will come in the months and years ahead,” said Mike Seiffert, project scientist for the NASA contribution to Euclid at the agency’s Jet Propulsion Laboratory in Southern California.

Given these test images, scientists and engineers behind the mission are confident that the telescope and instruments are working well. Mission specialists will continue performance-verification tests for the next couple of months before science observations begin.

“After more than 11 years of designing and developing Euclid, it’s exhilarating and enormously emotional to see these first images,” says Euclid Project Manager Giuseppe Racca of ESA. “It’s even more incredible when we think that we see just a few galaxies here, produced with minimum system tuning. The fully-calibrated Euclid will ultimately observe billions of galaxies to create the biggest-ever 3D map of the sky.”

Source: Jet Propulsion Laboratory

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Monday, July 24, 2023

Hubble's Successor Makes a New Discovery in Our Search for Other Habitable Worlds...

An artist's concept of the star PDS 70 and its inner protoplanetary disk...which contains water vapor as detected by NASA's James Webb Space Telescope.
NASA, ESA, CSA, J. Olmsted (STScI)

Webb Detects Water Vapor in Rocky Planet-Forming Zone (News Release)

Water is essential for life as we know it. However, scientists debate how it reached the Earth and whether the same processes could seed rocky exoplanets orbiting distant stars.

New insights may come from the planetary system PDS 70, located 370 light-years away. The star hosts both an inner disk and outer disk of gas and dust, separated by a 5 billion-mile-wide (8 billion kilometer) gap, and within that gap are two known gas-giant planets.

New measurements by NASA’s James Webb Space Telescope’s MIRI (Mid-Infrared Instrument) have detected water vapor in the system’s inner disk, at distances of less than 100 million miles (160 million kilometers) from the star – the region where rocky, terrestrial planets may be forming. (The Earth orbits 93 million miles from our Sun.)

This is the first detection of water in the terrestrial region of a disk already known to host two or more protoplanets.

“We’ve seen water in other disks, but not so close in and in a system where planets are currently assembling. We couldn’t make this type of measurement before Webb,” said lead author Giulia Perotti of the Max Planck Institute for Astronomy (MPIA) in Heidelberg, Germany.

“This discovery is extremely exciting, as it probes the region where rocky planets similar to Earth typically form,” added MPIA director Thomas Henning, a co-author on the paper. Henning is co-principal investigator of Webb’s MIRI (Mid-Infrared Instrument), which made the detection, and the principal investigator of the MINDS (MIRI Mid-Infrared Disk Survey) program that took the data.

A Steamy Environment for Forming Planets

PDS 70 is a K-type star, cooler than our Sun, and is estimated to be 5.4 million years-old. This is relatively old in terms of stars with planet-forming disks, which made the discovery of water vapor surprising.

Over time, the gas and dust content of planet-forming disks declines. Either the central star’s radiation and winds blow out such material, or the dust grows into larger objects that eventually form planets.

As previous studies failed to detect water in the central regions of similarly-aged disks, astronomers suspected it might not survive the harsh stellar radiation, leading to a dry environment for the formation of any rocky planets.

Astronomers haven’t yet detected any planets forming within the inner disk of PDS 70. However, they do see the raw materials for building rocky worlds in the form of silicates.

The detection of water vapor implies that if rocky planets are forming there, they will have water available to them from the beginning.

“We find a relatively high amount of small dust grains. Combined with our detection of water vapor, the inner disk is a very exciting place,” said co-author Rens Waters of Radboud University in The Netherlands.

What is the Water’s Origin?

The discovery raises the question of where the water came from. The MINDS team considered two different scenarios to explain their finding.

One possibility is that water molecules are forming in place, where we detect them, as hydrogen and oxygen atoms combine. A second possibility is that ice-coated dust particles are being transported from the cool outer disk to the hot inner disk, where the water ice sublimates and turns into vapor.

Such a transport system would be surprising, since the dust would have to cross the large gap carved out by the two giant planets.

Another question raised by the discovery is how water could survive so close to the star, when the star’s ultraviolet light should break apart any water molecules. Most likely, surrounding material such as dust and other water molecules serves as a protective shield.

As a result, the water detected in the inner disk of PDS 70 could survive destruction.

Ultimately, the team will use two more of Webb’s instruments, NIRCam (Near-Infrared Camera) and NIRSpec (Near-Infrared Spectrograph) to study the PDS 70 system in an effort to glean an even greater understanding.

These observations were taken as part of Guaranteed Time Observation program 1282. This finding has been published in the journal Nature.

Source: NASA.Gov

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Spectroscopic data showing the water vapor that was detected at the PDS 70 planetary system by NASA's James Webb Space Telescope.
NASA, ESA, CSA, J. Olmsted (STScI)

Friday, July 21, 2023

Photos of the Day: Snapshots from My Latest Tour at NASA JPL...

A selfie I took with Europa Clipper inside the Spacecraft Assembly Facility at NASA's Jet Propulsion Laboratory near Pasadena, California...on July 20, 2023.

Yesterday, I marked the 54th anniversary of the Apollo 11 Moon landing by attending a tour at NASA's Jet Propulsion Laboratory...which I haven't visited since before the pandemic in early 2019!

The main reason why I went to JPL this time around was to see the Europa Clipper in person. Technicians inside the Spacecraft Assembly Facility are working around the clock to get this robotic probe completed as soon and efficiently as possible.

You can watch the technicians work on Europa Clipper via this live webcam! The unmanned explorer will launch on a six-year journey to Jupiter in October of 2024—courtesy of SpaceX's Falcon Heavy rocket.

It was also great visiting the Space Flight Operations Facility again...as well as seeing full-size replicas of the Perseverance Mars rover, the Ingenuity Mars helicopter and the Mars Ascent Vehicle (MAV) that may or may not send rock samples to an orbiting Martian spacecraft for return back to Earth. Read this latest article about the Mars Sample Return mission to know why I'm not so optimistic about the MAV becoming a reality.

The Europa Clipper should be transported to Cape Canaveral in Florida between May and July of next year to be prepped for launch to Jupiter. I plan on seeing this spacecraft in person one last time before it leaves Southern California...

Whether or not this will be through another tour or the JPL open house (a.k.a. Explore JPL) itself remains to be seen! Happy Friday.

Another photo I took with Europa Clipper inside the Spacecraft Assembly Facility at NASA's Jet Propulsion Laboratory near Pasadena, California...on July 20, 2023.

A snapshot of technicians working on Europa Clipper inside the Spacecraft Assembly Facility at NASA's Jet Propulsion Laboratory near Pasadena, California...on July 20, 2023.

A snapshot of the science instruments and avionics module at the top of the Europa Clipper spacecraft...on July 20, 2023.

A snapshot of technicians working near the bottom of Europa Clipper's propulsion module...on July 20, 2023.

A snapshot of Europa Clipper's high-gain antenna (the large dish covered by a silver tarp) inside the Spacecraft Assembly Facility at NASA's Jet Propulsion Laboratory near Pasadena, California...on July 20, 2023.

Full-size replicas of the Perseverance Mars rover and Ingenuity Mars helicopter on display at NASA's Jet Propulsion Laboratory near Pasadena, California...on July 20, 2023.

A full-size replica of the Mars Ascent Vehicle from NASA's Mars Sample Return mission...which may or may not fly depending on the U.S. Congress.

A snapshot of the Space Flight Operations Facility at NASA's Jet Propulsion Laboratory near Pasadena, California...on July 20, 2023.

Taking a selfie inside the Space Flight Operations Facility at NASA's Jet Propulsion Laboratory near Pasadena, California...on July 20, 2023.

Thursday, July 20, 2023

Webb's Predecessor Took a Stunning Image of DART's Target Last Fall...

An image of Dimorphos, plus 37 free-flying boulders that were jettisoned from the asteroid during DART's impact last September, as seen by NASA's Hubble Space Telescope on December 19, 2022.
NASA, ESA, David Jewitt (UCLA); Alyssa Pagan (STScI)

Hubble Sees Boulders Escaping from Asteroid Dimorphos (News Release)

The popular 1954 rock song Shake, Rattle and Roll could be the theme music for the Hubble Space Telescope's latest discovery about what is happening to the asteroid Dimorphos in the aftermath of NASA's DART (Double Asteroid Redirection Test) experiment. DART intentionally impacted Dimorphos on September 26, 2022, slightly changing the trajectory of its orbit around the larger asteroid Didymos.

Astronomers using Hubble's extraordinary sensitivity have discovered a swarm of boulders that were possibly shaken off the asteroid when NASA deliberately slammed the half-ton DART impactor spacecraft into Dimorphos at approximately 14,000 miles per hour.

The 37 free-flung boulders range in size from three feet to 22 feet across, based on Hubble photometry. They are drifting away from the asteroid at little more than a half-mile per hour – roughly the walking speed of a giant tortoise.

The total mass in these detected boulders is about 0.1% the mass of Dimorphos.

"This is a spectacular observation – much better than I expected. We see a cloud of boulders carrying mass and energy away from the impact target. The numbers, sizes and shapes of the boulders are consistent with them having been knocked off the surface of Dimorphos by the impact," said David Jewitt of the University of California at Los Angeles, a planetary scientist who has been using Hubble to track changes in the asteroid during and after the DART impact. "This tells us for the first time what happens when you hit an asteroid and see material coming out up to the largest sizes. The boulders are some of the faintest things ever imaged inside our solar system."

Jewitt says that this opens up a new dimension for studying the aftermath of the DART experiment using the European Space Agency's upcoming Hera spacecraft, which will arrive at the binary asteroid in late 2026. Hera will perform a detailed post-impact survey of the targeted asteroid.

"The boulder cloud will still be dispersing when Hera arrives," said Jewitt. "It's like a very slowly expanding swarm of bees that eventually will spread along the binary pair's orbit around the Sun."

The boulders are most likely not shattered pieces of the diminutive asteroid caused by the impact. They were already scattered across the asteroid's surface, as evident in the last close-up picture taken by the DART spacecraft just two seconds before collision, when it was only seven miles above the surface.

Jewitt estimates that the impact shook off two percent of the boulders on the asteroid's surface. He says the boulder observations by Hubble also give an estimate for the size of the DART impact crater.

"The boulders could have been excavated from a circle of about 160 feet across (the width of a football field) on the surface of Dimorphos," he said. Hera will eventually determine the actual crater size.

Long ago, Dimorphos may have formed from material shed into space by the larger asteroid Didymos. The parent body may have spun up too quickly or could have lost material from a glancing collision with another object, among other scenarios.

The ejected material formed a ring that gravitationally coalesced to form Dimorphos. This would make it a flying rubble pile of rocky debris loosely held together by a relatively weak pull of gravity.

Therefore, the interior is probably not solid, but has a structure more like a bunch of grapes.

It's not clear how the boulders were lifted off the asteroid's surface. They could be part of an ejecta plume that was photographed by Hubble and other observatories.

Or a seismic wave from the impact may have rattled through the asteroid – like hitting a bell with a hammer – shaking lose the surface rubble.

"If we follow the boulders in future Hubble observations, then we may have enough data to pin down the boulders' precise trajectories. And then we’ll see in which directions they were launched from the surface," said Jewitt.

The DART and LICIACube (Light Italian CubeSat for Imaging of Asteroids) teams have also been studying boulders detected in images taken by LICIACube’s LUKE (LICIACube Unit Key Explorer) camera in the minutes immediately following DART's kinetic impact.

The Hubble Space Telescope is a project of international cooperation between NASA and ESA. NASA's Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope.

The Space Telescope Science Institute (STScI) in Baltimore, Maryland, conducts Hubble and Webb science operations. STScI is operated for NASA by the Association of Universities for Research in Astronomy, in Washington, D.C.

Source: NASA.Gov

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An image of Dimorphos that was taken by NASA's DART spacecraft 11 seconds before it intentionally rammed into the asteroid moonlet...on September 26, 2022.
NASA / Johns Hopkins APL

Tuesday, July 18, 2023

America's Next Asteroid Explorer Is Set to Begin Its Mission Less Than 3 Months from Now...

Technicians work on NASA's Psyche spacecraft inside a clean room at Astrotech Space Operations facility near Kennedy Space Center in Florida...on June 26, 2023.
NASA / Frank Michaux

NASA’s Psyche Mission Enters Home Stretch Before Launch (News Release)

Engineers and technicians at Cape Canaveral are preparing the Psyche spacecraft for liftoff, which is slated for October 5.

With less than 100 days to go before its October 5 launch, NASA’s Psyche spacecraft is undergoing final preparations at Cape Canaveral, Florida. Teams of engineers and technicians are working almost around the clock to ensure the orbiter is ready to journey 2.5 billion miles (4 billion kilometers) to a metal-rich asteroid that may tell us more about planetary cores and how planets form.

The mission team recently completed a comprehensive test campaign of the flight software and installed it on the spacecraft, clearing the hurdle that kept Psyche from making its original 2022 launch date.

“The team and I are now counting down the days to launch,” said Henry Stone, Psyche’s project manager at NASA’s Jet Propulsion Laboratory in Southern California. “Our focus has shifted to safely completing the final mechanical closeout of the spacecraft and preparing the team for operations. The team is conducting numerous training activities to ensure that we are prepared and ready. It’s a very busy time, but everyone is very excited and looking forward to the launch.”

Psyche is set to launch atop a SpaceX Falcon Heavy (the first interplanetary launch for that rocket) from Launch Complex 39A at Kennedy Space Center at 10:38 a.m. EDT (7:38 a.m. PDT) on October 5, with additional opportunities scheduled through October 25. After escaping Earth’s gravity, the Psyche spacecraft will use solar electric propulsion to accomplish its six-year journey to asteroid Psyche.

Measuring about 173 miles (279 kilometers) at its widest point, the asteroid Psyche presents a unique opportunity to explore a metal-rich body that may be part of a core of a planetesimal, the building block of an early planet. Once the spacecraft reaches Psyche in the main asteroid belt between Mars and Jupiter, it will spend at least 26 months orbiting the asteroid, gathering images and other data that will tell scientists more about its history and what it is made of.

Next Steps

But first, a team of 30 or so engineers and technicians will wrap up the assembly, test and launch operations phase of the mission. The team recently finished several weeks of functional testing of the science instruments as well as the spacecraft hardware and software.

After removing the last of the cables that snake around the hardware for testing, they’ll “close out” the spacecraft by reinstalling some exterior panels that had been removed for access and complete the thermal blanketing. Later in July, they will integrate and test the deployment of the enormous solar arrays.

Then, in mid-August, a crew will begin slowly loading all 2,392 pounds (1,085 kilograms) of propellant – the neutral gas xenon – onto the spacecraft over the course of a couple weeks.

Luis Dominguez, the systems and electrical lead for assembly, test and launch operations, is usually based at JPL but has been working full time at the Cape since early June. “We are moving forward,” he said, “and we’re confident that when we’re on the pad, we’ll be ready to hit the button. For all of us, we’ll be excited to launch this bird.”

Source: NASA.Gov

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An artist's concept of NASA's Psyche spacecraft.
NASA / JPL - Caltech / ASU

Thursday, July 13, 2023

Intuitive Machines Is One Step Closer to Launching Its Moon Mission Later This Year...

Intuitive Machines' Nova-C lander is scheduled to lift off from Cape Canaveral Space Force Station in Florida later this year.
Intuitive Machines

Nova-C Lunar Lander Passes Complete Spacecraft Test Run (News Release)

HOUSTON, TX – Intuitive Machines, Inc. (Nasdaq: LUNR, LUNRW) (“Intuitive Machines” or the “Company”), a leading space exploration, infrastructure and services company, has successfully conducted a complete spacecraft test run of its Nova-C lunar lander – a significant technical achievement in the Company’s efforts to completing its lunar lander. The complete spacecraft test run verified Nova-C’s flight software, flight avionics, liquid oxygen and liquid methane loading, high-pressure helium system performance, propulsion system complete functionality, and culminating in a hot fire of the Nova-C main engine.

“This was the most comprehensive test to date short of flying the lander in space,” said Steve Altemus, Intuitive Machines Co-founder, President, and CEO. “This test run represents a crucial step forward in validating the performance of the entire Nova-C lunar lander system on its way to the Moon. The technical excellence the Intuitive Machines team showed during this comprehensive test has propelled the Company closer to delivering Nova-C to Florida for launch.”

The complete spacecraft test run conducted at Intuitive Machines’ Small Vehicle Engine Verification Facility at the Houston Spaceport is a culmination of a series of tests completed during Nova-C’s production.

Comprehensive testing of the full lander with all of its systems powered on and operating is an essential step in the process of verifying all systems are performing as expected. The Nova-C spacecraft systems have been undergoing significant integrated functional testing and checkout in preparation for this fully-integrated performance test.

Source: Intuitive Machines

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An image of Intuitive Machines' Nova-C lander inside the Small Vehicle Engine Verification Facility at Houston Spaceport in Texas.
Intuitive Machines

Wednesday, July 12, 2023

On This Day in 2022: Hubble's Successor Officially Began Its Historic Observation of the Cosmos...

An image of the Rho Ophiuchi cloud complex that was taken by NASA's James Webb Space Telescope.
NASA, ESA, CSA, STScI, Klaus Pontoppidan (STScI)

Webb Celebrates First Year of Science With Close-up on Birth of Sun-like Stars (News Release)

From our cosmic backyard in the solar system to distant galaxies near the dawn of time, NASA’s James Webb Space Telescope has delivered on its promise of revealing the universe like never before in its first year of science operations. To celebrate the completion of a successful first year, NASA has released Webb’s image of a small star-forming region in the Rho Ophiuchi cloud complex.

“In just one year, the James Webb Space Telescope has transformed humanity’s view of the cosmos, peering into dust clouds and seeing light from faraway corners of the universe for the very first time. Every new image is a new discovery, empowering scientists around the globe to ask and answer questions they once could never dream of,” said NASA Administrator Bill Nelson. “Webb is an investment in American innovation but also a scientific feat made possible with NASA’s international partners that share a can-do spirit to push the boundaries of what is known to be possible. Thousands of engineers, scientists and leaders poured their life’s passion into this mission, and their efforts will continue to improve our understanding of the origins of the universe – and our place in it.”

The new Webb image released today features the nearest star-forming region to us. Its proximity at 390 light-years allows for a highly-detailed close-up, with no foreground stars in the intervening space.

“On its first anniversary, the James Webb Space Telescope has already delivered upon its promise to unfold the universe, gifting humanity with a breathtaking treasure trove of images and science that will last for decades,” said Nicola Fox, associate administrator of NASA’s Science Mission Directorate in Washington. “An engineering marvel built by the world’s leading scientists and engineers, Webb has given us a more intricate understanding of galaxies, stars and the atmospheres of planets outside of our solar system than ever before, laying the groundwork for NASA to lead the world in a new era of scientific discovery and the search for habitable worlds.”

Webb’s image shows a region containing approximately 50 young stars, all of them similar in mass to the Sun, or smaller. The darkest areas are the densest, where thick dust cocoons still-forming protostars.

Huge bipolar jets of molecular hydrogen, represented in red, dominate the image, appearing horizontally across the upper third and vertically on the right. These occur when a star first bursts through its natal envelope of cosmic dust, shooting out a pair of opposing jets into space like a newborn first stretching her arms out into the world.

In contrast, the star S1 has carved out a glowing cave of dust in the lower half of the image. It is the only star in the image that is significantly more massive than the Sun.

“Webb’s image of Rho Ophiuchi allows us to witness a very brief period in the stellar lifecycle with new clarity. Our own Sun experienced a phase like this, long ago, and now we have the technology to see the beginning of another’s star’s story,” said Klaus Pontoppidan, who served as Webb project scientist at the Space Telescope Science Institute in Baltimore, Maryland, since before the telescope’s launch and through the first year of operations.

Some stars in the image display tell-tale shadows indicating protoplanetary disks – potential future planetary systems in the making.

A Full Year, Across the Full Sky

From its very first deep field image, unveiled by President Joe Biden, Vice President Kamala Harris and Nelson live at the White House, Webb has delivered on its promise to show us more of the universe than ever before. However, Webb revealed much more than distant galaxies in the early universe.

“The breadth of science Webb is capable of exploring really becomes clear now, when we have a full year’s worth of data from targets across the sky,” said Eric Smith, associate director for research in the Astrophysics Division at NASA Headquarters and Webb program scientist. “Webb’s first year of science has not only taught us new things about our universe, but it has revealed the capabilities of the telescope to be greater than our expectations, meaning future discoveries will be even more amazing.”

The global astronomy community has spent the past year excitedly poring over Webb’s initial public data and getting a feel for how to work with it.

Beyond the stunning infrared images, what really has scientists excited are Webb’s crisp spectra – the detailed information that can be gleaned from light by the telescope’s spectroscopic instruments. Webb’s spectra have confirmed the distances of some of the farthest galaxies ever observed, and have discovered the earliest, most distant supermassive black holes.

They have identified the compositions of planets' atmospheres (or lack thereof) with more detail than ever before, and have narrowed down what kinds of atmospheres may exist on rocky exoplanets for the first time. They have also revealed the chemical makeup of stellar nurseries and protoplanetary disks, detecting water, organic carbon-containing molecules, and more.

Already, Webb observations have resulted in hundreds of scientific papers answering longstanding questions and raising new ones to address with Webb.

The breadth of Webb science is also apparent in its observations of the region of space we are most familiar with – our own solar system. Faint rings of gas giants appear out of the darkness, dotted by moons, while in the background Webb shows distant galaxies.

By comparing detections of water and other molecules in our solar system with those found in the disks of other, much younger planetary systems, Webb is helping to build up clues about our own origins – how Earth became the ideal place for life as we know it.

"With a year of science under our belts, we know exactly how powerful this telescope is, and have delivered a year of spectacular data and discoveries,” said Webb Senior Project Scientist Jane Rigby of NASA's Goddard Space Flight Center. “We've selected an ambitious set of observations for year two — that builds on everything we've learned so far. Webb's science mission is just getting started — there's so much more to come."

Source: NASA.Gov

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Thursday, July 06, 2023

Photos of the Day: America's Next X-Plane Is Almost Ready for Flight...

NASA's X-59 QueSST aircraft sits inside a hangar at Lockheed Martin's Skunk Works facility in Palmdale, California...on June 19, 2023.
Lockheed Martin

NASA’s X-59 Moves Closer to Runway (News Release - July 5)

This series of images shows NASA’s X-59 as it sits on the flight line -- the space between the hangar and the runway -- at Lockheed Martin Skunk Works in Palmdale, California, on June 19, 2023. The move from its construction site to the flight line is one of many milestones that prepare the X-59 for its first and subsequent flights.

Next up, the team will conduct significant ground tests to ensure that the aircraft is safe to fly.

The X-59 aircraft—the centerpiece of NASA’s QueSST mission—is designed to demonstrate the ability to fly supersonic, or faster than Mach 1, while reducing the loud sonic boom to a quiet sonic thump. NASA will then fly the X-59 over several communities to gather data on human responses to the sound generated during supersonic flight.

NASA will deliver that data set to U.S. and international regulators to possibly enable commercial supersonic flight over land.

Source: NASA.Gov

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NASA's X-59 QueSST aircraft sits on the tarmac at Lockheed Martin's Skunk Works facility in Palmdale, California...on June 19, 2023.
Lockheed Martin

NASA's X-59 QueSST aircraft sits on the tarmac at Lockheed Martin's Skunk Works facility in Palmdale, California...on June 19, 2023.
Lockheed Martin

NASA's X-59 QueSST aircraft sits inside a hangar at Lockheed Martin's Skunk Works facility in Palmdale, California...on June 19, 2023.
Lockheed Martin

Wednesday, July 05, 2023

Rock Samples from Asteroid Bennu Will Arrive on Earth Less Than Three Months from Now...

Inside the newly-built OSIRIS-REx Curation Laboratory at NASA's Johnson Space Center in Houston, Texas, technicians rehearse the opening of the asteroid sample canister that will be delivered to Earth from NASA's OSIRIS-REx spacecraft this September.
NASA

NASA Hosts OSIRIS-REx Sample Lab Media Day in Houston (Press Release - June 30)

Ahead of the first asteroid sample collected by the U.S. arriving on Earth in September, media are invited on Monday, July 24, to meet mission scientists and see NASA’s newly-built OSIRIS-REx Sample Curation Laboratory where the agency will study the sample at its Johnson Space Center in Houston.

The asteroid Bennu, the target of the OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification and Security – Regolith Explorer) mission, is a carbonaceous asteroid whose regolith may record the earliest history of our solar system. The Bennu sample may contain the molecular precursors to the origin of life and Earth’s oceans, and its study will also help scientists understand planet formation.

The media day will include opportunities to speak with subject matter experts and capture still and moving imagery at the curation lab. Full interviews with subject matter experts will be available after the lab tour concludes.

U.S. and international media interested in participating must request accreditation no later than 5 p.m. CDT on Friday, July 7, by contacting the NASA Johnson newsroom at: 281-483-5111 or jsccommu@nasa.gov. Media accreditation is limited due to space.

Johnson houses the world’s largest collection of astromaterials from the solar system under one roof, including samples from asteroids, comets, Mars, the Moon, Sun and dust from other stars. Scientists use world-class laboratories to perform research on planetary materials and the space environment to investigate the origin and evolution of our solar system and beyond.

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An animated GIF showing the rotation of asteroid Bennu...using photos taken by NASA's OSIRIS-REx spacecraft from 50 miles (80 kilometers) away.
NASA's Goddard Space Flight Center / University of Arizona

Tuesday, July 04, 2023

OSIRIS-REx Is Getting Closer to Earth...

An artist's concept of OSIRIS-REx's sample return capsule laying in the Utah desert...at the U.S. Army's Dugway Proving Ground.
NASA's Goddard Space Flight Center / Conceptual Image Lab

NASA Offers Media Interviews in Utah on Asteroid Sample Return (Press Release - June 28)

NASA invites media to the U.S. Army’s Dugway Proving Ground about 80 miles southwest of Salt Lake City on Thursday, July 20, before the agency’s first asteroid sample collected in space is returned to Earth.

The sample was collected from the asteroid Bennu in October 2020 by NASA’s OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification and Security – Regolith Explorer) mission, and will arrive via parachute in the Utah desert on September 24.

Media will have the opportunity on July 20 to interview the researchers who provided essential technology that helped OSIRIS-REx capture and store the Bennu sample, as well as learn why NASA selected the Utah desert as the mission’s landing site.

The mission team will also discuss OSIRIS-REx’s landing and recovery operations. Activities for media include a cleanroom facility tour and viewing the sample return capsule training model.

The event is open to U.S. media, who must register online by 5 p.m. MDT on Friday, July 7, for consideration to participate. Check-in at Dugway Proving Ground will be at 8 a.m. on the day of the event.

NASA’s Goddard Space Flight Center in Greenbelt, Maryland, provides overall mission management, systems engineering and the safety and mission assurance for OSIRIS-REx. Dante Lauretta of the University of Arizona, Tucson, is the principal investigator.

The university leads the science team and the mission's science observation planning and data processing. Lockheed Martin Space in Littleton, Colorado, built the spacecraft and provides flight operations.

Goddard and KinetX Aerospace are responsible for navigating the OSIRIS-REx spacecraft. Curation for OSIRIS-REx, including processing the sample when it arrives on Earth, will take place at NASA’s Johnson Space Center in Houston.

International partnerships on this mission include the OSIRIS-REx Laser Altimeter instrument from CSA (Canadian Space Agency) and asteroid sample science collaboration with JAXA’s (Japan Aerospace Exploration Agency) Hayabusa2 mission.

OSIRIS-REx is the third mission in NASA's New Frontiers Program, managed by NASA's Marshall Space Flight Center in Huntsville, Alabama, for the agency's Science Mission Directorate in Washington.

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An artist's concept of NASA's OSIRIS-REx spacecraft approaching asteroid Bennu's surface to obtain soil samples.
NASA / Goddard / University of Arizona

Monday, July 03, 2023

An Interplanetary Chopper Is Ready to Leap into Action Again...

A snapshot of the Ingenuity Mars Helicopter that was taken by NASA's Perseverance rover on April 16, 2023...after the rotorcraft conducted its 50th flight.
NASA / JPL - Caltech / ASU / MSSS

NASA’s Ingenuity Mars Helicopter Phones Home (News Release - June 30)

The intrepid rotorcraft may head skyward again within the next couple of weeks.

The 52nd flight of NASA’s Ingenuity Mars Helicopter is now in the official mission logbook as a success. The flight took place back on April 26, but mission controllers at NASA’s Jet Propulsion Laboratory in Southern California lost contact with the helicopter as it descended towards the surface for a landing.

The Ingenuity team expected the communications dropout because a hill stood between the helicopter’s landing location and the Perseverance rover’s position, blocking communication between the two. The rover acts as a radio relay between the helicopter and mission controllers at JPL.

In anticipation of this loss of communications, the Ingenuity team had already developed re-contact plans for when the rover would drive back within range. Contact was re-established on June 28 when Perseverance crested the hill and could see Ingenuity again.

The goal of Flight 52, a 1,191-foot (363-meter) and 139-second-long flight, was to reposition the helicopter and take images of the Martian surface for the rover’s science team.

“The portion of Jezero Crater the rover and helicopter are currently exploring has a lot of rugged terrain, which makes communications dropouts more likely,” said JPL’s Josh Anderson, the Ingenuity team lead. “The team’s goal is to keep Ingenuity ahead of Perseverance, which occasionally involves temporarily pushing beyond communication limits. We’re excited to be back in communications range with Ingenuity and receive confirmation of Flight 52.”

Sixty-three days is a long time to wait for the results of a flight, but the data coming in indicates all is well with the first aircraft on another world. If the remainder of Ingenuity’s health checks are equally rosy, the helicopter may fly again within the next couple of weeks.

Source: Jet Propulsion Laboratory

Sunday, July 02, 2023

A Dark Matter-Detecting Space Telescope Has Slipped the Surly Bonds of Earth Yesterday...

A SpaceX Falcon 9 rocket carrying the European Space Agency's Euclid telescope launches from Cape Canaveral Space Force Station in Florida...on July 1, 2023.
SpaceX

ESA’s Euclid Mission Launches to Explore ‘Dark Universe’ (News Release - July 1)

NASA is contributing to the European Space Agency mission, which will complement dark energy studies by the agency’s upcoming Nancy Grace Roman Space Telescope.

The ESA (European Space Agency) Euclid spacecraft lifted off from Cape Canaveral Space Force Station in Florida at 11:12 a.m. EDT on Saturday, July 1, beginning its mission to study why the universe is expanding at an accelerating rate. Astronomers use the term “dark energy” in reference to the unknown cause of this accelerated expansion.

NASA’s Jet Propulsion Laboratory in Southern California delivered critical hardware for one of the Euclid spacecraft’s instruments. In addition, NASA has established a U.S.-based Euclid science data center, and NASA-funded science teams will join other Euclid scientists in studying dark energy, galaxy evolution and dark matter.

The agency’s forthcoming Nancy Grace Roman mission will also study dark energy – in ways that are complementary to Euclid. Mission planners will use Euclid’s findings to inform Roman’s dark energy work.

After the Euclid spacecraft separated from the second stage of a SpaceX Falcon 9 rocket, ESA announced a successful launch. Euclid will undergo a series of checks and calibrations before it starts collecting science data in about three months.

“We are thrilled about the successful launch of ESA’s Euclid mission and are eager to see the science it returns,” said Nicola Fox, associate administrator for NASA’s Science Mission Directorate in Washington. “By studying the ‘dark side’ of our universe, Euclid is not only paving the way for NASA’s Roman Space Telescope, it is igniting a new golden age of survey astronomy that will help us understand our universe’s history and structure in ways that were not possible before.”

Illuminating Dark Energy

The Euclid mission could help scientists determine whether our current understanding of gravity needs to be rewritten or if an entirely new mechanism is needed to explain the universe’s accelerating expansion.

Euclid will create a cosmic map that covers almost a third of the sky, charting the location of millions of galaxies and measuring the average spacing between them – one indicator of dark energy’s influence. Because the light from distant objects takes time to reach us, Euclid will observe galaxies as they were when the universe was about 3 billion years old.

By also looking at closer galaxies, the mission will track how dark energy’s effect has changed over time.

Euclid will also study dark energy by mapping the presence of another mysterious cosmic phenomenon called dark matter. Five times more common in the universe than regular matter, dark matter is distributed throughout the cosmos.

While dark matter does not absorb or reflect light, scientists can detect it via its gravitational influence on “regular” matter like stars and galaxies, and its distribution throughout the cosmos is affected by dark energy’s outward push.

Scheduled to launch by May 2027, Roman will study a smaller section of sky than Euclid, but it will provide higher-resolution images of millions of galaxies and peer deeper into the universe’s past, providing complementary information. Roman will also survey nearby galaxies, find and investigate planets throughout our galaxy, study objects on the outskirts of our solar system and more.

Source: Jet Propulsion Laboratory

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Saturday, July 01, 2023

VIPER's Test Model Continues to Go Through the Paces in California's Silicon Valley...

A snapshot of NASA's VIPER lunar rover prototype, known as MGRU3 (Moon Gravitation Representative Unit 3), conducting an egress test at the Ames Research Center in California's Silicon Valley.
NASA / Dominic Hart

NASA’s Moon Rover Prototype Conquers Steep, Scary Lander Exit Test (News Release - June 30)

NASA's VIPER – short for Volatiles Investigating Polar Exploration Rover – recently completed another successful round of rigorous tests of the agency’s first robotic Moon rover’s ability to drive off the Astrobotic Griffin lunar lander and onto the lunar surface. Called an egress, this hours-long operation is one of the most critical and trickiest parts of VIPER's 100-day mission.

It could be even trickier if VIPER’s off-ramps onto the Moon are super steep or tilted due to uneven terrain.

Recent tests using VIPER rover and Griffin lander prototypes conducted at NASA’s Ames Research Center in California’s Silicon Valley were designed to push VIPER’s systems to the limit to ensure that the rover will perform as expected during its science mission. By driving VIPER’s prototype MGRU3 – which stands for the Moon Gravitation Representative Unit 3 – down the lander’s ramps in a series of test configurations in a facility at Ames, engineers came away with a better understanding of how the rover would perform in both normal and unusual scenarios.

Unlike big rigs that deliver cars by rolling them off standardized ramps on trailers, the geometry of the lunar lander’s ramps is designed to vary substantially, depending on what the surface is like when it arrives at its target destination atop the flat-topped lunar mountain Mons Mouton near the Moon’s South Pole. Depending on the terrain around the lander, the angle of the ramps may be especially steep, posing the risk that the rover could lose traction and slip - or one ramp may be steeper than the other, requiring the VIPER real-time operations team to actively compensate for this tricky terrain.

“Through this series, we’ve tested all of the ‘bounding’ cases for VIPER’s egress on the Moon,” said Jasper Wolfe, VIPER egress test lead at Ames. “This included the worst-case high-pitch scenario using the steepest – and scariest – ramps, the worst-case roll scenario using the most uneven ramps, and the worst-case scenario with pitch and roll combined.”

Seen in the photo above is a key moment of the tests, which focused on the physical interface between the rover and the lander. Critical features of the tests included software that specifically handles VIPER’s egress and changes to physical components of both the rover and the lander’s ramps.

The team carefully checked to verify that MGRU3 had adequate clearance and engaged the ramps correctly as it rolled from top to bottom.

“We validated these test cases with MGRU3 to be sure VIPER can do it on the Moon,” said Wolfe.

Completing these tests means that VIPER should be able to successfully exit the lander even if it touches down in a tough spot – a major step forward towards flight.

“With VIPER, we’re doing a lot of firsts,” said Wolfe. “And it’s very exciting to reach this milestone.”

Source: NASA.Gov