Friday, October 23, 2026

The Latest Update on America's Next Saturn-bound Robotic Explorer...

A screenshot from the 'first flight' simulation of NASA's Dragonfly rotorcraft.
NASA / Johns Hopkins APL

NASA’s Dragonfly Completes First Simulated Flight (News Release)

Separated from its protective backshell, NASA’s Dragonfly rotorcraft autonomously speeds over the sand dunes of Titan. It scans the terrain below, searching for a safe place to land. When Dragonfly discovers a safe site, it turns, descends and lands at the selected location, touching down for the first time on the surface of Saturn’s largest moon.

A successful first flight – except, this wasn’t happening on Titan itself, but on a computer testbed at the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland, where the Dragonfly rotorcraft is undergoing integration and testing. It was the most comprehensive test to date of Dragonfly’s “first flight” in real time on flight-like avionics, incorporating most of the systems and maneuvers that the rotorcraft will employ when it arrives at Titan in 2034.

Dragonfly is scheduled to launch no earlier than 2028 for a six-year voyage to Saturn’s moon Titan, where it will spend three years flying from location to location to explore a range of sites to study the chemistry, geology and atmosphere of the Earthlike moon and ultimately advance our understanding of life’s chemical origins.

“The cool thing about first flight is that it’s our most challenging flight,” said Zach Putnam, Dragonfly mobility subsystem lead engineer at APL. “It uses every piece of flight sensor hardware on the lander.”

The recent test brought together flight software and avionics with simulated data input from the sensors that Dragonfly will use at Titan, including its newly-installed navigation cameras, inertial measurement units, and lidar system.

It was a milestone years in the making. The team has built Dragonfly’s flight capabilities incrementally, beginning with simulations of relatively simple activities such as the spinning of a single rotor. Later tests demonstrated a short “reposition” flight and a partial scouting flight, adding more sensors and capabilities at each step.

“Doing it incrementally is what enabled us to build these tests at all,” said Putnam. Adding lidar — the system that Dragonfly will use to measure terrain altitude and slope and identify potential hazards — provided the final piece needed to fully simulate what the rotorcraft will encounter on Titan.

The team generated simulated terrain for the lidar and created, in real time, the images that Dragonfly’s navigation cameras would see. A custom camera emulator used graphics processing units to render each simulated Titan scene in roughly the same 20 to 70 milliseconds exposure times that Dragonfly’s cameras will use during flight.

Running the complete sequence on flight-like hardware gave the team an important opportunity to see how all those pieces interact — including those details measured in milliseconds as information zips between different processes aboard the lander.

“These tests provide an important validation that everything works together,” said Putnam.

And there are many more tests to come. The team plans to run first flight on Dragonfly’s actual flight system, not a testbed, using the rotorcraft’s avionics. Engineers will also test other flight profiles and deliberately introduce faults to make sure that Dragonfly can respond autonomously if something goes wrong.

“That autonomy is essential at Titan, where Dragonfly will have to fly without real-time help from Earth,” Putnam said. “Everything we do on Titan has to happen autonomously.”

Striking a pose

Before Dragonfly can make that first flight on Titan, it has to shift into position to be able to fly. Testing is also underway to ensure that the mechanisms handling that critical step will lower the rotorcraft below the entry system’s backshell, where it can safely start its rotors prior to separation from the entry system and begin its final descent to Titan’s surface.

The test campaign evaluates Dragonfly’s “pose” mechanism, the system that will lower the rotorcraft from its stowed position inside the backshell into position for release during the descent at Titan. Engineers at Lockheed Martin in Colorado – where the elements of Dragonfly’s interplanetary cruise stage and atmospheric entry, descent and landing assembly are coming together – recently conducted static tests with representative mass, pushing and pulling on the mechanism to verify that it can withstand expected loads, as well as deployment tests to see how smoothly and quickly the system lowers, and whether it locks securely into place.

The tests also consider how Dragonfly’s backshell may swing beneath its parachute when the rotorcraft is deployed. Engineers tilt the test hardware to different angles and repeat the deployment to confirm that the mechanism performs properly across a range of conditions.

The pose structure connects the backshell to an aluminum interface structure that attaches to the Dragonfly lander. During the actual descent, the pose mechanism will lower that interface — and Dragonfly with it — before the rotorcraft separates and begins flying under its own power. The testing is designed to make sure that this critical transition works reliably before Dragonfly has to ever perform it nearly a billion miles from Earth.

Source: NASA.Gov

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Technician Emory Toomey installs one of two navigation cameras onto NASA's Dragonfly rotorcraft inside a clean room at the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland...on August 19, 2026.
NASA / Johns Hopkins APL / Ed Whitman

At Lockheed Martin's facility in Denver, Colorado, engineers monitor a test of the 'pose' mechanism for Dragonfly — the system that will lower NASA's rotorcraft from its stowed configuration inside the backshell into position for release during descent at Saturn's moon Titan.
Lockheed Martin

Thursday, October 22, 2026

The Latest Status Update on America's Newest Great Observatory...

An artist's concept of NASA's Nancy Grace Roman Space Telescope surveying the cosmos.
NASA

NASA’s Roman Space Telescope Enters Final Commissioning Phase (News Release)

NASA’s Nancy Grace Roman Space Telescope mission has now entered the science commissioning phase, having successfully completed a comprehensive checkout and refinement of the observatory and primary instrument performance.

“We’ve established that the observatory is fully functional,” said Julie McEnery, Roman’s senior project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “The telescope can guide and take exposures, data flows appropriately, and we can slew from one place to another for observations. So now we’re drilling into the fine details of the quality of the images we’re collecting.”

Thus far, the commissioning process is going smoothly, and the observatory has already undergone several challenging activities. For example, scientists thought Roman might have difficulty observing places that are chock full of stars, or nebulae that are shrouded by dense dust.

“The way Roman locks onto a target is by holding steady on individual stars found in the direction it needs to point,” said Tom Barclay, Roman operations project scientist at NASA Goddard. “We had a concern that in regions where stars are either packed extremely close together or embedded in thick dust, the fine guidance system might get confused or have trouble staying tethered to those stars. But test observations of such regions have shown that Roman performs wonderfully in all cases.”

Roman’s observing requirements are extraordinarily stringent. Multiple factors can influence the consistency of a telescope’s images. If some images were blurrier or brighter than others, it would be difficult to determine whether cosmic objects were truly changing or just appeared to differ because of effects intrinsic to the telescope.

“To achieve the groundbreaking science we expect from Roman, we need to have a crystal clear window into space, not one marred by pointing jitter or out-of-focus images,” said Josh Schlieder, Roman’s Wide Field Instrument scientist at NASA Goddard. “Any imperfections that affect image quality must be minimized because even very small flaws could mask the small signals we are aiming to measure.”

Now, the team is performing a series of carefully-planned test observations that will allow them to characterize observatory performance, calibrate how the instruments respond to light, and refine the telescope’s image quality before transitioning to science operations. The mission’s initial test observations have gone so well that the team is beginning to experience Roman’s superpower: speed.

“During commissioning, we are taking several test observations of famous parts of the sky,” said Jeremy Perkins, an astrophysicist serving as Roman’s observatory integration and test scientist at NASA Goddard. “I am marveling at the level of detail Roman provides in very short time periods.”

Fast survey speeds translate to enormous cosmic vistas, each packed with planets, stars and galaxies galore. Large mosaics that used to be reserved for special occasions will soon become routine, and rare sightings will become customary.

“In a typical observation with Roman’s Wide Field Instrument, we’ll see objects that are a hundred million times fainter than the human eye can detect,” Schlieder said. “So just imagine what strange and unexpected things might be buried in all that data.”

Fine-tuning Roman’s image detail during science commissioning will help scientists more fully understand what to expect. Since some of the observatory’s systems are performing even better than required, it could open up new scientific capabilities, adding even more to the data deluge that the mission will return.

Source: NASA.Gov

Monday, October 19, 2026

Photos of the Day: 'Real Nikki' Finally Met 'Roaming Nikki' Near Hollywood This Past Weekend!

The actress who portrays Nikki Freeman at Halloween Horror Nights poses with OBSESSION's real Nikki, Inde Navarrette, at Universal Studios near Hollywood...on October 18, 2026.
Hamilton Pytluk / Universal Studios Hollywood

Just thought I'd share these cool pictures of Obsession star Inde Navarrette finally coming face-to-face with the actress who plays Nikki Freeman—Navarrette's character in Curry Barker's hit horror film—at Universal Studios' Halloween Horror Nights (HHN) near Hollywood yesterday.

Seeing as how Navarrette should be heading to New York City pretty soon to prepare for her hosting debut on NBC's Saturday Night Live on October 31st, I was wondering if she'd ever visit "Roaming Nikki" at HHN (there are no haunted houses at the annual event that's dedicated to Obsession this year, so Nikki just roams around the theme park interacting with guests and scaring them). Inde visiting the scare actress who plays Nikki was an awesome gesture...considering the online controversy that ensued last month when it was revealed that Obsession's 'final girl' was going to be featured at HHN.

Anyways, Curry Barker himself visited Roaming Nikki at HHN almost a month ago. See the video of the encounter at the bottom of this Blog entry!

Another photo of the actress who portrays Nikki Freeman at Halloween Horror Nights posing with Inde Navarrette at Universal Studios near Hollywood...on October 18, 2026.
Hamilton Pytluk / Universal Studios Hollywood

Tuesday, October 13, 2026

The Latest Update on the Lunar Lander Built by Voyager Technologies (Formerly Astrobotic)...

Voyager Technologies' Griffin-1 Moon lander underwent vibration testing at NASA's Jet Propulsion Laboratory in Southern California last month.
Voyager Technologies

Voyager’s Griffin-1 On Track for the Moon (News Release)

Griffin-1 completes acceptance testing, passing major milestone ahead of lunar launch

DENVER--(BUSINESS WIRE)--Voyager Technologies (NYSE: VOYG) announced that Griffin Mission One (Griffin-1), the company’s infrastructure-class lunar lander, successfully completed acceptance testing, a critical milestone on the path to its targeted launch to the Moon in late 2026.

“Griffin-1 marks a turning point for commercial lunar infrastructure,” said Dylan Taylor, Chairman and CEO, Voyager. “We are an enabler in building the transportation layer for the lunar economy: the logistics, access and systems that make sustained operations on the Moon possible. When Griffin touches down, it will be the largest commercial payload delivery in lunar history. The team has put years of work into this mission, and we are focused on getting Griffin to the Moon and putting that capability to work.”

Acceptance testing verified Griffin-1’s systems performance and confirmed the spacecraft’s readiness for the next phase of launch preparation. The mission will carry 10 payloads from six countries to the lunar South Pole, including payloads from NASA, the European Space Agency and other commercial partners.

Griffin-1 is now returning to Voyager’s Lunar Systems headquarters in Pittsburgh, where the team will complete final preparations ahead of shipment to Cape Canaveral, Florida for launch.

“Completing integration and environmental testing on a mission this complex reflects the quality and discipline of the team,” said John Thornton, executive vice president, Voyager. “Every payload on Griffin’s manifest represents a customer and a capability, and each contributes to the operational knowledge base we need to make the Moon a place where people can reliably live and work. That’s the foundation we’re here to deliver.”

Griffin‑1 was developed through NASA’s Commercial Lunar Payload Services initiative and will now be part of Moon Base Phase I objectives. The lander is designed to support a range of future lunar operations, including the delivery of rovers, science instruments and other infrastructure. Its capabilities are intended to help lay the groundwork for future lunar infrastructure, including power systems that can advance the knowledge, technologies and capabilities needed to develop an enduring human presence on the Moon.

Source: Business Wire

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Voyager Technologies' Griffin-1 Moon lander underwent testing inside a thermal vacuum chamber at NASA's Jet Propulsion Laboratory in Southern California.
NASA / JPL

Voyager Technologies' Griffin-1 Moon lander underwent spin testing at NASA's Jet Propulsion Laboratory in Southern California.
NASA / JPL

Astrolab's FLIP rover, with Voyager Technologies' Griffin-1 Moon lander in the background, at NASA's Jet Propulson Laboratory in Southern California.
Astrolab

Sunday, October 11, 2026

Photos of the Day: Bear's Work Uniform...

The shirt worn by Bear (Michael Johnston) at his job inside Cassell's Music store in OBSESSION...on display (along with a One Wish Willow) at the FocusFest film festival on October 10, 2026.
Richard T. Par

Just thought I'd share this picture that I took of the shirt worn by Bear (Michael Johnston) at the Cassell's Music store in Obsession! This costume piece and a One Wish Willow were on display at the FocusFest film festival that I attended at the Universal Studios backlot near Hollywood yesterday.

This is the second wardrobe from Curry Barker's hit film that I saw in person over the past month; the other one being the black sundress that Nikki (Inde Navarrette) wore in the movie's climax. That outfit was on display inside of the Universal Cinema AMC theater at Universal CityWalk.

Nikki (Inde Navarrette) and Bear (Michael Johnston) stare at Nikki's phone while on the job at the Cassell's Music store in OBSESSION.

Wednesday, September 30, 2026

The Latest Update on America's Newest Space Telescope...

An artist's concept of NASA's Nancy Grace Roman Space Telescope surveying the cosmos.
NASA

NASA Checks Roman Guidance System, Takes First Coronagraph Observation (News Release)

NASA’s Nancy Grace Roman Space Telescope’s fine-guidance system, which allows the observatory to lock very steadily onto its targets during observations, passed a spate of tests from September 15 to 21. Then on September 22, the mission’s Coronagraph Instrument opened its eyes to cosmic light for the very first time.

The team assigned a small part of each of the 18 detectors in Roman’s primary instrument, the Wide Field Instrument, to rapidly observe a separate guide star — stars with well-known positions used as reference points. When Roman’s attitude control system gets the spacecraft pointed in the right direction, information from the fine-guidance system then helps hold it steady throughout each observation so that it doesn’t drift off target. Using only the attitude control system, Roman’s images wouldn’t be as crisp.

“Every Roman observation relies on its ability to stay precisely pointed at the correct region of space long enough to collect an image, which can take from minutes to hours for a deep exposure,” said Begoña Vila, Roman’s guiding instrument systems lead at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “The fine-guidance system reports the positions of the guide stars about four times each second to the attitude control system, which can move the observatory a tiny amount to counter any drift as needed. Our tests confirmed that we are able to keep the observatory very stable for science operations: better than 1/100,000 of a degree for half an hour at a time for Wide Field Instrument observations or for eight hours at a time for Coronagraph Instrument observations, which take much longer. This was a very exciting moment for the team.”

Roman’s current stability is roughly equivalent to focusing a laser beam on a U.S. dime from about 150 miles (about 240 kilometers) away. The team aims to improve this even further by tuning the guidance system, boosting the distance in the analogy to about 230 miles (370 kilometers).

Roman also has a new type of guiding that hasn’t been attempted before.

“Roman doesn’t have a separate guider instrument, like other space telescopes do,” Vila said. “Instead of tracking only a star’s point-like appearance, it will guide on detailed wavelength patterns called spectra. Because Roman is already equipped to measure spectra for science, it can use that same information to precisely position the telescope. We are looking forward to validating this spectral guiding mode in the coming weeks.”

Coronagraph captures first glimmer

Next, on September 22 and 27, the team tested out the fine-guidance system with the Coronagraph Instrument, which will demonstrate cutting-edge technology to block starlight and view planets and dusty disks around nearby stars.

“Roman’s coronagraph also has its own internal stability process, making it much more stable even than the Wide Field Instrument,” Vila said. That’s critical because even tiny vibrations or pointing errors could let starlight leak through, washing out the faint planets that scientists are trying to see.

The coronagraph woke up on September 1 and stretched its digital, electronic and mechanical “limbs” mid-month. Once the team confirmed that the fine-guidance system was holding the Coronagraph Instrument steady, scientists adjusted the focus so it could take its first bleary-eyed look at space that will help scientists fine-tune the instrument’s view.

“This observation confirms that the instrument can produce a focused image,” said Vanessa Bailey, a Roman Coronagraph Instrument scientist at NASA’s Jet Propulsion Laboratory in Southern California. “It’s a very limited test that kicks off a methodical process of increasingly complex tasks that help us prepare for the instrument’s future observations.”

For this step, the Coronagraph Instrument captured a faint star in a neighboring galaxy called the Large Magellanic Cloud, with “noise” seeping through because the detectors have been kept at a warmer temperature than they will ultimately operate. That helps to ensure contamination does not stick to the detectors.

“We were kicking the tires, making sure light goes through the system,” Bailey said. “The second step, on Sunday, was an observation that confirmed our pointing. The team cooled the detectors down for better sensitivity, and we observed a new location in the Large Magellanic Cloud where we expected to see many stars in a single image. And we did! We’re breathing a sigh of relief!”

Source: NASA.Gov

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Inside the Roman Coronagraph Commanding Center at Caltech's IPAC in Southern California, two coronagraph operators monitor telemetry and wait for data from the first observation by the Roman Space Telescope's Coronagraph Instrument.
Caltech / IPAC – SELab / Isabel Swafford

Tuesday, September 29, 2026

Launch the Proposed Interstellar Probe on this Rocket, NASA!

An artist's concept of Blue Origin's New Glenn 9x4 rocket lifting off from Launch Complex 36 at Cape Canaveral Space Force Station in Florida.
Blue Origin

NASA Adds Blue Origin New Glenn 9×4 to Launch Services Contract (News Release)

In accordance with a contract on-ramp clause, NASA has added Blue Origin’s New Glenn 9×4 launch service to the NASA Launch Services (NLS) II contract. The New Glenn 9×4 launch service will be available to NASA’s Launch Services Program Office to use for future missions.

The NLS II contracts are multiple-award, indefinite-delivery/indefinite-quantity contracts with an ordering period through June 2030, and an overall period of performance through December 2032. The NLS II contracts include an on-ramp provision that provides an opportunity annually for new launch service providers to compete for future missions and allows existing contractors to introduce launch vehicles not currently on their NLS II contracts.

The NLS II contracts support the goals and objectives of the agency’s Human Spaceflight Mission Directorate, Science Mission Directorate, and the Research and Technology Mission Directorate. Under the contract, NASA can also provide launch services to other government agencies, such as the National Oceanic and Atmospheric Administration.

Source: NASA.Gov

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An infographic showing the various science instruments that would fly on a proposed Interstellar Probe spacecraft.
Johns Hopkins University Applied Physics Laboratory

Saturday, September 26, 2026

Photos of the Day: Meeting Harry, the Novelty Shop Guy in OBSESSION...

Posing with OBSESSION cast member Darin Toonder and his autograph at The Cathedral in downtown Pomona...on September 19, 2026.

"Yea yea yea, you made a shitty wish and now you wanna reverse it. But you can't come in here with this energy, man!"

So a week ago today, I met Darin Toonder...who played Harry, the laid-back novelty shop clerk who gave Bear (Michael Johnston) grief for coming into the store—Spoiler Ahead—completely wrecked by the death of Sarah (Megan Lawless) at the hands of Nikki (Inde Navarrette) in Obsession. He's a really cool guy in person!

Toonder's photo op and autograph signing took place at the Goth Mall event inside The Cathedral in downtown Pomona, which is only around 2 miles from where I live. Imagine how stoked I would be if Navarrette, Lawless, Johnston, Cooper Tomlinson (who played Ian) and/or writer-director Curry Barker made an appearance in my neck of the woods as well! Happy Saturday.

My autograph by OBSESSION cast member Darin Toonder.

Friday, September 25, 2026

The Latest Status on America's Newest Great Observatory...

An artist's concept of NASA's Nancy Grace Roman Space Telescope surveying the cosmos.
NASA

NASA’s Roman Team Confirms Ground Stations Receiving Data (News Release)

NASA has now confirmed that all ground stations supporting the agency’s Nancy Grace Roman Space Telescope are ready to receive the mission’s high volume of data once science operations begin by early 2027.

Observing the far reaches of the cosmos wouldn’t be possible without a network of ground stations strategically located around the world serving as a tether between Earth and space. Ground stations from NASA’s Near Space Network in New Mexico, ESA (European Space Agency) in Australia, and JAXA (Japan Aerospace Exploration Agency) in Japan will receive the science data at extremely high data rates, up to 500 megabits per second.

Recent testing ensured that these stations will be able to receive approximately 1.4 terabytes of data that Roman will downlink each day, the highest rate of any NASA astrophysics mission so far, from Roman’s location a million miles away in space.

To confirm this capacity, scientists began drawing down “housekeeping” information.

“This is real, operational data starting with details about how the instruments are doing, things like temperature, power draw, and preliminary image data,” said Bob Kalogerakos, a radio frequency engineer at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.

The Roman team started with JAXA’s Misasa Deep Space Station in Saku City on September 7. Engineers tested out the station’s antenna and confirmed that it can receive data at rates up to 500 megabits per second throughout most of the year. The rate will vary with Roman’s distance from and elevation relative to Earth as it orbits the Lagrange point 2, or L2.

“This was our first time downlinking data at Roman’s maximum rate,” said Matthew Wasiak, an advanced systems engineer at NASA Goddard. “There was also a typhoon in Japan during the test and conditions were not perfect, which makes this a particularly rigorous test.”

Adverse weather can create a major obstacle for drawing down space telescope data because raindrops are not much smaller than the radio wavelengths Roman is using to send its data. That means they can scatter or weaken the signals.

“Because of this, we have a diversity of ground stations, from the subtropical island of JAXA’s ground station in Japan to the arid Western Australian desert to summer monsoon-prone New Mexico,” Kalogerakos said. “When weather and rain do interfere with our signal, our automated ground systems will determine what data didn’t downlink properly and ask the spacecraft to re-transmit from its onboard solid-state recorder in a few hours.”

After the Misasa Deep Space Station passed the team’s tests, their focus shifted to the Near Space Network ground station and its backup in White Sands, New Mexico, from September 8 to 11. Both antennas successfully downlinked data at the rates the team tested.

Finally, the team tested the ESA station, located near New Norcia in Western Australia, on September 17. Again, engineers cycled through different rates, and the ground system successfully downlinked even the highest.

“These ground stations are Roman’s primary conduit to get our data down to Earth, and the team is thrilled with their exceptional performance,” said Jeremy Perkins, Roman’s observatory integration and test scientist at NASA Goddard. “It’s great news for a mission that will send back data at an incredible pace.”

Bringing Roman’s data to the ground is an international effort. NASA’s Near Space Network ground station in New Mexico receives Roman’s science data in partnership with antennas from ESA in Australia and JAXA in Japan. Managed by NASA’s Jet Propulsion Laboratory in Southern California, the agency’s Deep Space Network stations in California, Spain, and Australia provide critical tracking data, observatory telemetry, and command.

Source: NASA.Gov

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The Near Space Network antennas at NASA's White Sands Complex in Las Cruces, New Mexico.
NASA

Wednesday, September 23, 2026

A New Space-based Observatory Is on the Horizon...

An artist's concept of NASA's PRIMA space telescope.
NASA

NASA Selects Far-Infrared Telescope as First in New Mission Class (News Release)

NASA announced on Wednesday that a mission to explore the history and evolution of the Universe, PRIMA (PRobe far-Infrared Mission for Astrophysics), is advancing to the next phase of development. This space telescope is the first in a new class of NASA astrophysics missions, called Probe Explorers, within the agency’s longstanding Explorers Program.

“The PRIMA mission is humanity’s next window into the deep Universe. It will unveil the obscure across cosmic time to better understand the formation of planets, stars, black holes, and even how water on Earth came to be,” said Nicky Fox, associate administrator, Science Mission Directorate, NASA Headquarters in Washington.

NASA selected PRIMA to move into Phase B, the stage of development that advances the preliminary design and technology development for the mission. The mission is subject to a confirmation review, based on technical, programmatic, and cost performance, to determine its readiness to begin implementation in Phase C. If confirmed, PRIMA’s project cost is capped at $1.2 billion, not including launch and other non-project costs.

The observatory will be targeted to launch in 2033, for a planned five-year mission.

With a 5.9-foot telescope, PRIMA will conduct deep, sensitive surveys of the Universe in far-infrared light, helping bridge the gap between existing infrared observatories, such as NASA’s James Webb Space Telescope, and radio telescopes. By studying radiant energy that only emerges in the far-infrared, PRIMA will address a wide range of questions about the Universe. This includes the origins of planets outside our Solar System, how galaxies and their black holes have grown and evolved over cosmic history, and how dust and heavy elements have built up in the Universe over time – all helping paint a better picture of why the Universe looks the way it does today.

“A single mission alone can’t probe all the Universe’s mysteries. But by extending the survey capabilities of our fleet into far-infrared wavelengths with PRIMA, we’re enabling an incredibly comprehensive look at the cosmos,” said Shawn Domagal-Goldman, director, Astrophysics Division, NASA Headquarters. “With our Webb and Roman space telescopes, we set a cadence of launching premiere-class missions in both halves of the decade. We’re going to keep that up and kick off the next decade with PRIMA, as part of a pipeline that will consistently have missions of this caliber ready to go.”

The National Academies of Sciences, Engineering, and Medicine’s 2020 Decadal Survey, Pathways to Discovery in Astronomy and Astrophysics for the 2020s, recommended that NASA establish this new Probe Explorers mission class. NASA selected PRIMA for development after detailed evaluation of concept studies for Probe Explorer missions, based on their scientific merit in alignment with the Decadal Survey’s recommendations, feasibility of their development plans on cost and schedule, and use of technologies that could support the development of future large missions.

NASA’s Jet Propulsion Laboratory in Southern California will manage the PRIMA mission. Other partners include NASA’s Goddard Space Flight Center in Greenbelt, Maryland and NASA’s Marshall Space Flight Center in Huntsville, Alabama. The PRIMA mission will also have contributions from international partners: CNES (Centre National D’Etudes Spatiales), ASI (Agenzia Spaziale Italiana), DLR (Deutsches Zentrum für Luft- und Raumfahrt), CSA (Canadian Space Agency), KASI (Korea Astronomy and Space Science Institute)/KASA (Korea AeroSpace Administration), JAXA (Japan Aerospace Exploration Agency), and the UK Space Agency.

The Explorers Program is the oldest continuous NASA program designed to provide frequent, low-cost access to space using principal investigator-led space science investigations relevant to the Science Mission Directorate’s astrophysics and heliophysics programs. Since the Explorer 1 launch in 1958, which discovered Earth’s radiation belts, the Explorers Program has launched more than 100 missions, including the Uhuru and Cosmic Background Explorer missions that led to Nobel prizes for their investigators.

The Explorers Program is managed by NASA Goddard for the Science Mission Directorate, which conducts a wide variety of research and scientific exploration programs for Earth studies, space weather, the Solar System, and the Universe.

Source: NASA.Gov