The Heat is On! NASA’s “Flawless” Heat Shield Demo Passes the Test

The Heat is On! NASA’s “Flawless” Heat Shield Demo Passes the Test

5 Min Read

The Heat is On! NASA’s “Flawless” Heat Shield Demo Passes the Test

The Low-Earth Orbit Flight Test of an Inflatable Decelerator, or LOFTID, spacecraft is pictured after its atmospheric re-entry test in November 2022.

The Low-Earth Orbit Flight Test of an Inflatable Decelerator, or LOFTID, spacecraft is pictured after its atmospheric re-entry test in November 2022.

Credits:
NASA / Greg Swanson

A little more than a year ago, a NASA flight test article came screaming back from space at more than 18,000 mph, reaching temperatures of nearly 2,700 degrees Fahrenheit before gently splashing down in the Pacific Ocean. At that moment, it became the largest blunt body — a type of reentry vehicle that creates a heat-deflecting shockwave — ever to reenter Earth’s atmosphere.

The Low-Earth Orbit Flight Test of an Inflatable Decelerator (LOFTID) launched on Nov. 10, 2022, aboard a United Launch Alliance (ULA) Atlas V rocket and successfully demonstrated an inflatable heat shield. Also known as a Hypersonic Inflatable Aerodynamic Decelerator (HIAD) aeroshell, this technology could allow larger spacecraft to safely descend through the atmospheres of celestial bodies like Mars, Venus, and even Saturn’s moon, Titan.

“Large-diameter aeroshells allow us to deliver critical support hardware, and potentially even crew, to the surface of planets with atmospheres. This capability is crucial for the nation’s ambition of expanding human and robotic exploration across our solar system,” said Trudy Kortes, director of the Technology Demonstrations Missions (TDM) program within the agency’s Space Technology Mission Directorate (STMD) at NASA Headquarters in Washington.

NASA has been developing HIAD technologies for over a decade, including two smaller scale suborbital flight tests before LOFTID. In addition to this successful tech demo, NASA is investigating future applications, including partnering with commercial companies to develop technologies for small satellite reentry, aerocapture, and cislunar payloads.

“This was a keystone event for us, and the short answer is: It was highly successful,” said LOFTID Project Manager Joe Del Corso. “Our assessment of LOFTID concluded with the promise of what this technology may do to empower the exploration of deep space.”

Due to the success of the LOFTID tech demo, NASA announced under its Tipping Point program that it would partner with ULA to develop and deliver the “next size up,” a larger 12-meter HIAD aeroshell for recovering the company’s Vulcan engines from low Earth orbit for reuse.

A Successful Test in the Books, A Video Recap

The LOFTID team recently held a post-flight analysis assessment of the flight test at NASA’s Langley Research Center in Hampton, Virginia. Their verdict?

Upon recovery, the team discovered LOFTID appeared pristine, with minimal damage, meaning its performance was, as Del Corso puts it, “Just flawless.”

Here are some interesting visual highlights from LOFTID’s flight test.

NASA

To get to atmospheric reentry, LOFTID had to go through an intricate sequence of events. Del Corso compared it to a Rube Goldberg device, a complex machine designed to carry out simple tasks through a series of chain reactions.

Video captured the moment LOFTID deployed the HIAD (on the left), compared to a preflight animation developed by NASA Langley’s Advanced Concepts Lab (on the right). Inflation happens at the bottom of the video as LOFTID flies over the African continent.

NASA

As it flew over the Mediterranean Sea, LOFTID separated from the ULA Centaur upper stage. On the left, LOFTID is seen from Centaur’s forward-facing camera. The composite image on the right is from cameras around LOFTID’s center body, looking forward and outboard at the orange inflatable HIAD structure. In the center, looking back at Centaur, LOFTID is seen from an aft-facing camera.

The camera captured footage of the plasma quickly changing colors from orange to purple. Why the color change? “We’re still investigating exactly what causes that,” said John DiNonno, LOFTID chief engineer. The animation on the left shows an artist’s concept of what the front side may have looked like.
NASA

As LOFTID reentered Earth’s atmosphere and reached nearly 2,700 degrees Fahrenheit, the extreme heat caused gases around it to ionize and form plasma. On the right, the images from the center body cameras became extremely bright in the visible spectrum, while the Earth is visible on infrared cameras  as the vehicle rotated.

The camera captured footage of the plasma quickly changing colors from orange to purple. Why the color change? “We’re still investigating exactly what causes that,” said John DiNonno, LOFTID chief engineer. The animation on the left shows an artist’s concept of what the front side may have looked like.

This video, captured by NASA Langley’s Scientifically Calibrated In-Flight Imagery team, shows LOFTID during peak deceleration as the plasma recedes. On the left, LOFTID streaks through the night sky over the Pacific Ocean. On the right, the purple coloration flares up on the back side of LOFTID. In the second part of the video, the left shifts to one of the cameras looking at the back of the aeroshell, with the receding plasma streaking at its edge.
NASA

This video, captured by NASA Langley’s Scientifically Calibrated In-Flight Imagery  team, shows LOFTID during peak deceleration as the plasma recedes. On the left, LOFTID streaks through the night sky over the Pacific Ocean. On the right, the purple coloration flares up on the back side of LOFTID.

In the second part of the video, the left shifts to one of the cameras looking at the back of the aeroshell, with the receding plasma streaking at its edge.

After slowing down from more than 18,000 mph to less than 80 mph, LOFTID deployed its parachutes. From an infrared camera aboard the recovery ship, this video shows the parachute deployment and splashdown just over the horizon. The preflight animation is provided on the right for comparison.
NASA

After slowing down from more than 18,000 mph to less than 80 mph, LOFTID deployed its parachutes. 

From an infrared camera aboard the recovery ship, this video shows the parachute deployment and splashdown just over the horizon. The preflight animation is provided on the right for comparison.

LOFTID splashed down in the Pacific Ocean several hundred miles off the east coast of Hawaii and only about eight miles from the recovery ship’s bow — almost exactly as modeled. A crew got on a small boat and retrieved and hoisted LOFTID onto the recovery ship. Here is an image from the first contact with LOFTID after it splashed down.
NASA

LOFTID splashed down in the Pacific Ocean several hundred miles off the east coast of Hawaii and only about eight miles from the recovery ship’s bow — almost exactly as modeled. A crew got on a small boat and retrieved and hoisted LOFTID onto the recovery ship. Here is an image from the first contact with LOFTID after it splashed down.

“The LOFTID mission was important because it proved the cutting-edge HIAD design functioned successfully at an appropriate scale and in a relevant environment,” said Tawnya Laughinghouse, manager of the TDM program office at NASA’s Marshall Space Flight Center in Huntsville, Alabama.

The LOFTID demonstration was a public private-partnership with ULA funded by STMD and managed by the Technology Demonstration Mission Program, executed by NASA Langley with contributions from across NASA centers. Multiple U.S. small businesses contributed to the hardware. NASA’s Launch Services Program  was responsible for NASA’s oversight of launch operations.

For more information on LOFTID, click here.

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Julia L. Bradshaw

Hubble Images Galaxy with an Explosive Past

Hubble Images Galaxy with an Explosive Past

2 min read

Hubble Images Galaxy with an Explosive Past

A spiral galaxy, seen face-on from Earth. The spiral arms of the galaxy are bright but not well defined, merging into a swirling disk with a faint halo of dimmer gas around it. The core glows brightly in a lighter color and has a bit of faint dust crossing it. Two redder, visually smaller galaxies and a bright star are prominent around the galaxy, with more tiny objects in the background.
A NASA Hubble Space Telescope image of the spiral galaxy NGC 941.
ESA/Hubble & NASA, C. Kilpatrick

This image from NASA’s Hubble Space Telescope features the spiral galaxy NGC 941, which lies about 55 million light-years from Earth. Hubble’s Advanced Camera for Surveys (ACS) collected the data that created this image. Beautiful NGC 941 is undoubtedly the main attraction in this view; however, the hazy-looking galaxy was not the motivation for collecting the data. That distinction belongs to an astronomical event that took place in the galaxy years before: the supernova SN 2005ad. The location of this faded supernova was observed as part of a study of multiple hydrogen-rich supernovae, also known as type II supernovae, to better understand the environments in which certain types of supernovae take place. While the study was conducted by professional astronomers, SN 2005ad itself owes its discovery to a distinguished amateur astronomer named Kōichi Itagaki, who has discovered over 170 supernovae.

This might raise the question of how an amateur astronomer could spot something like a supernova event before professional astronomers who have access to telescopes such as Hubble. The detection of supernovae is a mixture of skill, facilities, and luck. Most astronomical events happen over time spans that dwarf human lifetimes, but supernova explosions are extraordinarily fast, appearing very suddenly and then brightening and dimming over a period of days or weeks. Another aspect is time – data from a few hours of observations with telescopes like Hubble might take weeks, months, or sometimes even years to process and analyze. Amateur astronomers can spend much more time actively observing the skies, and sometimes have extremely impressive systems of telescopes, computers, and software they can use. 

Because amateurs like Itagaki spot so many supernovae, there is actually an online system set up to report them (the Transient Name Server). This system is a big help to professional astronomers, because time is truly of the essence with supernovae events. After the reported discovery of SN 2005ab, professional astronomers were able to follow up with spectroscopic studies and confirm it as a type II supernova, which eventually led to Hubble to study its location. Such a study wouldn’t be possible without a rich library of cataloged supernovae, built with the keen eyes of amateur astronomers.

Text credit: European Space Agency

Media Contact:

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

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Last Updated
Nov 16, 2023
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Andrea Gianopoulos
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NASA’s Deep Space Optical Comm Demo Sends, Receives First Data

NASA’s Deep Space Optical Comm Demo Sends, Receives First Data

6 min read

NASA’s Deep Space Optical Comm Demo Sends, Receives First Data

NASA’s Psyche spacecraft is shown in a clean room
NASA’s Psyche spacecraft is shown in a clean room at the Astrotech Space Operations facility near the agency’s Kennedy Space Center in Florida on Dec. 8, 2022. DSOC’s gold-capped flight laser transceiver can be seen, near center, attached to the spacecraft.
NASA/Ben Smegelsky

DSOC, an experiment that could transform how spacecraft communicate, has achieved ‘first light,’ sending data via laser to and from far beyond the Moon for the first time.

NASA’s Deep Space Optical Communications (DSOC) experiment has beamed a near-infrared laser encoded with test data fromnearly 10 million miles (16 million kilometers) away – about 40 times farther than the Moon is from Earth – to the Hale Telescope at Caltech’s Palomar Observatory in San Diego County, California. This is the farthest-ever demonstration of optical communications.

Riding aboard the recently launched Psyche spacecraft, DSOC is configured to send high-bandwidth test data to Earth during its two-year technology demonstration as Psyche travels to the main asteroid belt between Mars and Jupiter. NASA’s Jet Propulsion Laboratory in Southern California manages both DSOC and Psyche.

The tech demo achieved “first light” in the early hours of Nov. 14 after its flight laser transceiver – a cutting-edge instrument aboard Psyche capable of sending and receiving near-infrared signals – locked onto a powerful uplink laser beacon transmitted from the Optical Communications Telescope Laboratory at JPL’s Table Mountain Facility near Wrightwood, California. The uplink beacon helped the transceiver aim its downlink laser back to Palomar (which is 100 miles, or 130 kilometers, south of Table Mountain) while automated systems on the transceiver and ground stations fine-tuned its pointing.

Learn more about how DSOC will be used to test high-bandwidth data transmission beyond the Moon for the first time – and how it could transform deep space exploration. Credit: NASA/JPL-Caltech/ASU

“Achieving first light is one of many critical DSOC milestones in the coming months, paving the way toward higher-data-rate communications capable of sending scientific information, high-definition imagery, and streaming video in support of humanity’s next giant leap: sending humans to Mars,” said Trudy Kortes, director of Technology Demonstrations at NASA Headquarters in Washington.

Test data also was sent simultaneously via the uplink and downlink lasers, a procedure known as “closing the link” that is a primary objective for the experiment. While the technology demonstration isn’t transmitting Psyche mission data, it works closely with the Psyche mission-support team to ensure DSOC operations don’t interfere with those of the spacecraft.

“Tuesday morning’stest was the first to fully incorporate the ground assets and flight transceiver, requiring the DSOC and Psyche operations teams to work in tandem,” said Meera Srinivasan, operations lead for DSOC at JPL. “It was a formidable challenge, and we have a lot more work to do, but for a short time, we were able to transmit, receive, and decode some data.”

Before this achievement, the project needed to check the boxes on several other milestones, from removing the protective cover for the flight laser transceiver to powering up the instrument. Meanwhile, the Psyche spacecraft is carrying out its own checkouts, including powering up its propulsion systems and testing instruments that will be used to study the asteroid Psyche when it arrives there in 2028.

First Light and First Bits

With successful first light, the DSOC team will now work on refining the systems that control the pointing of the downlink laser aboard the transceiver. Once achieved, the project can begin its demonstration of maintaining high-bandwidth data transmission from the transceiver to Palomar at various distances from Earth. This data takes the form of bits (the smallest units of data a computer can process) encoded in the laser’s photons – quantum particles of light. After a special superconducting high-efficiency detector array detects the photons, new signal-processing techniques are used to extract the data from the single photons that arrive at the Hale Telescope.

The DSOC experiment aims to demonstrate data transmission rates 10 to 100 times greater than the state-of-the-art radio frequency systems used by spacecraft today. Both radio and near-infrared laser communications utilize electromagnetic waves to transmit data, but near-infrared light packs the data into significantly tighter waves, enabling ground stations to receive more data. This will help future human and robotic exploration missions and support higher-resolution science instruments.

The flight laser transceiver operations team
The flight laser transceiver operations team for NASA’s Deep Space Optical Communications (DSOC) technology demonstration works in the Psyche mission support area at JPL in the early hours of Nov. 14, when the project achieved “first light.”
NASA/JPL-Caltech
DSOC ground laser transmitter operators pose for a photo at the Optical Communications Telescope Laboratory at JPL’s Table Mountain Facility near Wrightwood, California, shortly after the technology demonstration achieved “first light” on Nov. 14.
NASA/JPL-Caltech

“Optical communication is a boon for scientists and researchers who always want more from their space missions, and will enable human exploration of deep space,” said Dr. Jason Mitchell, director of the Advanced Communications and Navigation Technologies Division within NASA’s Space Communications and Navigation (SCaN) program. “More data means more discoveries.”

While optical communication has been demonstrated in low Earth orbit and out to the Moon, DSOC is the first test in deep space. Like using a laser pointer to track a moving dime from a mile away, aiming a laser beam over millions of miles requires extremely precise “pointing.”

The demonstration also needs to compensate for the time it takes for light to travel from the spacecraft to Earth over vast distances: At Psyche’s farthest distance from our planet, DSOC’s near-infrared photons will take about 20 minutes to travel back (they took about 50 seconds to travel from Psyche to Earth during the Nov. 14 test). In that time, both spacecraft and planet will have moved, so the uplink and downlink lasers need to adjust for the change in location.

“Achieving first light is a tremendous achievement. The ground systems successfully detected the deep space laser photons from DSOC’s flight transceiver aboard Psyche,” said Abi Biswas, project technologist for DSOC at JPL. “And we were also able to send some data, meaning we were able to exchange ‘bits of light’ from and to deep space.”

More About the Mission

DSOC is the latest in a series of optical communication demonstrations funded by NASA’s Space Technology Mission Directorate and the Space Communications and Navigation (SCaN) program within the agency’s Space Operations Mission Directorate.

The Psyche mission is led by Arizona State University. JPL is responsible for the mission’s overall management, system engineering, integration and test, and mission operations. Psyche is the 14th mission selected as part of NASA’s Discovery Program under the Science Mission Directorate, managed by the agency’s Marshall Space Flight Center in Huntsville, Alabama. NASA’s Launch Services Program, based at the agency’s Kennedy Space Center, managed the launch service. Maxar Technologies in Palo Alto, California, provided the high-power solar electric propulsion spacecraft chassis.

For more information about DSOC, visit:

https://www.jpl.nasa.gov/missions/dsoc

News Media Contact

Ian J. O’Neill
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-2649
ian.j.oneill@jpl.nasa.gov

2023-171

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Anthony Greicius

55 Years Ago: Eight Months Before the Moon Landing

55 Years Ago: Eight Months Before the Moon Landing

November 1968 proved pivotal to achieving the goal of landing a man on the Moon before the end of the decade. The highly successful Apollo 7 mission that returned American astronauts to space provided the confidence for NASA to decide to send the next flight, Apollo 8, on a trip to orbit the Moon in December. At NASA’s Kennedy Space Center (KSC) in Florida, the Saturn V rocket and the Apollo spacecraft for that mission sat on Launch Pad 39A undergoing tests for its upcoming launch. In the nearby Vehicle Assembly Building (VAB), the three stages of the Saturn V for the Apollo 9 mission sat stacked awaiting the addition of its spacecraft undergoing final testing. Also in the VAB, workers had begun stacking the Apollo 10 Saturn V, while the Apollo 10 spacecraft arrived for testing. As the Apollo 8 and 9 crews continued their training, NASA named the crew for Apollo 10 and announced the science experiments that the first Moon landing astronauts would deploy.

Image of President Lyndon B. Johnson, second from left, presents Apollo 7 astronauts Walter M. Schirra, left, Donn F. Eisele, and R. Walter Cunningham with Exceptional Service Medals at the LBJ Ranch Entertainer Bob Hope, second from right, taped an episode of his show at the Manned Spacecraft Center, now NASA’s Johnson Space Center in Houston, with guests the “Voice of Mission Control” Paul P. Haney, left, Apollo 7 astronauts Schirra, Cunningham, and Eisele, and television star Barbara Eden The Apollo 7 Command Module on display at the Frontiers of Flight Museum at Dallas Love Field
Left: President Lyndon B. Johnson, second from left, presents Apollo 7 astronauts Walter M. Schirra, left, Donn F. Eisele, and R. Walter Cunningham with Exceptional Service Medals at the LBJ Ranch. Middle: Entertainer Bob Hope, second from right, taped an episode of his show at the Manned Spacecraft Center, now NASA’s Johnson Space Center in Houston, with guests the “Voice of Mission Control” Paul P. Haney, left, Apollo 7 astronauts Schirra, Cunningham, and Eisele, and television star Barbara Eden. Right: The Apollo 7 Command Module on display at the Frontiers of Flight Museum at Dallas Love Field.

Following their highly successful flight, Apollo 7 astronauts Walter M. Schirra, Donn F. Eisele, and R. Walter Cunningham returned to Houston’s Ellington Air Force Base on Oct. 26. On Nov. 2, President Lyndon B. Johnson presented the astronauts with Exceptional Service Medals at the LBJ Ranch in Johnson City, Texas. Four days later, comedian Bob Hope filmed an episode of his weekly television variety show in the auditorium of the Manned Spacecraft Center (MSC), now the Johnson Space Center in Houston. Hope saluted the Apollo 7 astronauts in a skit that included actress Barbara Eden, star of the television series “I Dream of Jeannie” that featured fictional astronauts. Paul P. Haney, MSC Director of Public Affairs and the “Voice of Mission Control,” also participated in the skit. Following the recovery of Apollo 7, the prime recovery ship U.S.S. Essex sailed for Norfolk Naval Air Station in Virginia, where on Oct. 27 workers offloaded the Command Module (CM), and placed it aboard a cargo plane to fly it to California for return to its manufacturer, North American Rockwell Space Division in Downey, for postflight inspection. On Jan. 20, 1969, the Apollo 7 astronauts as well as their spacecraft took part in President Richard M. Nixon’s first inauguration parade. In 1970, NASA transferred the Apollo 7 spacecraft to the Smithsonian Institution that loaned it to the National Museum of Science and Technology in Ottawa, Canada, for display. Following its return to the United States in 2004, it went on display at the Frontiers of Flight Museum at Love Field in Dallas.

Image of the circumlunar trajectory of Apollo 8 Apollo 8 astronauts William A. Anders, left, James A. Lovell, and Frank Borman during a press conference shortly after the announcement of their mission to orbit the Moon Photo of Anders, left, Lovell, and Borman in the Command Module simulator
Left: The circumlunar trajectory of Apollo 8. Middle: Apollo 8 astronauts William A. Anders, left, James A. Lovell, and Frank Borman during a press conference shortly after the announcement of their mission to orbit the Moon. Right: Anders, left, Lovell, and Borman in the Command Module simulator.

On Nov. 12, 1968, NASA Headquarters put out the following statement: “The National Aeronautics and Space Administration today announced that the Apollo 8 mission would be prepared for an orbital flight around the Moon.” That momentous statement ended weeks of intense internal agency deliberations and public speculation about Apollo 8’s targeted mission. The original mission plan called for Apollo 8 to conduct the first test of the Lunar Module (LM) in Earth orbit, but when the LM fell behind schedule, NASA managers in August began contemplating sending the Apollo 8 crew on a lunar orbital test of the Command Module (CM). The decision hinged partly on a successful Apollo 7 mission, and with that milestone passed, NASA Administrator James E. Webb approved the daring plan. On only the second crewed Apollo mission, the first crew to launch on the Saturn V, and only the third launch of the mighty Moon rocket, with the second of those experiencing some serious anomalies, the decision weighed the risks against the benefits of achieving the Moon landing goal before the end of the decade. With the Dec. 21 launch date fast approaching, the Apollo 8 crew of Frank Borman, James A. Lovell, and William A. Anders and their backups Neil A. Armstrong, Edwin E. “Buzz” Aldrin, and Fred W. Haise had begun training for the lunar mission even before the official announcement. During a Nov. 16 press conference, Borman, Lovell, and Anders discussed their preparations for the historic mission. On Nov. 19, at KSC’s Launch Complex 39, engineers completed the Flight Readiness Test to validate the launch vehicle, spacecraft, and ground systems.

Photo of The Apollo 9 prime crew of James A. McDivitt, left, David R. Scott, and Russell L. Schweickart, not pictured, prepares for an altitude chamber test of their Command Module (CM) in the Manned Spacecraft Operations Building at NASA’s Kennedy Space Center in Florida Photo of McDivitt, emerging from the CM, Schweickart, at left in the raft, and Scott complete water egress training in the Gulf of Mexico Photo of The Apollo 9 backup crew of Charles “Pete” Conrad, left, Richard F. Gordon, and Alan L. Bean prepares for their water egress training
Left: The Apollo 9 prime crew of James A. McDivitt, left, David R. Scott, and Russell L. Schweickart, not pictured, prepares for an altitude chamber test of their Command Module (CM) in the Manned Spacecraft Operations Building at NASA’s Kennedy Space Center in Florida. Middle: McDivitt, emerging from the CM, Schweickart, at left in the raft, and Scott complete water egress training in the Gulf of Mexico. Right: The Apollo 9 backup crew of Charles “Pete” Conrad, left, Richard F. Gordon, and Alan L. Bean prepares for their water egress training.

The LM formed a critical component to the Moon landing effort. Delays in preparing LM-3 for flight resulted in the crewed test to slip to Apollo 9 in early 1969. The three stages of the Apollo 9 Saturn V stood stacked on Mobile Launcher 2 in High Bay 3 of the VAB. The Apollo 9 spacecraft components, CSM-104 and LM-3, continued testing in the KSC’s Manned Spacecraft Operations Building (MSOB). The prime crew of James A. McDivitt, David R. Scott, and Russell L. Schweickart, as well as their backups Charles “Pete” Conrad, Richard F. Gordon, and Alan L. Bean completed several altitude chamber tests with CSM-104 during the month of November. On Nov. 30, workers placed LM-3 inside its Spacecraft LM Adapter, topping it with CSM-104 to complete the spacecraft for its Dec. 3 rollover to the VAB for mating with the Saturn V. McDivitt, Scott, and Schweickart conducted water egress training in the Gulf of Mexico near Galveston, Texas. On Nov. 25, workers aboard the Motor Vessel M/V Retriever lowered a mockup CM with the crew inside into the water in a nose-down position. Flotation bags inflated to right the spacecraft to a nose-up position. The astronauts then exited the capsule onto life rafts and recovery personnel hoisted them aboard a helicopter. Backups Conrad, Gordon, and Bean completed the test on Dec. 6.

Photo of The Apollo 10 prime crew of Eugene A. Cernan, left, John W. Young, and Thomas P. Stafford Photo of the Apollo 10 backup crew of L. Gordon Cooper, Edgar D. Mitchell, and Donn F. Eisele
Left: The Apollo 10 prime crew of Eugene A. Cernan, left, John W. Young, and Thomas P. Stafford. Right: The Apollo 10 backup crew of L. Gordon Cooper, Edgar D. Mitchell, and Donn F. Eisele.

On Nov. 13, NASA announced the crew for the Apollo 10 mission planned for the spring of 1969. The fourth crewed Apollo mission would involve the launch of a CM and LM on a Saturn V rocket. Depending on the success of earlier missions, Apollo 10 planned to test the CM and LM either in Earth orbit or in lunar orbit, the latter a dress rehearsal for the actual Moon landing likely to follow on Apollo 11. NASA designated Thomas P. Stafford, John W. Young, and Eugene A. Cernan as the prime crew, the first all-veteran three person crew. The trio had served as the backup crew on Apollo 7 and had flight experience in the Gemini program. As backups, NASA assigned L. Gordon Cooper, Donn F. Eisele, and Edgar D. Mitchell. Cooper had flown previously on Mercury 9 and Gemini VIII, Eisele had just returned from Apollo 7, while this marked the first crew assignment for Mitchell. As support crew members, NASA named Joe H. Engle, James B. Irwin, and Charles M. Duke.

Photo of the Apollo 10 Command Module, left, and Service Module arrive at NASA’s Kennedy Space Center (KSC) in Florida Photo of the Apollo 10 S-IC first stage arrives at KSC’s Vehicle Assembly Building (VAB). Workers in the VAB stack the Apollo 10 first stage on its Mobile Launcher
Left: The Apollo 10 Command Module, left, and Service Module arrive at NASA’s Kennedy Space Center (KSC) in Florida. Middle: The Apollo 10 S-IC first stage arrives at KSC’s Vehicle Assembly Building (VAB). Right: Workers in the VAB stack the Apollo 10 first stage on its Mobile Launcher.

Flight hardware in support of Apollo 10 continued to arrive at KSC. Following delivery of LM-4 in October, on Nov. 2 workers mated its two stages and placed the vehicle in one of the MSOB’s altitude chambers. Stafford and Cernan carried out a sea level run on Nov. 22. The CM-106 and SM-106 for Apollo 10 arrived at KSC on Nov. 23 and workers trucked them to the MSOB where they mated the two modules three days later. In the VAB, the Saturn V’s S-IC first stage arrived on Nov. 27 and workers erected it on Mobile Launcher 3 in High Bay 2, awaiting the arrival of the upper stages.

A mockup of the laser ranging retroreflector (LRRR) experiment A mockup of the passive seismic experiment package (PSEP) A mockup of the solar wind composition (SWC) experiment A suited technician deploys mockups of the Apollo 11 experiments – the SWC, far left, the PSEP, and the LRRR, during a test session
Left: A mockup of the laser ranging retroreflector (LRRR) experiment. Middle left: A mockup of the passive seismic experiment package (PSEP). Middle right: A mockup of the solar wind composition (SWC) experiment. Right: A suited technician deploys mockups of the Apollo 11 experiments – the SWC, far left, the PSEP, and the LRRR, during a test session.

On Nov. 19, NASA announced that when Apollo astronauts first land on the Moon, possibly as early as during the Apollo 11 mission in the summer of 1969, they would deploy three scientific experiments – a passive seismometer experiment package (PSEP), a laser ranging retro-reflector (LRRR), and a solar wind composition (SWC) experiment – during their 2.5-hour excursion on the lunar surface. The PSEP will provide information about the Moon’s interior by recording any seismic activity. The passive LRRR consists of an array of precision optical reflectors that serve as a target for Earth-based lasers for highly precise measurements of the Earth-Moon distance. The SWC consists of a sheet of aluminum foil that the astronauts deploy at the beginning of their spacewalk and retrieve at the end for postflight analysis. During the exposure, the foil traps particles of the solar wind, especially noble gases.

The Lunar Module Test Article-8 (LTA-8) inside Chamber B of the Space Environment Simulation Laboratory (SESL) at the Manned Spacecraft Center, now NASA’s Johnson Space Center in Houston Astronaut James B. Irwin inside LTA-8 during one of the altitude runs Workers remove LTA-8 from SESL’s Chamber B at the conclusion of the altitude tests
Left: The Lunar Module Test Article-8 (LTA-8) inside Chamber B of the Space Environment Simulation Laboratory (SESL) at the Manned Spacecraft Center, now NASA’s Johnson Space Center in Houston. Middle: Astronaut James B. Irwin inside LTA-8 during one of the altitude runs. Right: Workers remove LTA-8 from SESL’s Chamber B at the conclusion of the altitude tests.

On Nov. 14, engineers in MSC’s Space Environment Simulation Laboratory (SESL) completed a series of altitude tests with LM Test Article-8 (LTA-8) to certify the vehicle for lunar missions. Astronaut Irwin and Grumman Aircraft Corporation consulting pilot Gerald P. Gibbons completed the final test, the last in a series of five that started on Oct. 14. Grumman pilot Glennon M. Kingsley paired up with Gibbons for three of the tests. During the tests that simulated various portions of the LM’s flight profile, the chamber maintained a vacuum simulating an altitude of about 150 miles and temperatures as low as -300o F. Strip heaters attached to the LTA’s surface provided the simulated solar heat. NASA transferred the LTA-8 to the Smithsonian Institution in 1978 and it is now on public display at Space Center Houston.

Depiction of Zond 6’s circumlunar trajectory
Depiction of Zond 6’s circumlunar trajectory. Image credit: courtesy RKK Energia.

A Proton rocket with a Zond spacecraft on the launch pad at the Baikonur Cosmodrome Zond 6 photographed the Earth as it looped around the Moon
Left: A Proton rocket with a Zond spacecraft on the launch pad at the Baikonur Cosmodrome. Right: Zond 6 photographed the Earth as it looped around the Moon. Image credits: courtesy RKK Energia.

Depiction of Zond 6’s skip reentry trajectory flown
Depiction of Zond 6’s skip reentry trajectory flown. Image credit: courtesy RKK Energia.

In another reminder that the race to the Moon still existed, on Nov. 10 the Soviet Union launched the Zond 6 spacecraft. Although it launched uncrewed, the Zond spacecraft, essentially a Soyuz without the forward orbital compartment and modified for flights to lunar distances, could carry a crew of two cosmonauts. A cadre of cosmonauts trained for such missions. Similar to the Zond 5 mission in September, Zond 6 entered a trajectory that looped it around the Moon on Nov. 13, passing within 1,500 miles of the lunar surface. The spacecraft took photographs of the Moon’s near and far sides and of the distant Earth. As it neared Earth during its return journey, trouble developed aboard the spacecraft as a faulty hatch seal caused a slow leak and it began to lose atmospheric pressure. Ground controllers initially steadied the pressure loss and performed a final midcourse maneuver that allowed Zond 6 to perform a skip reentry to land in Soviet territory on Nov. 17. However, the spacecraft continued to lose pressure and a buildup of static electricity created a coronal discharge that triggered the spacecraft’s soft landing rockets to fire and cut the parachute lines while it was still descending through 5,300 meters altitude. Although the capsule hit the ground at a high velocity, rescue forces were able to recover the film containers. The Soviets at the time did not reveal either the depressurization or the crash but claimed the flight was a successful circumlunar mission. With two apparently successful uncrewed circumlunar flights and the resumption of crewed missions with Soyuz 3 in October, these Soviet activities perhaps played a part in the decision to send Apollo 8 to the Moon.

News from around the world in November 1968:

Nov. 5 – Richard M. Nixon elected as the 37th U.S. President.

Nov. 5 – Shirley A. Chisolm of Brooklyn, New York, becomes the first African American woman elected to the U.S. Congress.

Nov 8 – The United States launches Pioneer 9 into solar orbit to monitor solar storms that could be harmful to Apollo astronauts traveling to the Moon.

Nov. 13 – The HL-10 lifting body aircraft with NASA pilot John A. Manke at the controls made its first successful powered flight after being dropped from a B-52 bomber at Edwards Air Force Base in California’s Mojave Desert.

Nov. 14 – Yale University announces it is going co-ed beginning in the 1969-1970 academic year.

Nov. 22 – The Beatles release the “The Beatles” (better known as the White Album), the band’s only double album.

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50 Years Ago: Launch of Skylab 4, The Final Mission to Skylab

50 Years Ago: Launch of Skylab 4, The Final Mission to Skylab

The third and final crewed mission to the Skylab space station, Skylab 4, got underway on Nov. 16, 1973, with a thunderous launch from NASA’s Kennedy Space Center (KSC) in Florida. Docking eight hours later, astronauts Gerald P. Carr, Edward G. Gibson, and William R. Pogue began a planned 56-day mission that program managers extended to a record-breaking 84 days. During their first month, as they adjusted to weightlessness and their new surroundings, they completed the first of four spacewalks. They began an extensive science program, investigating the effects of long-duration spaceflight on human physiology, examining the Sun, conducting observations of the Earth, as well as technology and student-led experiments. They began their systematic observations of recently discovered Comet Kohoutek as it approached the Sun.

Crew patch of the third and final crewed mission to Skylab Photo of the Skylab 4 crew of Gerald P. Carr, Edward G. Gibson, and William R. Pogue Photo of the Skylab 4 backup crew of Vance D. Brand, left, William B. Lenoir, and Don L. Lind
Left: Crew patch of the third and final crewed mission to Skylab. Middle: Official photo of the Skylab 4 crew of Gerald P. Carr, left, Edward G. Gibson, and William R. Pogue. Right: The Skylab 4 backup crew of Vance D. Brand, left, William B. Lenoir, and Don L. Lind.

In January 1972, NASA announced the astronauts it had selected for the Skylab program. For Skylab 4, the third crewed mission and at the time planned to last 56 days, NASA named Carr as commander, Gibson as science pilot, and Pogue as pilot to serve as the prime crew, the first all-rookie prime crew since Gemini VIII in 1966. For the backup crew, NASA designated Vance D. Brand, William B. Lenoir, and Don L. Lind, who also served as the backup crew for Skylab 3. Brand and Lind would serve as the two-person crew for a possible rescue mission.

The S-IB first stage for the Skylab 4 mission’s SA-208 Saturn IB rocket arrives at the Vehicle Assembly Building (VAB) at NASA’s Kennedy Space Center in Florida The two S-IVB second stages for the Skylab 4 SA-208 rocket, right, and the SA-209 Skylab rescue rocket sit side by side in the VAB Image of workers in the VAB stack the second stage onto the first stage for the Skylab 4 Saturn IB
Left: The S-IB first stage for the Skylab 4 mission’s SA-208 Saturn IB rocket arrives at the Vehicle Assembly Building (VAB) at NASA’s Kennedy Space Center in Florida. Middle: The two S-IVB second stages for the Skylab 4 SA-208 rocket, right, and the SA-209 Skylab rescue rocket sit side by side in the VAB. Right: Workers in the VAB stack the second stage onto the first stage for the Skylab 4 Saturn IB.

Preparations at KSC for the Skylab 4 mission began on Nov. 4, 1971, with the arrival of the S-IVB second stage of the SA-208 Saturn IB rocket. Workers placed it in long-term storage in the Vehicle Assembly Building (VAB). The rocket’s S-IB first stage arrived on June 20, 1973. Workers in the VAB mounted it on Mobile Launcher 1 on July 31, adding the second stage later that same day.

Photo of the arrival of the Skylab 4 Command Module (CM), front, and Service Module, partly hidden at left, in the Manned Spacecraft Operations Building (MSOB) at NASA’s Kennedy Space Center in Florida Photo of Skylab 4 astronauts conduct an altitude test aboard their CM in the MSOB Photo of the rollout of the Skylab 4 vehicle from the Vehicle Assembly Building to Launch Pad 39B Photo of workers at Launch Pad 39B replace the eight stabilization fins on the Saturn IB rocket’s first stage
Left: The arrival of the Skylab 4 Command Module (CM), front, and Service Module, partly hidden at left, in the Manned Spacecraft Operations Building (MSOB) at NASA’s Kennedy Space Center in Florida. Middle left: The Skylab 4 astronauts conduct an altitude test aboard their CM in the MSOB. Middle right: Rollout of the Skylab 4 vehicle from the Vehicle Assembly Building to Launch Pad 39B. Right: Workers at Launch Pad 39B replace the eight stabilization fins on the Saturn IB rocket’s first stage.

Meanwhile, Command and Service Module-118 (CSM-118) for the mission arrived in KSC’s Manned Spacecraft and Operations Building (MSOB) on Feb. 10, 1973, where engineers placed it inside a vacuum chamber. The prime and backup crews conducted altitude tests of the CSM in early August. With the thruster problems aboard the Skylab 3 spacecraft docked to the space station, managers accelerated the processing flow for the Skylab 4 vehicle to enable a launch as early as Sept. 9 in case they had to implement a rescue mission. Workers mated CSM-118 to the Saturn rocket on Aug. 10 and rolled the stack to Launch Pad 39B four days later. By this time, the need for a rescue had diminished and the processing flow readjusted to enable a launch on need within nine days until the Skylab 3 splashdown on Sept. 25. Normal processing then resumed for a planned Nov. 9 launch, later adjusted to Nov. 11. Carr, Gibson, and Pogue entered their preflight health stabilization plan quarantine on Oct. 20. On Nov. 6, workers found hairline cracks in the mounting brackets of the Saturn IB’s stabilizing fins, requiring a slip of the launch date to Nov. 16 to complete their replacement at the pad. The Skylab 4 countdown began on Nov. 14, the day after the astronauts arrived at KSC.

Photo of Skylab 4 astronauts William R. Pogue, left, Edward G. Gibson, and Gerald P. Carr training in the Skylab training mockup Photo of Gibson, left, Carr, and Pogue display a model of the Skylab space station at the conclusion of their preflight press conference Photo of Gibson, left, Carr, and Pogue pose in front of a T-38 Talon aircraft at Ellington Air Force Base in Houston prior to their departure for NASA’s Kennedy Space Center in Florida for the launch
Left: Skylab 4 astronauts William R. Pogue, left, Edward G. Gibson, and Gerald P. Carr training in the Skylab training mockup. Middle: Gibson, left, Carr, and Pogue display a model of the Skylab space station at the conclusion of their preflight press conference. Right: Gibson, left, Carr, and Pogue pose in front of a T-38 Talon aircraft at Ellington Air Force Base in Houston prior to their departure for NASA’s Kennedy Space Center in Florida for the launch.

Photo of Skylab 4 astronauts William R. Pogue, left, Edward G. Gibson, and Gerald P. Carr enjoy the traditional prelaunch breakfast Carr, Gibson, and Pogue test the pressure integrity of their spacesuits before launch Photo of Carr, front, Gibson, and Pogue exit crew quarters to board the transfer van for the ride to Launch Pad 39B
Left: Skylab 4 astronauts William R. Pogue, left, Edward G. Gibson, and Gerald P. Carr enjoy the traditional prelaunch breakfast. Middle: Carr, front, Gibson, and Pogue test the pressure integrity of their spacesuits before launch. Right: Carr, front, Gibson, and Pogue exit crew quarters to board the transfer van for the ride to Launch Pad 39B.

Liftoff of Skylab 4
Liftoff of Skylab 4!

The third and final mission to the Skylab space station got underway on Nov. 16, 1973, with a thunderous liftoff from KSC’s Launch Pad 39B. Although officially planned as a 56-day mission for several years, mission managers had confidence of an extension to 84 days and planned accordingly, with the astronauts bringing additional food, supplies, and science experiments.

Photo of Skylab during the rendezvous and docking Three astronaut manikins wear the Skylab 4 crew’s flight overalls
Left: Skylab during the rendezvous and docking. Right: Left by the Skylab 3 crew before their departure from the station, three astronaut manikins wear the Skylab 4 crew’s flight overalls.

Eight hours after launch, and following two unsuccessful attempts, Carr hard docked the spacecraft to the space station. Pogue, who on Earth appeared resistant to all forms of motion sickness, developed a case of space motion sickness during the crew’s first evening, requiring several days to fully recover. This incident along with an overly packed timeline caused the astronauts to fall behind in accomplishing their tasks as they adjusted to weightlessness and learned their way around the large space station. The astronauts spent their first night in space aboard the Command Module, opening the hatch the next morning to begin reactivating Skylab. To their surprise, the station appeared to already have three occupants. As a joke, before they left the station in September, the Skylab 3 crew stuffed their successors’ flight suits with used clothing and left them in strategic places throughout the workshop. Carr, Gibson, and Pogue began settling into the routine aboard Skylab, preparing meals, exercising, and starting the large number of experiments. They continued the science program begun by the previous two Skylab crews, including biomedical investigations on the effects of long-duration space flight on the human body, Earth observations using the Earth Resources Experiment Package (EREP), and solar observations with instruments mounted on the Apollo Telescope Mount (ATM). With the prediction earlier in the year that newly discovered Comet Kohoutek would make its closest approach to the Sun in late December, scientists added cometary observations to the crew’s already busy schedule. The astronauts brought a Far Ultraviolet Electronographic Camera, the backup to the instrument deployed on the Moon during Apollo 16, to Skylab especially for observations of the comet, and used it for cometary photography during two spacewalks added to the mission.

Photo of Edward G. Gibson, left, William R. Pogue, and Gerald P. Carr prepare a meal in the Skylab wardroom Photo of Carr using the Thornton treadmill to exercise Carr “weighs” himself in weightlessness using the body mass measurement device
Left: Edward G. Gibson, left, William R. Pogue, and Gerald P. Carr prepare a meal in the Skylab wardroom. Middle: Carr uses the Thornton treadmill to exercise. Right: Carr “weighs” himself in weightlessness using the body mass measurement device.

One of the lessons learned from the first two Skylab missions indicated that the onboard bicycle ergometer alone did not provide enough exercise to maintain leg and back muscle mass and strength. To remedy this problem, physician and Skylab support astronaut Dr. William E. Thornton designed a makeshift treadmill that the third crew brought with them to the station. The treadmill device consisted of a teflon-coated aluminum plate bolted to the floor of the workshop. Bungee cords attached to the floor and to the ergometer harness supplied the downward force for the back and leg muscles with the astronauts sliding over the teflon-coated plate while walking or jogging in stocking feet. Because the exercise provided quite a strenuous workout, the crew dubbed it “Thornton’s revenge.” They also increased the overall amount of time they spent exercising.

Photo of William R. Pogue replaces film in the Apollo Telescope Mount during the mission’s first spacewalk Gerald P. Carr flies the Astronaut Maneuvering Unit Overall view showing the large volume of the Skylab Orbital Workshop
Left: William R. Pogue replaces film in the Apollo Telescope Mount during the mission’s first spacewalk. Middle: Gerald P. Carr flies the Astronaut Maneuvering Unit. Right: Overall view showing the large volume of the Skylab Orbital Workshop.

In addition to the heavy science experiment load, the astronauts spent the first week in orbit preparing for the first spacewalk of the mission. On Nov. 22, their seventh day in space and also Thanksgiving Day, Gibson and Pogue suited up and stepped outside the space station with Gibson exclaiming, “Boy, if this isn’t the great outdoors.” During this six-hour 33-minute spacewalk, they replaced film canisters in the ATM and deployed an experiment package on the ATM truss. They took photographs with a camera that had originally been intended for the airlock now blocked by the sunshade that the first crew deployed in May to help cool the station. Gibson and Pogue accomplished all the tasks planned for this first spacewalk. Back inside the station, the astronauts settled in for the first Thanksgiving meal in space. For their dinner, Carr selected prime rib, Gibson went with traditional turkey, and Pogue chose chicken.

The S-IB first stage for Saturn-IB SA-209, the Skylab 4 rescue mission, arrives at the Vehicle Assembly Building (VAB) at NASA’s Kennedy Space Center Photo of the S-IVB second stage for SA-209 inside the VAB Workers stack the Command and Service Module CSM-119, the Skylab 4 rescue spacecraft, atop SA-209 Image of the Skylab 4 rescue vehicle at Launch Pad 39B
Left: The S-IB first stage for Saturn-IB SA-209, the Skylab 4 rescue mission, arrives at the Vehicle Assembly Building (VAB) at NASA’s Kennedy Space Center. Middle left: The S-IVB second stage for SA-209 inside the VAB. Middle right: Workers stack the Command and Service Module CSM-119, the Skylab 4 rescue spacecraft, atop SA-209. Right: The Skylab 4 rescue vehicle at Launch Pad 39B.

The inclusion of two docking ports on the Skylab space station enabled an in-flight rescue capability for the first time in human spaceflight history. In case a failure of the docked CSM stranded the onboard three-person crew, a two-person crew would launch in a second Apollo spacecraft specially configured with two extra couches to return all five astronauts. For the first two Skylab missions, the rocket and spacecraft for the subsequent mission served as the potential rescue vehicle. The failure of two Service Module thruster groups during Skylab 3 nearly required the rescue capability. Since Skylab 4 was the final mission, NASA procured an additional Saturn IB rocket, SA-209, and Apollo spacecraft, CSM-119, for the rescue role. The spacecraft arrived at KSC on May 2, 1973, and workers placed it in storage in the MSOB. In September, the backup crew of Brand, Lenoir, and Lind completed altitude chamber tests with the CSM, although only Brand and Lenoir would fly any the rescue mission. The S-IVB second stage for Saturn IB SA-209 arrived at KSC on Jan. 12, 1972, and workers placed it in storage in the VAB. The S-IB first stage arrived on Aug. 20, 1973. Because only one Mobile Launcher included the milkstool to launch a Saturn IB, assembly of the rescue vehicle had to await its return from the launch pad the day after the Skylab 4 liftoff. Assembly of the rocket in the VAB began on Nov. 26, and workers topped the rocket off with the spacecraft four days later. The stacked vehicle rolled out to Launch Pad 39B on Dec. 3 where engineers prepared the vehicle so that after Dec. 20, it could support a launch within nine days, should the need arise. The vehicle remained at the pad until Feb. 14, 1974, six days after the Skylab 4 splashdown.

Gerald P. Carr monitors Edward G. Gibson during a lower body negative pressure test of his cardiovascular system Gibson works out on the bicycle ergometer during a test of his cardiopulmonary function Gibson in the rotating chair to test his vestibular system
Left: Gerald P. Carr monitors Edward G. Gibson during a lower body negative pressure test of his cardiovascular system. Middle: Gibson works out on the bicycle ergometer during a test of his cardiopulmonary function. Right: Gibson in the rotating chair to test his vestibular system.

To add to their packed timeline, one of the station’s three control moment gyros (CMGs) failed the day after the first spacewalk. Skylab used CMGs to control the station’s attitude without expending precious attitude control gas, a non-renewable resource heavily depleted early in the station’s life. Engineers on the ground worked out a plan to control the station’s attitude using only the two working CMGs, thereby enabling completion of the remaining science, especially the Earth resource passes and comet Kohoutek observations. Pogue made the first measurements of Comet Kohoutek on Nov. 23 from inside the station using a photometric camera brought to Skylab especially to observe the comet. The astronauts practiced flying the Astronaut Maneuvering Unit, a precursor of the Manned Maneuvering Unit used during the space shuttle program to retrieve satellites, inside the large dome of the workshop.

Image of Edward G. Gibson at the controls of the Apollo Telescope Mount Image of William R. Pogue, left, and Gerald P. Carr at the control panel for the Earth Resources Experiment package inside the Multiple Docking Adapter
Left: Edward G. Gibson at the controls of the Apollo Telescope Mount. Right: William R. Pogue, left, and Gerald P. Carr at the control panel for the Earth Resources Experiment package inside the Multiple Docking Adapter.

Image of a massive solar flare taken by one of the Apollo Telescope Mount instruments Earth Resources Experiment Package photograph of the San Francisco Bay area Crew handheld photograph of a cyclone in the South Pacific
Left: Image of a massive solar flare taken by one of the Apollo Telescope Mount instruments. Middle: Earth Resources Experiment Package photograph of the San Francisco Bay area. Right: Crew handheld photograph of a cyclone in the South Pacific.

On Dec. 13, the mission’s 28th day, program officials assessed the astronauts’ performance and the status of the station and fully expected that they could complete the nominal 56-day mission and most likely the full 84 days. Despite being overworked and often behind the timeline, Carr, Gibson, and Pogue had already accomplished 84 hours of solar observations, 12 Earth resources passes, 80 photographic and visual Earth observations, all of the scheduled medical experiments, as well as numerous other activities such as student experiments, and science demonstrations. The astronaut’s major concern centered around the timelining process that had not given them time to adjust to their new environment and did not take into account their on-orbit daily routine. Despite the crew sending taped verbal messages to the ground asking for help in fixing these issues, the problem persisted. Skylab 4 Lead Flight Director Neil B. Hutchinson later admitted that the ground team learned many lessons about timelining long duration missions during the first few weeks of Skylab 4.

For more insight into the Skylab 4 mission, read Carr’s, Gibson’s, and Pogue’s oral histories with the JSC History Office.

To be continued …

With special thanks to Ed Hengeveld for his expert contributions on Skylab imagery.

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