Saturday, October 31, 2026

Fly Aboard America's Next Saturn-bound Robotic Explorer!

Fly your name aboard NASA's Dragonfly rotorcraft...which launches to Titan in July 2028 and arrives at Saturn's moon in late 2034. The deadline is January 15, 2027.
NASA / Johns Hopkins APL

Send Your Name to Titan Aboard NASA’s Dragonfly Mission (News Release - October 29)

You may never soar under the clouds or over the organic sands of Saturn’s moon Titan, but your name can. NASA is inviting the public to send their names aboard the agency’s Dragonfly rotorcraft and be part of the first science mission to fly and explore the surface of another world.

To have your name included on a microchip aboard Dragonfly and receive a personalized digital boarding pass commemorating your place on this historic mission, visit:

https://go.nasa.gov/dragonfly-names

“NASA’s Dragonfly mission will simply blow your mind,” said Nicky Fox, associate administrator, Science Mission Directorate, NASA Headquarters in Washington. “By flying the first-ever rotorcraft science mission, NASA will explore Saturn’s largest moon, Titan, as we search for signs of habitability on a distant world that is most similar to our own. We are excited to bring humanity along for the journey of a lifetime, and we invite everyone to send their names on this small, but mighty rotorcraft that will unlock the secrets of the Universe in what is widely considered one of the most exciting space missions of our lifetime.”

The public can secure a place on Dragonfly’s passenger list until 11:59 p.m. EST January 15, 2027.

The Dragonfly rotorcraft is currently being assembled at the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland. Scheduled to launch in 2028, the rotorcraft will travel to Titan, a remarkable world with a thick atmosphere, rivers and lakes of liquid methane, sweeping dunes, and a landscape rich in organic material. After arriving in 2034, Dragonfly will fly to different locations on the moon, exploring Titan’s diverse environments and searching for clues about prebiotic chemistry — the chemistry that came before biology — to help scientists better understand the ingredients and conditions for life.

Dragonfly is being designed and built under the direction of APL, which leads the mission for NASA. Elizabeth Turtle of APL is the principal investigator. Dragonfly is the fourth 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.

Source: NASA.Gov

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My 'boarding pass' for NASA's Dragonfly mission.

Thursday, October 29, 2026

The Latest Update on Humanity's Most-Distant Interstellar Probe...

An artist's concept of a Voyager probe traveling through deep space.
Caltech / NASA - JPL

NASA’s Voyager 1 Conserves Power, Resolves Brief Communications Pause (News Release)

NASA’s Voyager team is celebrating two recent developments with the Voyager 1 spacecraft: In September, they successfully completed a months-long effort to stretch the spacecraft’s diminishing power supply. Then, on October 20, an unexpected loss of communication with the spacecraft resolved itself after 48 hours, before the team sent commands to the spacecraft to troubleshoot the issue.

In early September, engineers successfully turned off three devices on the Voyager 1 spacecraft and substituted them with three lower-power alternatives. Nicknamed the “Big Bang,” the energy-saving effort was completed about six weeks after the mission team performed the same swap on Voyager 2. The Big Bang will enable Voyager 1’s remaining science instruments to operate longer than previously anticipated.

The Voyagers get their power from radioisotope thermoelectric generators, which convert heat from decaying plutonium into electricity. With the plutonium supply continually depleting, both probes lose about 4 watts of power each year. Almost a half-century since Voyager launched, the spacecraft power margins have grown thin, requiring the team to conserve energy by shutting off nonessential devices and systems.

The Big Bang was unique because it required the swaps to occur simultaneously. The six devices help keep the spacecraft warm enough to operate in the frigid expanse of space, and only by swapping all three could the team both reduce the amount of power Voyager 1 uses and ensure that heat is properly distributed on the spacecraft.

In recent years, the dwindling power supply has forced the team to turn off two science instruments. The mission launched in 1977 with 10 dedicated science instruments, some of which were turned off after the spacecraft’s planetary encounters. Some instruments were left on to study the outer region of the heliosphere, a bubble of particles and magnetic fields created by the Sun.

Now, the Voyagers are traveling through interstellar space, the area outside the heliosphere, and are the only spacecraft to ever study this region directly. Without performing the Big Bang, the mission would have needed to turn off another instrument on Voyager 1 as early as summer 2027.

Brief signal loss

But between now and summer 2027, the team is at the ready for more surprises like the one that they recently encountered when they briefly lost contact with Voyager 1 on October 18 and 19. NASA’s Deep Space Network — large antennas at three facilities around the globe used to communicate with spacecraft at the Moon and beyond — was unable to detect a radio signal from the probe, which is 16 billion miles (24 billion kilometers) from Earth, during two scheduled communications attempts, 24 hours apart. The spacecraft’s signal reappeared 24 hours later, on October 20, and the team has maintained communication with it since then.

Engineers are still investigating what caused the communication loss. The team has so far determined that one group of thrusters went offline and their backups turned on. Such a swap is programmed to occur automatically if the spacecraft's computers detect something amiss with the active thrusters. This automatic response is known as fault protection and directs the spacecraft to put itself in a safe, or stable, configuration and pause normal operations, giving engineers time to diagnose the issue and take action.

“This is the first time we’ve seen the spacecraft do something like this, but we are also at a point in the mission where we have to expect the unexpected,” said Kareem Badaruddin, Voyager mission manager at NASA’s Jet Propulsion Laboratory in Southern California. “We’re relieved to be back in contact with Voyager 1 and are eager to understand what happened.”

Historic milestone

As the investigation continues, Voyager 1 is speeding at 38,000 mph (61,155 kph) towards a major milestone: On November 18, the spacecraft that has traveled farther than any other human-made object will be 16.09 billion miles (25.89 billion kilometers) from Earth — the equivalent of one light-day, or the distance that light can travel in one day. That means that the radio waves used to communicate with the probe take 24 hours to reach it, and the radio waves carrying the spacecraft’s return message take another 24 hours.

“If you want to say ‘hello’ to Voyager, you send your message and then you go home and you wait two days before you finally get a response,” said Suzanne Dodd, Voyager project manager at JPL.

The spacecraft will not detect any change in its environment when it passes one light-day, nor will anything change aboard the spacecraft. The milestone’s significance is in its demonstration of the vastness of the Universe and the endurance of humanity’s most distant explorer.

Source: NASA.Gov

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

Wednesday, October 21, 2026

The Latest Update on Japan's Newly-Launched Mission to Phobos...

An artist's concept of JAXA's MMX spacecraft approaching the Martian moon Phobos.
JAXA

Completion of the Initial Critical Operations Phase of the Martian Moons eXploration (MMX) Spacecraft (News Release)

Today, on October 21, the Japan Aerospace Exploration Agency (JAXA) confirmed that the critical sequence during the initial operations of the Martian Moons eXploration (MMX) spacecraft, which launched on October 20, was successfully completed and that the spacecraft is in good health. This marks the completion of the initial critical operations phase - the period following the spacecraft’s separation from the launch vehicle until the completion of a series of operations to establish spacecraft health, including deployment of the solar array paddles, establishment of three-axis attitude control, and release of the medium-gain antenna (MGA) hold-down mechanism.

JAXA will now conduct initial functional checks of the spacecraft’s onboard equipment while preparing for the outbound cruise operations phase towards the Martian system.

JAXA expresses its deepest gratitude to all those who provided cooperation and support for the launch, tracking and control of the MMX spacecraft.

Source: Japan Aerospace Exploration Agency

Tuesday, October 20, 2026

An Interplanetary Mission Led by Japan Is on its Way to Phobos!

An H3-24L rocket carrying JAXA's Martian Moons eXploration (MMX) spacecraft launches from Tanegashima Space Center in Japan...on October 20, 2026 (Japan Time).
JAXA

Launch Result of the Martian Moons eXploration (MMX) Spacecraft aboard H3 Launch Vehicle Flight No.10 (News Release)

The Japan Aerospace Exploration Agency (JAXA) launched the Martian Moons eXploration (MMX) spacecraft aboard H3 Launch Vehicle flight No.10 at 04:41:03 JST on October 20, 2026 from the Tanegashima Space Center.

The H3 Launch Vehicle flew as planned, and approximately 71 minutes and 13 seconds after liftoff, the separation of the MMX spacecraft was confirmed. The MMX spacecraft was then injected into the predetermined orbit.

JAXA would like to express sincere gratitude for your support.

Source: Japan Aerospace Exploration Agency

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An image of the Idefix rover, developed by CNES (French National Centre for Space Studies) and DLR (German Aerospace Center), before it was attached to JAXA's MMX spacecraft for launch.
JAXA

A technician attaches an SD memory card carrying the names and messages of 5,000 people onto the Idefix rover after it was mated to JAXA's MMX spacecraft for launch.
JAXA

Two technicians pose with a sign commemorating the installation of the SD memory card carrying 5,000 names and messages onto the Idefix rover.
JAXA

An image of JAXA's MMX spacecraft as it underwent preparations for launch.
JAXA

A technician poses with the H3-24L payload fairing that housed JAXA's MMX spacecraft for launch.
JAXA

In the distance, the H3-24L rocket carrying JAXA's MMX spacecraft stands tall on the launch pad at Tanegashima Space Center in Japan...on October 19, 2026 (Japan Time).
JAXA

The H3-24L rocket carrying JAXA's MMX spacecraft launches from Tanegashima Space Center in Japan...on October 20, 2026 (Japan Time).
JAXA

An artist's concept of JAXA's MMX spacecraft approaching the Martian moon Phobos.
JAXA

An artist's concept of the Idefix rover on the surface of Phobos.

My participation certificate for JAXA's MMX mission.

My late Mom's participation certificate for JAXA's MMX mission.

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