NASA Invites Public to Share in Excitement of PACE Mission Launch

NASA Invites Public to Share in Excitement of PACE Mission Launch

NASA and SpaceX technicians safely encapsulate NASA’s PACE (Plankton, Aerosol, Cloud, ocean Ecosystem) spacecraft in SpaceX’s Falcon 9 payload fairings on Tuesday, Jan. 30, 2024.
NASA and SpaceX technicians safely encapsulate NASA’s PACE (Plankton, Aerosol, Cloud, ocean Ecosystem) spacecraft in SpaceX’s Falcon 9 payload fairings on Tuesday, Jan. 30, 2024, at the Astrotech Space Operations Facility near the agency’s Kennedy Space Center in Florida.
Photo Credit: NASA Goddard/Denny Henry

NASA is hosting virtual activities ahead of the launch of the PACE (Plankton, Aerosol, Cloud, ocean Ecosystem) mission and invites you to share in the fun. The PACE mission will help us better understand how the ocean and atmosphere exchange carbon dioxide, measure key atmospheric variables associated with air quality and Earth’s climate, and monitor ocean health, in part by studying phytoplankton, tiny plants and algae that sustain the marine food web. PACE will extend and expand NASA’s long-term observations of our living planet. By doing so, it will take Earth’s pulse in new ways for decades to come.

NASA’s PACE is scheduled to launch no earlier than 1:33 a.m. EST, Tuesday, Feb. 6, on a SpaceX Falcon 9 rocket from Space Launch Complex 40 at Cape Canaveral Space Force Station in Florida.

Members of the public can register to attend the launch virtually. As a virtual guest, you have access to curated resources, schedule changes, and mission-specific information delivered straight to your inbox. Following each activity, virtual guests will receive a commemorative stamp for their virtual guest passport.

Live launch coverage will begin at 12:45 a.m., Feb. 6, on NASA+, NASA Television, and the agency’s website. For more information about the PACE mission, visit: https://pace.oceansciences.org/.

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Elyna N. Niles-Carnes

UNITE All-Nighter Delights Amateur Astronomers

UNITE All-Nighter Delights Amateur Astronomers

2 min read

UNITE All-Nighter Delights Amateur Astronomers

A father and his daughter smile as they pose for a photo next to a large telescope with the sky darkening in the background.
Fadi Saibi and his daughter Sophie, age 14, pose for a photograph with their Unistellar telescope in their backyard in Sunnyvale, Calif., on Thursday, Jan. 11, 2024.
Credit: Bay Area News Group/Nhat V. Meye

Maybe you read about them in the papers–amateur astronomers in Japan, Russia, France, Finland, and the United States have been pulling all-nighters to spot extraordinary exoplanets, planets orbiting stars other than the Sun. 

NASA’s UNITE project holds these planetary stakeouts several times every month, and you can join in!

This October, the UNITE team undertook a 20-hour marathon as part of tracking a Saturn-sized planet called TOI-4600 c. They watched and waited, trying to see the planet’s star dim by about 1% as the planet passed in front of it. 

Success would tell us that the planet takes a little more than one Earth year to orbit its star. It would place this planet on a short list of gas-giant planets known outside our own solar system that have sizes and temperatures similar to those of Saturn and Jupiter. Such planets are key laboratories for studying how our solar system was formed, so each new example is precious.

In mid-January, the UNITE team coordinated observations across Europe to catch the third-ever star-crossing event for a different planet. (The third one seen by humans, that is!) Once the team does catch it, they’ll know if it takes three Earth years to orbits its star, which would make it fairly cold planet, or something closer to 100 Earth days, telling us that the planet is relatively warm.

The final results of these observations remain closely-guarded secrets, but they will soon be released in an astronomy journal articles. 

The Unistellar Network Investigating TESS Exoplanets (UNITE) project is a global team of volunteer telescope observers tracking down rare worlds in distant solar systems. Visit science.unistellaroptics.com and you can be part of the next UNITE discovery!

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Feb 02, 2024

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30 Years Ago: STS-60, the First Shuttle-Mir Mission

30 Years Ago: STS-60, the First Shuttle-Mir Mission

On Feb. 3, 1994, space shuttle Discovery took off on its 18th flight, STS-60. Its six-person crew of Commander Charles F. Bolden, Pilot Kenneth S. Reightler, and Mission Specialists N. Jan Davis, Ronald M. Sega, Franklin R. Chang-Díaz, who served as payload commander, and Sergei K. Krikalev of the Russian Space Agency, now Roscosmos, flew the first mission of the Shuttle-Mir Program. Other objectives of the mission included the first flight of the Wake Shield Facility, a free-flying satellite using the ultra-vacuum of space to generate semi-conductor films for advanced electronics and the second flight of a Spacehab commercially developed pressurized module to enable multidisciplinary research and technology demonstrations. The eight-day mission marked an important step forward in international cooperation and the commercial development of space.

The STS-60 crew patch The STS-60 crew of (clockwise from bottom left) Pilot Kenneth S. Reightler, Mission Specialists Franklin R. Chang-Díaz, Ronald M. Sega, Sergei K. Krikalev representing the Russian Space Agency, now Roscosmos, and N. Jan Davis, and Commander Charles F. Bolden The patch for the Phase 1 Shuttle-Mir program
Left: The STS-60 crew patch. Middle: The STS-60 crew of (clockwise from bottom left) Pilot Kenneth S. Reightler, Mission Specialists Franklin R. Chang-Díaz, Ronald M. Sega, Sergei K. Krikalev representing the Russian Space Agency, now Roscosmos, and N. Jan Davis, and Commander Charles F. Bolden. Right: The patch for the Phase 1 Shuttle-Mir program.

In Oct. 1992, NASA announced Bolden, Reightler, Davis, Sega, and Chang-Díaz as the STS-60 crew. For Bolden and Chang-Díaz, STS-60 represented their fourth trips into space; for Bolden the second as commander. Reightler and Davis each had completed one previous spaceflight, with Sega as the sole rookie on the crew. The announcement noted that one of two RSA cosmonauts already in training at NASA’s Johnson Space Center in Houston would join the crew at a later date. In early April 1993, NASA designated Krikalev, a veteran of two long-duration missions aboard the Mir space station, as the prime international crew member, with Vladimir G. Titov named as his backup. The now six-person crew trained extensively for the next nine months for the history-making flight.

Space shuttle Discovery departs the Vehicle Assembly Building on its way to Launch Pad 39A The STS-60 crew departs crew quarters for Launch Pad 39A Liftoff of space shuttle Discovery to begin the STS-60 mission
Left: Space shuttle Discovery departs the Vehicle Assembly Building on its way to Launch Pad 39A. Middle: The STS-60 crew departs crew quarters for Launch Pad 39A. Right: Liftoff of space shuttle Discovery to begin the STS-60 mission.

Discovery landed at NASA’s Kennedy Space Center in Florida after its previous mission, STS-51, on Sept. 22, 1993, where workers towed it to the Orbiter Processing Facility to refurbish it for STS-60. They towed it to the Vehicle Assembly Building on Jan. 4, 1994, for mating with its external tank and twin solid rocket boosters, and rolled the completed stack to Launch Pad 39A six days later. The astronauts participated in the Terminal Countdown Demonstration Test, a rehearsal for the actual countdown, on Jan. 14. Senior managers held the Flight Readiness Review on Jan. 22 to confirm the Feb. 3 launch date. Engineers began the countdown for launch on Jan. 31. Liftoff occurred on schedule at 7:10 a.m. EST on Feb. 3, and Discovery and its six-person crew flew up the U.S. East Coast to achieve a 57-degree inclination orbit.

Discovery’s payload bay, showing the Spacehab module including the externally mounted Sample Return Experiment, and the Canadian-built Remote Manipulator System Astronauts N. Jan Davis, left, and Franklin R. Chang-Díaz open the hatch to the Spacehab module Ronald M. Sega monitors Sergei K. Krikalev as he performs a neurosensory investigation
Left: Discovery’s payload bay, showing the Spacehab module including the externally mounted Sample Return Experiment, and the Canadian-built Remote Manipulator System. Middle: Astronauts N. Jan Davis, left, and Franklin R. Chang-Díaz open the hatch to the Spacehab module. Right: Ronald M. Sega monitors Sergei K. Krikalev as he performs a neurosensory investigation.

Once in orbit, the astronauts opened Discovery’s payload bay doors to begin their activities. Chang-Díaz and Davis opened the hatches to the Spacehab, accessed from the middeck through the airlock and a connecting tunnel, and activated the module’s systems. They began activating some of the 12 experiments in the Spacehab, primarily focused on biotechnology and materials processing. In the middeck, Reightler, Davis, Sega, and Krikalev performed the first session of the joint neurovestibular experiment, which they repeated five more times during the mission. The astronauts also began activating some of the experiments in the shuttle’s middeck.

Charles F. Bolden prepares to take a blood sample from Franklin R. Chang-Díaz for the metabolic experiment Kenneth S. Reightler processes blood samples in the centrifuge Reightler places the processed blood samples in the GN2 freezer
Left: Charles F. Bolden prepares to take a blood sample from Franklin R. Chang-Díaz for the metabolic experiment. Middle: Kenneth S. Reightler processes blood samples in the centrifuge. Right: Reightler places the processed blood samples in the GN2 freezer.

The astronauts began the joint metabolic experiment to investigate biochemical responses to weightlessness on flight day 2. With Bolden and Chang-Díaz serving as phlebotomists, they and Reightler participated as subjects for this study that involved drawing blood samples, spinning them in a centrifuge, and placing them in gaseous nitrogen freezers for return to Earth for analysis.

The Wake Shield Facility (WSF) deployed at the end of the Canadian-built Remote Manipulator System, with the aurora in the background The WSF at the end of the RMS The robotic arm about to stow the Wake Shield Facility
Left: The Wake Shield Facility (WSF) deployed at the end of the Canadian-built Remote Manipulator System, with the aurora in the background. Middle: The WSF at the end of the RMS. Right: The robotic arm about to stow the Wake Shield Facility.

Operations with the wake shield began in flight day three. Davis grappled the WSF (Wake Shield Facility) with the shuttle’s Canadian-built remote manipulator system, or robotic arm, lifting it out of the payload bay, placing it in the “ram clearing” attitude to have atomic oxygen present in low Earth orbit cleanse it of contaminants that could hamper the purity of any produced samples. Plans called for Davis to then release the facility for its two days of free flight. During this process, the astronauts and Mission Control could not properly assess the satellite’s configuration, and troubleshooting efforts led to loss of communications with it. Mission Control instructed the astronauts to berth the facility overnight as ground teams assessed the problem. Engineers traced the problem to a radio frequency interference issue missed due to inadequate preflight testing. The next morning, Davis once again picked up the facility with the robotic arm. The communications issue recurred, but a reboot of the facility’s computer appeared to fix that problem. However, problems cropped up with the satellite’s navigation system, precluding its deployment. All operations and manufacturing occurred with the WSF remaining attached to the robotic arm. Despite this, the facility demonstrated its capabilities by producing five semiconductor films of good quality before Davis berthed it back in the payload bay on flight day seven.

N. Jan Davis takes a peripheral venous pressure measurement on Charles F. Bolden Davis operates a fluid processing apparatus, one of the experiments in the Commercial Generic Bioprocessing Apparatus Bolden operates the Organic Separation experiment
Left: N. Jan Davis takes a peripheral venous pressure measurement on Charles F. Bolden. Middle: Davis operates a fluid processing apparatus, one of the experiments in the Commercial Generic Bioprocessing Apparatus. Right: Bolden operates the Organic Separation experiment.

Meanwhile, the astronauts continued with experiments in the middeck and the Spacehab. Another joint investigation called for the measurement of peripheral venous blood pressure. The Spacehab module contained 12 experiments in the fields of biotechnology, materials processing, and microacceleration environment measurement. A thirteenth experiment mounted on the module’s exterior collected cosmic dust particles on aerogel capture cells.

Ronald M. Sega operates the liquid phase sintering experiment Franklin R. Chang-Díaz operates the Space Experiment Furnace The Stirling Orbiter Refrigerator/Freezer technology demonstration The STS-60 crew enjoys ice cream stored in the freezer
Left: Ronald M. Sega operates the liquid phase sintering experiment. Middle left: Franklin R. Chang-Díaz operates the Space Experiment Furnace. Middle right: The Stirling Orbiter Refrigerator/Freezer technology demonstration. Right: The STS-60 crew enjoys ice cream stored in the freezer.

A technology demonstration on STS-60 involved the test flight of a Stirling Orbiter Refrigerator/Freezer. Planned for use on future missions to store biological samples, on STS-60 the astronauts tested the unit’s ability to chill water containers and provided the crew with a rare treat in space: real ice cream.

In the Mission Control Center, President William J. “Bill” Clinton chats with the STS-60 crew during his visit to NASA’s Johnson Space Center The Mir crew and the STS-60 crew talk with each other through the communications link established during the ABC program Good Morning America
Left: In the Mission Control Center, President William J. “Bill” Clinton chats with the STS-60 crew during his visit to NASA’s Johnson Space Center. Right: The Mir crew and the STS-60 crew talk with each other through the communications link established during the ABC program Good Morning America.

On the astronauts’ fifth day in orbit, President William J. “Bill” Clinton visited Johnson and stopped in the Mission Control Center to talk with them. NASA Administrator Daniel S. Golden and Johnson Director Carolyn L. Huntoon accompanied the President on his tour. President Clinton praised the crew, saying, “I think this is the first step in what will become the norm in global cooperation. And when we get this space station finished…it’s going to be a force for peace and progress that will be truly historic, and you will have played a major role in that.” The following day, the ABC program Good Morning America set up a communications link between Bolden, Davis, and Krikalev aboard Discovery and the three cosmonauts aboard the Mir space station. The two crews chatted with each other and answered reporters’ questions.

STS-60 Earth observation photographs of North American city Los Angeles STS-60 Earth observation photographs of North American city Chicago STS-60 Earth observation photographs of North American city Montréal STS-60 Earth observation photographs of North American city New York City
A selection of STS-60 Earth observation photographs of North American cities. Left: Los Angeles. Middle left: Chicago. Middle right: Montréal. Right: New York City.

Every space mission includes astronaut Earth photography, and the 57-degree inclination of STS-60 enabled this crew to image areas on the planet not usually visible to astronauts. Many of the images included spectacular views of snow-covered landscapes in the northern hemisphere winter.

Deployment of one of the six spheres of the Orbital Debris Radar Calibration Spheres experiment The six spheres fly away from the shuttle Deployment of the University of Bremen satellite
Left: Deployment of one of the six spheres of the Orbital Debris Radar Calibration Spheres experiment. Middle: The six spheres fly away from the shuttle. Right: Deployment of the University of Bremen satellite.

Once the astronauts had stowed the WSF on flight day seven, they could proceed to the deployment of two payloads. The first called Orbital Debris Radar Calibration Spheres consisted of deploying six metal spheres of three different sizes from Discovery’s payload bay. Ground-based radars and optical telescopes observed and tracked the metal spheres to calibrate their instruments. The University of Bremen in Germany provided the second deployable payload. It measured various parameters of its in-orbit environment as well as its internal pressure and temperature as it burned up when it reentered Earth’s atmosphere.

The STS-60 crew members pose near the end of their successful mission Franklin R. Chang-Díaz, left, and N. Jan Davis close the hatch to the Spacehab module at the end of the mission
Left: The STS-60 crew members pose near the end of their successful mission. Right: Franklin R. Chang-Díaz, left, and N. Jan Davis close the hatch to the Spacehab module at the end of the mission.

With most of the experiments completed by flight day eight, the astronauts busied themselves with tidying up the middeck and the Spacehab. Bolden and Reightler tested Discovery’s reaction control system thrusters and flight control surfaces in preparation for the deorbit, entry, and landing the following day.

Charles F. Bolden prepares to bring Discovery home Bolden makes a perfect touchdown at NASA’s Kennedy Space Center in Florida to conclude STS-60
Left: Charles F. Bolden prepares to bring Discovery home. Right: Bolden makes a perfect touchdown at NASA’s Kennedy Space Center in Florida to conclude STS-60.

On the morning of Feb. 11, the mission’s final day in space, Chang-Díaz and Davis deactivated the Spacehab and closed the hatches to the module. The astronauts donned their launch and entry suits, but NASA delayed their deorbit burn by one orbit due to inclement weather at John F. Kennedy Space Center. Ninety minutes later, they fired the two Orbital Maneuvering System engines to bring them out of orbit and Bolden guided Discovery to a smooth landing at Kennedy, ending the STS-60 mission after 8 days, 7 hours, and 9 minutes, having circled the Earth 130 times.

Enjoy the crew narrate a video about the STS-60 mission. Read Bolden’s and Sega‘s recollections of the STS-60 mission in their oral histories with Johnson’s History Office.

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Kelli Mars

Tiny NASA Cameras to Picture Interaction Between Lander, Moon’s Surface

Tiny NASA Cameras to Picture Interaction Between Lander, Moon’s Surface

4 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Say cheese, Moon. We’re coming in for a close-up.

As Intuitive Machines’ Nova-C lander descends toward the Moon, four tiny NASA cameras will be trained on the lunar surface, collecting imagery of how the surface changes from interactions with the spacecraft’s engine plume.

The Stereo Cameras for Lunar Plume-Surface Studies will help us to land larger payloads as we explore space. Olivia Tyrrell from the SCALPPS photogrammetry team explains how a small array of cameras will capture invaluable imagery during lunar descent and landing, and how that imagery can inform our future missions to the Moon and beyond.

Developed at NASA’s Langley Research Center in Hampton, Virginia, Stereo Cameras for Lunar Plume-Surface Studies (SCALPSS) is an array of cameras placed around the base of a lunar lander to collect imagery during and after descent. Using a technique called stereo photogrammetry, researchers at Langley will use the overlapping images from the version of SCALPSS on Nova-C — SCALPSS 1.0 — to produce a 3D view of the surface.

These images of the Moon’s surface won’t just be a “gee-whiz” novelty. As trips to the Moon increase and the number of payloads touching down in proximity to one another grows, scientists and engineers need to be able to accurately predict the effects of landings.

How much will the surface change? As a lander comes down, what happens to the lunar soil, or regolith, it ejects? With limited data collected during descent and landing to date, SCALPSS will be the first dedicated instrument to measure plume-surface interaction on the Moon in real time and help to answer these questions.

“If we’re placing things  – landers, habitats, etc. – near each other, we could be sand blasting what’s next to us, so that’s going to drive requirements on protecting those other assets on the surface, which could add mass, and that mass ripples through the architecture,” said Michelle Munk, principal investigator for SCALPSS and acting chief architect for NASA’s Space Technology Mission Directorate at NASA Headquarters. “It’s all part of an integrated engineering problem.”

Under Artemis, NASA intends to collaborate with commercial and international partners to establish the first long-term presence on the Moon. On this Commercial Lunar Payload Services (CLPS) initiative delivery, SCALPSS 1.0 is purely focused on how the lander alters the surface of the Moon during landing. It will begin capturing imagery from before the time the lander’s plume begins interacting with the surface until after the landing is complete.

The final images will be gathered on a small onboard data storage unit before being sent to the lander for downlink back to Earth. The team will likely need at least a couple of months to process the images, verify the data, and generate the 3D digital elevation maps of the surface. The expected depression they reveal probably won’t be very deep — not this time, anyway.

“Even if you look at the old Apollo images — and the Apollo crewed landers were larger than these new robotic landers — you have to look really closely to see where the erosion took place,” said Rob Maddock, SCALPSS project manager at Langley. “We’re anticipating something on the order of centimeters deep — maybe an inch. It really depends on the landing site and how deep the regolith is and where the bedrock is.”

But this is a chance for researchers to see how well SCALPSS will work as the U.S. advances into a future where Human-Landing-Systems-class spacecraft will start making trips to the Moon.

“Those are going to be much larger than even Apollo. Those are pretty large engines, and they could conceivably dig some good holes,” said Maddock. “So that’s what we’re doing. We’re collecting data we can use to validate the models that are predicting what will happen.”

SCALPSS 1.1, which will feature two additional cameras, is scheduled to fly on another CLPS delivery — Firefly Aerospace’s Blue Ghost — later this year. The extra cameras are optimized to take images at a higher altitude, prior to the expected onset of plume-surface interaction, and provide a more accurate before-and-after comparison.

SCALPSS 1.0 was funded by NASA’s Science Mission Directorate through the NASA-Provided Lunar Payloads Program. The SCALPSS 1.1 project is funded by the Space Technology Mission Directorate’s Game Changing Development Program.

NASA is working with several American companies to deliver science and technology to the lunar surface through the CLPS initiative.

These companies, ranging in size, bid on delivering payloads for NASA. This includes everything from payload integration and operations, to launching from Earth and landing on the surface of the Moon.

Joe Atkinson
NASA Langley Research Center

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Feb 02, 2024

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Julia L. Bradshaw

Hubble Views a Dim but Distinct Galaxy

Hubble Views a Dim but Distinct Galaxy

2 min read

Hubble Views a Dim but Distinct Galaxy

A spiral galaxy, with two prominent, tightly wound arms around the brighter core. The arms disperse into a wide halo of stars and dust at their ends, giving the galaxy an oval shape. A number of bright, foreground stars appear to flank the galaxy, each holding the signature cross of diffracting light. The image also holds a few distant background galaxies.
Both visible and ultraviolet wavelengths of light comprise this Hubble Space Telescope image of the spiral galaxy UGC 11105.
ESA/Hubble & NASA, R. J. Foley (UC Santa Cruz)

This image of the softly luminous spiral galaxy UGC 11105 is from the NASA/ESA Hubble Space Telescope. It lies about 110 million light-years from Earth in the constellation Hercules.

Astronomers have different ways of quantifying how bright celestial objects are. Apparent magnitude is one of those methods. It describes how bright an object appears to an observer on Earth, which is not the same thing as measuring how bright an object actually is; or its intrinsic brightness. Apparent magnitude depends heavily on an object’s proximity to Earth.

To better understand how apparent magnitude works, consider streetlights; each lamppost is putting out the same amount of light, but the light that is closer to you is much brighter than one several blocks away. Although their intrinsic brightness is the same, their apparent brightness is different.

UGC 11105 has an apparent magnitude, or brightness, of around 13.6 in the light our eyes are sensitive to, called visible or optical light. However, this image also holds ultraviolet data, allowing us to see wavelengths beyond those that the human eye can see. Because of its proximity and our perspective here on Earth, the Sun appears to be about 14 thousand trillion times brighter than UGC 11105, even though UGC 11105 is an entire galaxy. Hubble’s sensitivity and location above Earth’s light-distorting atmosphere allows the observatory to see extraordinarily dim objects in visible light, ultraviolet light, and a small portion of infrared light.

Text credit: European Space Agency (ESA)

Media Contact:

Claire Andreoli
NASA’s Goddard Space Flight CenterGreenbelt, MD
claire.andreoli@nasa.gov

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Last Updated
Feb 02, 2024
Editor
Andrea Gianopoulos
Location
Goddard Space Flight Center

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