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Final Piece of Rocket Hardware Added to Artemis I Stack

Final OSA stacked on top of the ICPS — After successfully completing the integrated modal test, technicians removed the Space Launch System (SLS) rocket’s Orion stage adapter structural test article and the Mass simulator for Orion. Then, they moved the Orion stage adapter flight hardware to the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida. On Oct. 9, the Orion stage adapter was connected to the top of the Interim Cryogenic Propulsion Stage (ICPS) that provides the power to send Orion to the Moon. Soon, Orion, which rides on top of SLS, will be stacked to complete the Artemis I spaceship. Artemis I is the first integrated flight of SLS and Orion. This uncrewed flight test will be followed by Artemis II, which will be the first mission to send astronauts on a mission to orbit the Moon.

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The last piece of Space Launch System (SLS) rocket hardware has been added to the stack at NASA’s Kennedy Space Center in Florida. Crews with NASA’s Exploration Ground Systems and contractor Jacobs added the Orion stage adapter to the top of the rocket inside the spaceport’s Vehicle Assembly Building. To complete the Artemis I stack, crews will soon add the Orion spacecraft and its launch abort system on top of Orion stage adapter.

The Orion stage adapter, built at NASA’s Marshall Space Flight Center in Huntsville, Alabama connects Orion to the Interim Cryogenic Propulsion Stage (ICPS), which was built by Boeing and United Launch Alliance at ULA’s factory in Decatur, Alabama. During the mission, the ICPS will fire one RL10 engine in a maneuver called trans-lunar injection, or TLI, to send Orion speeding toward the Moon.

As Orion heads to the Moon for its mission, the ICPS will separate from Orion and then deploy 10 secondary payloads that are riding to space inside the Orion stage adapter. These CubeSats have their own propulsion systems that will take them on missions to the Moon and other destinations in deep space.

While the ICPS and Orion stage adapter are making it possible for SLS to send its first science payloads to space on this uncrewed mission, they only will be used for the first three Artemis missions. The Exploration Upper Stage (EUS), a more powerful stage with four RL10 engines, will be used on future Artemis missions. The EUS can send 83,000 pounds to the Moon, which is 40 percent more weight than the ICPS. The EUS makes it possible to send Orion, astronauts, and larger and heavier co-manifested payloads to the Moon.

Artemis I will be followed by a series of increasingly complex missions. With Artemis, NASA will land the first woman and the first person of color on the lunar surface and establish long-term exploration at the Moon in preparation for human missions to Mars. SLS and NASA’s Orion spacecraft, along with the commercial human landing system and the Gateway in orbit around the Moon, are NASA’s backbone for deep space exploration. SLS is the only rocket that can send Orion, astronauts, and supplies to the Moon in a single mission.

How many Perseids will I see in 2021?

By Bill Cooke, NASA Meteoroid Environments Office

Many Perseid-related news stories and social media posts state that the maximum rate is about 100 meteors per hour, which is a lot. So, folks get excited and go out on the peak night, braving mosquitos and other nightly hazards. But they are often disappointed; we routinely hear, “I went out and only saw a few meteors. Not even 20, much less 100!” And they would be right. The problem is that the 100 per hour is a theoretical number used by meteor scientists and does not convey what people are actually going to see.

In the 1980’s, meteor researchers were searching for a way to compare the meteor shower rates observed by various individuals and groups across the globe. People were reporting the rates, but the differences in sky conditions, radiant altitude and observer eyesight made getting a comprehensive view of shower activity difficult.

So, the meteor researchers put their heads together and came up with the concept of a ZHR, or Zenithal Hourly Rate. The ZHR is what you get after you correct the observed rates for the sky conditions, the altitude of the radiant above the horizon and observer biases. In other words, it is basically what a perfect observer would see under perfect skies with the meteor shower radiant straight overhead – which never happens!

The often-quoted ZHRs overestimate the meteor rates people actually see – sometimes by a lot. Fortunately, we can take the ZHR and invert things to get the hourly rates for certain locations and circumstances – it’s only math, after all. We have done this for select locations in the United States, producing the following maps.

These maps show the hourly rates that can be expected on the night of the Perseid shower’s peak, provided there are no clouds in the sky. (It’s hard to account for partial cloud cover.)

These rates assume you are out in the country, where lots of stars and the Milky Way are visible and no clouds, of course:

So, instead of 100 Perseids per hour, people in the U.S. can reasonably expect to see around 40-ish Perseids in the hour just before dawn on the peak nights. That’s about one every couple of minutes – not bad. However, we are assuming you are out in the country, well away from cities and suburbs.

What rates can you expect if you want to do your Perseid watching from the neighborhood? We also computed that:

The brighter skies of the suburbs greatly cut down the rates. We have gone from a Perseid every couple of minutes to one every 6-7 minutes – a factor of three reduction. This explains the great disappointment expressed by many casual Perseid watchers; they go outside, expecting to see at least a meteor a minute and end up with 10 or less in an hour. The brightness of your sky is everything in meteor observing – you have to get away from the lights!

But what about those in cities? The rates are close to zero:

Ugh! City dwellers might see a Perseid or two in an hour. Not very inspiring. Perhaps the only good news is that, if someone in a city sees a Perseid, it has to be really, really bright and spectacular.

Want to see Perseids? Then head out into the dark – it’s worth it!

Check out our previous blog post, The Perseids are on the Rise, for more information on the Perseids and tips on how to observe them.

The Perseids are on the Rise!

It’s time again for one of the biggest meteor showers of the year! The Perseids are already showing up in our night skies—and when they peak in mid-August, it’s likely to be one of our most impressive skywatching opportunities for a while.

Perseid Meteor image — In this 30 second exposure taken with a circular fish-eye lens, a meteor streaks across the sky during the annual Perseid meteor shower on Friday, Aug. 12, 2016 in Spruce Knob, West Virginia. Photo Credit: (NASA/Bill Ingalls)

Our meteor-tracking cameras spotted their first Perseid on July 26, but your best chance to see them will start the night of Aug. 11. With the crescent moon setting early, the skies will be dark for the peak viewing hours of midnight (local time) to dawn on Aug. 12.

This chart shows expected levels of Perseid activity for July and August 2021, relative to the peak on Aug. 11-13, ignoring the effects of the Sun, Moon, and clouds. All times are in UTC. Credits: (NASA/MEO/Bill Cooke)

If you’re in the Northern Hemisphere, and far away from light pollution, you might spot more than 40 Perseids an hour! (If you’re in a city, you may only see a few every hour; skywatchers in the Southern Hemisphere will also see fewer Perseids, with none visible below about 30 degrees south latitude.) The night of Aug. 12-13 will be another great opportunity to see the Perseids: with a full Moon (and lower meteor activity) during the Perseids’ peak in 2022 and a waning crescent high in the sky for 2023, this might be your best chance to do some summer skywatching for a few years.

Find somewhere comfortable, avoiding bright lights as much as possible (yes, including your phone), and give your eyes some time to adjust to the dark—up to half an hour if you can. The Perseids will appear as quick, small streaks of light: they get their name because they look like they’re coming from the direction of the constellation Perseus (near Aries and Taurus in the night sky), but Perseids in that area can be hard to spot from the perspective of Earth. So just look up and enjoy the show!

If you can’t see the Perseids where you live, join NASA to watch them on social media! Tune in overnight Aug. 11-12 (10 PM–5 AM CDT; 3–10 AM UTC) on Facebook, Twitter and YouTube to look for meteors with space fans from around the world. If skies are cloudy the night of Aug. 11, we’ll try again the same time on Aug. 12-13. Our livestream is hosted by the Meteoroid Environment Office at NASA’s Marshall Space Flight Center, which tracks meteors, fireballs, and other uncommon sights in the night sky to inform the public and help keep our astronauts and spacecraft safe.

Where do the Perseids *actually* come from?

The Perseids are fragments of the comet Swift-Tuttle, which orbits between the Sun and beyond the orbit of Pluto once every 133 years. Every year, the Earth passes near the path of the comet, and the debris left behind by Swift-Tuttle shows up as meteors in our sky. (Don’t worry, there’s no chance that we’ll run into the actual comet anytime soon.)

Where can I go to learn more?

We’ve got some great space-rock lessons for students, starting with the biggest question: what’s the difference between an asteroid and a meteor? Our NASA Space Place site also has a kid-friendly introduction to meteor showers in general. If you’re looking for something a little more hands-on, try this asteroid-building classroom activity—or, for an older audience, learn how to describe rocks like a NASA scientist.

And, if you want to know what else is in the night sky this month, check out the video below from Jet Propulsion Laboratory’s monthly “What’s Up” video series:

Happy skywatching!

by Brice Russ

NASA Prepares Three More CubeSat Payloads for Artemis I Mission

Two more secondary payloads that will travel to deep space on the Artemis I mission were integrated for launch on July 23, and another is ready for installation at NASA’s Kennedy Space Center in Florida.

The satellites – called CubeSats – are roughly the size of a large shoe box and weigh no more than 30 pounds. Despite their small size, they enable science and technology experiments that may enhance our understanding of the deep space environment, expand our knowledge of the Moon, and demonstrate new technologies that could be used on future missions.

The OMOTENASHI (Outstanding MOon exploration Technologies demonstrated by NAno Semi-Hard Impactor) team prepares their secondary payload for a ride on NASA’s Space Launch System rocket during the Artemis I mission. If successful, OMOTENASHI will be the smallest spacecraft ever to land on the lunar surface and will mark Japan as the fourth nation to successfully land a craft on the Moon.

OMOTENASHI (Outstanding MOon exploration Technologies demonstrated by NAno Semi-Hard Impactor) and ArgoMoon, which will both study the Moon, were integrated with their dispensers and installed on the Orion stage adapter along with seven other payloads for the Space Launch System (SLS) rocket’s first flight. A third payload, the BioSentinel CubeSat is the only CubeSat that will contain a biological experiment on Artemis I and will be the first CubeSat to support biological research in deep space. The team placed it in its dispenser for the flight, and to preserve its biological contents, it is being kept in a controlled environment at NASA’s Kennedy Space Center in Florida. At a date closer to launch, it will be placed in the Orion stage adapter.

OMOTENASHI was developed by the Japan Aerospace Exploration Agency (JAXA). While OMOTENASHI is one of several Artemis I secondary payloads that are studying the Moon, it is the only one that will conduct a controlled landing on the Moon’s surface. Its primary objective is to test the technologies and trajectory maneuvers that allow a small lander to land on the Moon while keeping its systems – including power, communication, and propulsion systems – intact. Testing these systems around and on the Moon can help with development of similar small landers that could explore other planets. The spacecraft will also measure the radiation environment beyond low-Earth orbit, providing data that will help develop technologies to manage radiation exposure for human exploration. If successful, OMOTENASHI will be the smallest spacecraft ever to land on the lunar surface and will mark Japan as the fourth nation to successfully land on the Moon.

ArgoMoon, developed by Italian company Argotec and sponsored by Agenzia Spaziale Italiana (ASI), Italy’s national space agency, will perform autonomous visual-based proximity operations around the Interim Cryogenic Propulsion Stage (ICPS), the in-space stage of SLS, that provides the propulsion to send Orion on a lunar trajectory. The CubeSat will use high-definition cameras and advanced imaging software to record images of the ICPS and later of the Earth and the Moon for historical documentation, provide mission data on the deployment of other CubeSats, and test optical communication capabilities between the CubeSat and Earth. ArgoMoon will use a hybrid micropropulsion system (MiPS) that combines green mono-propellant and cold gas propulsion in a single system to provide attitude control and orbital maneuvering using a small amount of power.

The enhanced attitude capabilities are also used to run and validate artificial intelligence-based algorithms for autonomous Failure Detection, Isolation and Recovery systems that perform continuous monitoring of the health of the satellite to detect any potential fault. In the case of fault detection, this service performs several operations to solve the problem. If the fault is not recoverable, the satellite goes in safe mode, which means that only the functionalities to keep the satellite alive and to communicate with ground are used.

ArgoMoon’s mission is a forerunner of technologies for deep space application that can be used for inspection of satellites not originally designed to be serviced, without the involvement of the ground segment.

BioSentinel will be the first long-duration biology experiment to take place in deep space and will be among the first studies of the biological response to space radiation outside low-Earth orbit in nearly 50 years. Its primary objective is to measure the impact of space radiation on living organisms – in this case, yeast – over long durations beyond low-Earth orbit.

The BioSentinel team prepares their CubeSat to be the first long-duration biology experiment to take place in deep space, and the first study of the biological response to space radiation outside low-Earth orbit in nearly 50 years. The team placed the CubeSat in its dispenser and to preserve its biological contents, it is being kept in a controlled environment at NASA’s Kennedy Space Center in Florida. It will be placed in the Orion stage adapter at date closer to launch.

Developed by NASA’s Ames Research Center in California’s Silicon Valley, BioSentinel will enter an orbit around the Sun via a lunar flyby. The experiment will use yeast as a “living radiation detector” to evaluate the effects of ambient space radiation on biology. Human cells and yeast cells have many similar biological mechanisms, including DNA damage and repair.

The payload carries dry yeast cells stored in microfluidic cards – custom hardware that allows for the controlled flow of extremely small volumes of liquids that will activate and sustain the yeast. These yeast-filled cards are situated alongside a physical radiation detection instrument – developed at NASA’s Johnson Space Center in Houston – that measures and characterizes the radiation environment. Results from the physical instrument will be compared to the payload’s biological response. After completing a lunar flyby and spacecraft checkout, the yeast will be rehydrated at various points during the six-month mission. As yeast cells activate in space, they will sense and respond to the radiation damage.

Experiments using the BioSentinel instruments will also take place on the International Space Station and on the ground to demonstrate how varied amounts of radiation affect the yeast. While Earth-bound research has helped identify some of the potential effects of space radiation on living organisms, no terrestrial source can fully simulate the unique radiation environment of deep space. BioSentinel’s data will provide critical insight on the effects of deep space radiation on biology as NASA seeks to establish long-term human exploration of the Moon under Artemis and prepare us for human exploration on Mars.

SLS will launch America into a new era of exploration to destinations beyond low Earth orbit. On its first flight, NASA will demonstrate the rocket’s heavy-lift capability and send an uncrewed Orion spacecraft into deep space. The agency is also taking advantage of additional available mass and space to provide the rare opportunity to send several CubeSats to conduct science experiments and technology demonstrations in deep space. All CubeSats are deployed after SLS completes its primary mission, launching the Orion spacecraft on a trajectory toward the Moon.

Two More Artemis I Deep Space CubeSats Prepare for Launch

Two additional secondary payloads that will travel to deep space on Artemis I, the first flight of the Space Launch System (SLS) rocket and Orion spacecraft, are ready for launch.

The Team Miles and EQUilibriUm Lunar-Earth point 6U Spacecraft (EQUULEUS) CubeSats are tucked into dispensers and installed in the Orion stage adapter – the ring that connects Orion to the SLS rocket. They are joining five other secondary payloads that were recently installed. These small satellites, known as CubeSats, will conduct a variety of science experiments and technology demonstrations. The CubeSats will deploy after the Orion spacecraft separates from SLS.

Developed by Miles Space in partnership with software developer Fluid & Reason, LLC, the Team Miles CubeSat will travel to deep space to demonstrate propulsion using plasma thrusters, a propulsion that uses low-frequency electromagnetic waves. The CubeSat was developed as part of NASA’s Cube Quest Challenge and sponsored by the agency’s Space Technology Mission Directorate (STMD) Prizes, Challenges, and Crowdsourcing program. The team, composed of citizen scientists and engineers, came together through the nonprofit Tampa Hackerspace in Florida to develop Team Miles. The group considers itself a team of “makers,” who are open to trying technologies that may fall outside of engineering norms.

Members of the EQUULEUS (EQUilibriUm Lunar-Earth point 6U Spacecraft) team prepare their CubeSat to be loaded in the Space Launch System’s Orion stage adapter for launch on the Artemis I mission. This CubeSat, developed jointly by the Japan Aerospace Exploration Agency (JAXA) and the University of Tokyo, will help scientists understand the radiation environment in the region of space around Earth called the plasmasphere.

Team Miles’ mission will be flown autonomously by a sophisticated onboard computer system. In addition, the breadbox-sized spacecraft will use a software-defined radio for communications with Earth. If successful, the CubeSat will travel farther than this size of craft has ever gone – 59.6 million miles (96 million kilometers) – before ending the mission. (For comparison, the minimum distance from Earth to Mars is around 34 million (54 million) kilometers.)

EQUULEUS, developed jointly by the Japan Aerospace Exploration Agency (JAXA) and the University of Tokyo, will travel to Earth-Moon Lagrange Point 2, an Earth-Moon orbit where the gravitational pull of the Earth and Moon equal the force required for a small object to move with them. The CubeSat will demonstrate trajectory control techniques within the Sun-Earth-Moon region and image Earth’s plasmasphere, a region of the atmosphere containing electrons and highly ionized particles that rotate with the planet.

Team Miles works in a clean room at NASA’s Kennedy Space Center in Florida to prepare their CubeSat to be launched on the Artemis I mission. The team designed the satellite to travel farther than this size of craft has ever gone – 59.6 million miles (96 million kilometers) – before ending its mission. The CubeSat was developed as part of NASA’s Cube Quest Challenge and sponsored by Space Technology Mission Directorate (STMD) Prizes, Challenges, and Crowdsourcing program.

EQUULEUS will measure the distribution of the plasmasphere, providing important insight for protecting humans and electronics from radiation damage during long space journeys. The CubeSat will also measure meteor impact flashes and the dust environment around the Moon, providing additional important information for human exploration. EQUULEUS will be powered by two deployable solar arrays and batteries, propelled by a warm gas propulsion system with water as the propellant.

SLS will launch America into a new era of exploration to destinations beyond Earth’s orbit and demonstrate the rocket’s heavy-lift capability. The agency is taking advantage of additional available mass and space to provide the rare opportunity to send several CubeSats to conduct science experiments and technology demonstrations in deep space. All CubeSats are deployed after SLS completes its primary mission, launching the Orion spacecraft on a trajectory toward the Moon.

Artemis I CubeSats will study the Moon, solar radiation

Three additional CubeSats that will ride aboard the Space Launch System (SLS) rocket for the Artemis I mission are installed in the rocket’s Orion stage adapter that will deploy them toward their deep space destinations.

The Lunar Polar Hydrogen Mapper (LunaH-Map), the CubeSat to Study Solar Particles (CuSP) spacecraft, and LunIR were integrated with their dispensers and installed on the Orion stage adapter along with several other small satellites for the first flight of SLS and Orion. Artemis I provides a rare opportunity for CubeSats, each about the size of a large cereal box, to hitch a ride to deep space. The Orion stage adapter connects the Orion spacecraft to the SLS rocket and will carry the CubeSats and deploy them after Orion departs for its lunar exploration mission.

LunaH-Map, developed by Arizona State University and sponsored by NASA’s Science Mission Directorate (SMD), will measure the distribution and amount of hydrogen throughout the Moon’s South Pole. If successful, the LunaH-Map spacecraft will produce a high-resolution map of the Moon’s bulk water deposits, unveiling new details about the spatial and depth distribution of potential ice previously identified during a variety of missions. Confirming and mapping these deposits in detail will help NASA understand how the water got there, how much water might be available, and how it could potentially serve as a resource for longer exploration missions on the Moon. The CubeSat’s mission is designed to last around 60 days.

A team prepares the LunaH-Map before its installation in the Space Launch System rocket Orion stage adapter at NASA’s Kennedy Space Center in Florida. Once deployed from the rocket, the CubeSat will orbit the Moon for two months while searching for water deposits near the South Pole.

LunIR was developed by Lockheed Martin Space in Denver, Colorado, and sponsored by NASA’s Advanced Exploration Systems division under the Human Exploration and Operations Mission Directorate. The CubeSat will conduct a lunar flyby and use an advanced miniature infrared sensor to gather images and data about the lunar surface and its environment. This effort will help collect data to address knowledge gaps related to transit and long-duration exploration to Mars and beyond. The CubeSat will collect data about the lunar surface, including material composition, thermal signatures, presence of water, and potential landing sites. LunIR’s infrared sensor will be able to map the Moon during both day and night and can collect data at much higher temperatures than similar sensors, thanks to an innovative micro-cryocooler – similar to a refrigerator – designed to reach cryogenic temperatures below minus 234 degrees Fahrenheit.

CuSP will be deployed for an interplanetary mission to study the particles and magnetic fields that stream from the Sun. CuSP was developed by the Southwest Research Institute , NASA Goddard Space Flight Center in Greenbelt, Maryland, and the Jet Propulsion Laboratory in Pasadena, CA and is also sponsored by NASA’s SMD. This CubeSat will orbit the Sun with three instruments to measure incoming radiation and the magnetic field that can create a variety of effects on Earth, such as interfering with radio communications, tripping up satellite electronics, and creating electronic currents in power grids. CuSP can observe events in space hours before those events potentially reach Earth.

Team CuSP cheers on the solar CubeSat prior to loading it in the Space Launch System rocket Orion stage adapter at NASA’s Kennedy Space Center in Florida.

SLS will launch America into a new era of exploration to destinations beyond Earth’s orbit. On its first flight, NASA will demonstrate the rocket’s super heavy-lift capability and send an uncrewed Orion spacecraft into deep space. The agency is also taking advantage of additional available mass and space to provide the rare opportunity to send several CubeSats to conduct science experiments and technology demonstrations in deep space. All CubeSats are deployed after SLS completes its primary mission, launching the Orion spacecraft on a trajectory toward the Moon.

First CubeSats Aboard for Artemis I Mission

The first two CubeSats are aboard for the Artemis I mission as secondary payloads that will conduct a range of science experiments and technology demonstrations in deep space.

In preparation for their missions, Lunar IceCube and Near-Earth Asteroid (NEA) Scout have been integrated with their dispensers and installed in the Orion stage adapter at NASA’s Kennedy Space Center in Florida. Housed in the spaceport’s Space Station Processing Facility, the Orion stage adapter connects the top of the Space Launch System (SLS) rocket to the Orion spacecraft. The small satellites, roughly the size of large shoeboxes and weighing no more than 30 pounds, enable science and technology experiments that may enhance our understanding of the deep space environment, expand our knowledge of the Moon and beyond, and demonstrate technology that could open up possibilities for future missions. The payloads will deploy from the rocket after the Orion spacecraft separates from the rocket’s Interim Cryogenic Propulsion Stage that provides the propulsion to send Orion to the Moon.

The Near-Earth Asteroid Scout team prepares their secondary payload for installation in the Space Launch System rocket’s Orion stage adapter at NASA’s Kennedy Space Center in Florida. NEA Scout will be deployed and go to an asteroid after the Orion spacecraft separates from the Space Launch System rocket and heads to the Moon during the Artemis I mission.

NEA Scout will be the first CubeSat to travel to an asteroid. The small payload was developed by NASA’s Marshall Space Flight Center in Huntsville and the agency’s Jet Propulsion Laboratory in Southern California. NEA Scout will be propelled by a square-shaped solar sail that will measure about 925 square feet (86 square meters) when unfurled. The sail is made of an aluminum-coated plastic film that is thinner than a human hair, with an area about the size of a racquetball court. NEA Scout is outfitted with a high-powered camera that will take photographs of and collect data from a near-Earth asteroid that represents asteroids that may one day become destinations for human exploration. Observations will include the asteroid’s position in space, its shape, rotational properties, spectral class, and geological characteristics. NEA Scout’s mission will take approximately two years.

Teams prepare the Lunar IceCube before its installation in the Space Launch System rocket Orion stage adapter at NASA’s Kennedy Space Center in Florida. This small satellite will be deployed from the rocket and will orbit the Moon for six months and search for water and ice with an infrared spectrometer.

Lunar IceCube will search for water ice and other resources from above the surface of the Moon. It was developed by Morehead State University in Kentucky, Busek Space Propulsion and Systems of Massachusetts, NASA’s Goddard Space Flight Center in Greenbelt, Maryland, JPL, and NASA’s Katherine Johnson Independent Verification and Validation Facility in Fairmont, West Virginia. Once deployed, the CubeSat will take up to nine months to arrive at its destination and begin orbiting the Moon. Using state-of-the-art miniature electric thrusters for propulsion and relying on gravity assists from Earth and the Moon, Lunar IceCube will search for water and other materials in ice, liquid, or vapor states that may be useful for future exploration missions. Once in orbit, Lunar IceCube’s mission could last one to six months and the ground station at Morehead State will be used to track the CubeSat for the duration of the mission.

SLS will launch America into a new era of exploration to destinations beyond Earth’s orbit. On its first flight, NASA will demonstrate the rocket’s heavy-lift capability and send an uncrewed Orion spacecraft into deep space. The agency is also taking advantage of additional available mass and space to provide the rare opportunity to send several CubeSats to conduct science experiments and technology demonstrations in deep space.

The NEA Scout and Lunar IceCube secondary payloads are the first to be installed in the Space Launch System (SLS) rocket’s Orion stage adapter for the Artemis I mission on July 14 at NASA’s Kennedy Space Center in Florida.

Parabolic Pre-flight Checklist

How do you prepare for weightlessness? A team of researchers at NASA’s Marshall Space Flight Center has been doing so in preparation of their April 28 and 29 parabolic flights with ZERO-G in Fort Lauderdale, Florida.

Marshall's parabolic flight crew — The Marshall team exits the G Force One after the first day of parabolic flights. (NASA)

So what is on their parabolic pre-flight checklist?

An easily digestible breakfast
The flight team is served a doctor-recommended breakfast of bagels, fruit, and juice — all of which digest quickly and easily to provide fuel for their bodies as they experience periods of variable gravity.

Proper attire
Fort Lauderdale is a subtropical climate with warm and humid conditions in the spring. Participants wear light, comfortable clothing and closed toed shoes for movement in the hangar, on the ramp, and on the aircraft. Each flyer wears a ZERO-G flight suit, which enables ease of movement in air.

A COVID-19 test
All non-vaccinated participants are tested for COVID-19 daily to ensure safety of all parties.

Identification
Just like a typical commercial flight, each individual must complete a TSA check before boarding the aircraft. They must present a valid driver’s license, passport, or other TSA-approved identification.

Once all the pre-flight boxes are checked, the team will board a modified Boeing 727 — named G Force One — to execute their experiment in a weightless environment.

Marshall's flight team completes a TSA check before boarding G Force One. — Marshall’s flight team completes a TSA check before boarding G Force One. (NASA)

While in the air, the team will test an experiment known as the Ring-Sheared Drop. Developed by Marshall and Rensselaer Polytechnic Institute of Troy, New York, the experiment will study the formation of potentially destructive amyloid fibrils, or protein clusters, like those found in the brain tissue of patients battling neurodegenerative diseases — such as Alzheimer’s and Parkinson’s.

To track the flight path as it performs parabolas, check out Flight Aware.

For more updates on the flight, the team, and the experiment, continue to follow Watch the Skies blog in the coming week.

Ring-Sheared Drop Team Prepares for Zero-G Flight

A team of researchers from NASA’s Marshall Space Flight Center is preparing to take flight and evade gravity in pursuit of science.

Team members are traveling to Fort Lauderdale, Florida, to test an experiment known as the Ring-Sheared Drop. Developed by Marshall and Rensselaer Polytechnic Institute of Troy, New York, the experiment will study the formation of potentially destructive amyloid fibrils, or protein clusters, like those found in the brain tissue of patients battling neurodegenerative diseases — such as Alzheimer’s and Parkinson’s.

The Ring-Sheared Drop team boards G Force One in Fort Lauderdale, Florida with their equipment. (NASA)

In Earth-based experiments, researchers determined that amyloid fibrils may be created by shear flow, or the difference in flow velocity between adjacent layers of a liquid. In the case of ground experiments, that formation is affected by the presence of container walls and by convection, or the circular motion that occurs when warmer liquid rises while cooler liquid descends.

The goal now is to conduct experiments in microgravity — in a containerless reactor — where the liquid specimens form spherical drops, containing themselves via surface tension. Researchers will “pin” a droplet of liquid between two rings and cultivate amyloid fibrils for study.

The experiment was initially launched to the International Space Station in 2019. However, when the experiment failed, efforts began on Earth to improve the testing apparatus for future testing. Now, before the equipment is ready for another trip to the space station, the team will “practice” pinning liquid drops on a parabolic flight.

The research team installs their experimental hardware on G Force One in preparation for April 28, 29 parabolic flights. (NASA)

How exactly is weightlessness reached? A modified Boeing 727 — named G-Force One — achieves periods of variable gravity through a series of maneuvers called parabolas. The team will be able to interact with their hardware in zero gravity for 22 seconds at a time.

NASA’s Flight Opportunities program, within the Space Technology Mission Directorate, makes these experiment flights possible by facilitating rapid demonstration of promising technologies for space exploration, discovery, and results benefit life on Earth.

The program matures capabilities needed for NASA missions and commercial applications while strategically investing in the growth of the U.S. commercial spaceflight industry.

The Ring-Sheared Drop team is scheduled to fly with their hardware April 28 and 29 on a parabolic flight managed by Zero G of Fort Lauderdale, Florida.

Continue to follow NASA’s Watch the Skies blog in the coming weeks for the latest updates on the team, the parabolic flight, and the results of the Ring-Sheared Drop experiment.

NASA Team Preparing Hardware for Future Moon Rockets

Technicians and engineers continue to make progress manufacturing core stages that will help power NASA’s Space Launch System (SLS) rocket for its second and third flights. NASA and Boeing, the lead contractor for the core stage, are in the process of conducting one of the biggest Artemis II milestones: assembling the top half of the core stage.

The 212-foot tall core stage for the SLS rocket is the largest rocket stage NASA has ever produced. The five individual elements that make up the core stage – the forward skirt, liquid oxygen tank, intertank, liquid hydrogen tank, and the engine section – are manufactured and assembled at NASA’s Michoud Assembly Facility in New Orleans. Together, the elements will supply propellant, vehicle control, and power to the four RS-25 engines at the bottom of the stage to produce more than 2 million pounds of thrust to send missions to the Moon.

The team manufactures every SLS core stage in Michoud’s 43-acre building which provides more than enough space for crews to work in tandem to build the core stages for Artemis II and Artemis III, the second and third flights of the SLS rocket and the first crewed missions of NASA’s Artemis program.

It takes teamwork to build a super heavy-lift rocket. Look behind the scenes at the work being done at NASA’s rocket factory:

The Artemis II Intertank is lifted into the Cell D of the VAB at NASA Michoud Assembly Facility on Friday, March 19, 2021.

Coming together to build the upper part of the rocket

After all the core stage’s large five structures are built and outfitted, these structures are connected during three major joining operations. For first one, the forward or upper parts of the core stage are joined together for the first time. First, teams move the intertank into an assembly area and connect it to the liquid oxygen tank, and then they add the forward skirt to form the entire upper part of the SLS core stage.

Crews with NASA and Boeing, the core stage prime contractor, recently moved the Artemis II intertank, above, to the assembly area where the three components will be stacked.

The Artemis II forward skirt, pictured above, has been outfitted and is ready for integration with the other large core stage structures. The forward skirt houses flight computers, cameras, and avionics systems. It is located at the very top of the core stage and connects to the upper part of the rocket.

Moving through the manufacturing process

The core stage has two huge cryogenic liquid propellant tanks that collectively hold more than 733,000 gallons of liquid propellant to help launch the Space Launch System rocket to the Moon. Moving the immense hardware, especially the two propellant tanks, around the factory is a delicate process.

Teams carefully orchestrate every step of every lift and transport inside and outside the rocket factory. To safely and securely move hardware, they use special transporters and cranes that are designed to contain, hold, and handle the weight of each element. Above, teams move the more than 130-foot-tall liquid hydrogen tank to the same area as the liquid oxygen tank. Both propellant tanks will be used for Artemis II.

The aisles at Michoud are extra-wide to ensure large hardware can be transported throughout the factory. For the next phase of manufacturing, crews recently moved the boat-tail, a fairing-like cover that attaches to the engine section on the bottom of the core stage. The boat-tail is shown in the image foreground, and the engine section for Artemis II can be seen in the background covered with scaffolding. The four RS-25 engines for the SLS rocket will be mounted inside the engine section, and the boat-tail helps to protect and cover most of the four RS-25 engines’ critical systems.

Fusion Weld on H3 R2

It’s all in the details

As crews prepare the core stage elements that will be used for Artemis II for assembly and integration, the hardware for Artemis III is being welded in other areas of the factory. Engineers and technicians use friction-stir welding methods to connect the panels that make up each piece of hardware together and build larger structures. Fusion welding is traditional welding, and it uses heat to plug holes left by machines welding the larger pieces as well as for any necessary weld repairs.

Welding processes help to create the shells, or outside, of the core stage structures. Above, the engine section for Artemis III comes together in the Vertical Weld Center at Michoud. They are made by connecting panels such as the one in the front of this image. The engine section has been completed and moved to another part of the factory. One of the biggest tasks ahead, is outfitting it with a network of internal components and systems that connect to the RS-25 engines.

In May, the core stage team will begin work on the Artemis IV core stage, so three stages will be under construction at the same time. Because of the factory’s size, state-of-the-art equipment, and manufacturing processes, skilled workers can produce multiple rocket stages to power NASA’s next-generation Moon missions through the Artemis program.

NASA is working to land the first woman and the first person of color on the Moon. SLS and Orion, along with the human landing system and the Gateway in orbit around the Moon, are NASA’s backbone for deep space exploration. SLS is the only rocket that can send Orion, astronauts, and supplies to the Moon in a single mission.