University High Wins L.A. Ocean Sciences Bowl at NASA’s JPL

University High Wins L.A. Ocean Sciences Bowl at NASA’s JPL

2 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

The team from University High School in Irvine, California
The team from University High School in Irvine, California, proved victorious in the 2024 Los Angeles regional Ocean Sciences Bowl tournament at NASA’s Jet Propulsion Laboratory. From left: senior Julianne Wu, team captain and senior Maia Kopylova, sophomore Angelina Yan, sophomore Matthew Feng, senior Claudia Kahana, and team coach Ruby-Ann Lopez.
NASA/JPL-Caltech

The annual competition aims to help students expand their ocean-related knowledge outside the classroom and to become environmental stewards.

University High School of Irvine, California, emerged victorious on Jan. 20 at the Los Angeles regional Ocean Sciences Bowl tournament, which NASA’s Jet Propulsion Laboratory has hosted annually since 2000.

Eight schools from Los Angeles and Orange counties competed, with Santa Monica High School taking second place and and Torrance High placing third.

“For me,” said University High senior Claudia Kahanka, “it’s less about winning and more about interacting with people who are my own age and who are interested in the same things as me. It’s wonderful.”

The student teams spend months studying and preparing for the fast-paced academic competition, with contestants tapping “Jeopardy!”-style buzzers before answering challenging questions on science and policy regarding Earth’s oceans.

“We have practices every week – two-hour practices,” said team captain Maia Kopylova, a senior at University High. “Each individual studies a specific topic. And then we come together on Discord or in person and practice.”

Teams of four to five students have just 5 seconds to answer multiple-choice “buzzer questions,” worth 4 points each, in one of eight categories: biology, chemistry, geography, geology, marine policy, physical oceanography, social sciences, and technology. If a student answers a question correctly, they receive a bonus question worth 6 points and have 20 seconds to consult with their teammates before the team captain must provide an answer. They also face a handful of “team challenge questions” in which they can work together for a longer period to come up with an answer.

The JPL event – called the Los Angeles Surf Bowl – was the first of nearly 20 regional Ocean Sciences Bowl competitions across the country. The tournaments are coordinated by the Center for Ocean Leadership, which is a program of the University Corporation for Atmospheric Research, an organization focused in part on Earth science-related education. The event at JPL is staffed by volunteers from the lab and University of Southern California, several of whom are competition alumni.

Melissa Pamer
Jet Propulsion Laboratory, Pasadena, Calif.
626-314-4928
melissa.pamer@jpl.nasa.gov

2024-004

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Jan 22, 2024

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Anthony Greicius

NASA Glenn’s Langley Legacy

NASA Glenn’s Langley Legacy

5 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Group of people posing in front of building.
Members of the AERL design team pose outside the Structures Laboratory at Langley in 1941. Many would later transfer to Cleveland later that year.
NASA

“[On December 15, 1941] a few shivering, startled Southerners from Langley, the vanguard of those in the Power Plants Division transferring to Cleveland, arrived in the biggest snowstorm in years,” recalled former receptionist Mary Louise Gosney. This vanguard was the first large group of NACA employees to relocate from the Langley Memorial Aeronautical Laboratory to the new Aircraft Engine Research Laboratory (AERL).  As construction of the AERL proceeded over the next two years, larger factions followed suit. Langley employees not only designed and constructed the AERL but formed the core of the Laboratory’s leadership and research staff for three decades.

For the newcomers, the mid-December snowstorm was a dramatic change from Virginia, where temperatures had reached 60 degrees Fahrenheit just days before. The challenge of acclimation to the northern climate, however, paled in comparison to the tumult resulting from Japan’s attack on Pearl Harbor and the Philippines just eight days before. The United States was now involved in World War II on two fronts, and there was a new urgency to get the NACA’s new engine research laboratory operational. The military was relying on the AERL to resolve a host of propulsion issues for its aircraft.

Nearly a year beforehand, in January 1941, Langley construction engineer Charles Herrmann had relocated to Cleveland with Helen Ford, an administrative assistant from NACA Headquarters.

From a 19th-century farmhouse on the barren AERL site, they managed the construction contracting and inspections. Meanwhile, in a room above Langley’s Structural Research Laboratory, a team of civil engineers designed the AERL’s test facilities and other structures. In August 1941, the NACA decided to transfer the Chief of Langley’s Construction Division, Edward Raymond Sharp, to Cleveland to expedite the work.

Women working at desks
Temporary offices constructed inside the hangar to house the architectural and drafting personnel as well the machines shops.
NASA/GRC

The Langley arrivals of December 1941, which included inspectors, engineers, draftsmen, mechanics, and administrative staff, were stationed in temporary offices inside the aircraft hangar—the only completed building. Sharp negotiated a key contract with a new construction company in the ensuing weeks that provided a breakthrough in the work. The first test facility was operational in May 1942. One after another, the other buildings and facilities were completed during the following year, and the former Langley staff left the hangar for their permanent offices.

In the fall of 1942, units of the Langley engine research staff began transferring to Cleveland. What had been modest-size sections in Langley’s Power Plants Division were expanded to full divisions in Cleveland. These divisions, led by experienced Langley engineers, included Addison Rothrock’s Fuels and Lubrication Division, Benjamin Pinkel’s Thermodynamics Division, Ernest Whitney’s Engine Installation Division, Charles Moore’s Engine Research Division, Oscar Schey’s Supercharger Division, and Joseph Vensel’s Flight Research Division.

Man standing by chalkboard with holiday message.
Ray Sharp in his in December 1946. He began his NACA career at Langley in 1922 and transferred to the Cleveland lab in August 1941.
NASA

In a somewhat surprising move, the NACA assigned construction manager Ray Sharp the responsibility for running the laboratory on a permanent basis. At Langley and Ames, technically skilled engineers performed that task. Sharp, who had a law degree but no formal scientific or engineering background, was assisted by Executive Engineers Carlton Kemper and Addison Rothrock. Sharp managed the day-to-day activities, while Rothrock and Kemper supervised the research. In 1949, Abe Silverstein, who had helped design and operate Langley’s Full Scale Wind Tunnel, became Chief of Research.

Although the AERL was continually hiring new researchers in the 1940s and 1950s, the ex-Langley personnel provided the laboratory’s backbone. With the arrival of the newcomers, more and more of the Langley veterans moved into the management ranks. Nearly all of the division chiefs and upper-management positions during the NACA era were occupied by former Langley people.

The relatively small size of the AERL staff and the fact that many of them were new to northeast Ohio resulted in a close community. Everyone knew nearly everyone else, families were started, and lifelong friendships formed. Sharp and his wife Vera were parental figures who looked after the employees and participated in the staff dances, sporting events, and other social activities.

Group sitting at table in cafeteria.
Members of the Old Timers Club, all former Langley employees, meet for their annual luncheon in March 1948. Back row, left to right: Harold Gerrish, Achilles Gellales, Clarence Decker, Carlton Kemper, Hampton Foster, William Dewey. Front row, left to right: Emery Gilbert, Charles Moore, Dale McConnaha, Addison Rothrock, Oscar Schey, Arthur Tesman.
NASA

The transition from the NACA to NASA in 1958 brought a number of changes to the organization, including the transfer of Silverstein and a number of other key Lewis employees to Headquarters and Langley’s Space Task Group. There was also a shift from the NACA’s mostly in-house research to NASA’s management of external development contracts. The new space agency also dramatically increased the size of its staff in the early 1960s. Silverstein, who replaced Sharp as Director in 1961, knew the importance of camaraderie and successfully encouraged the older NACA veterans to interact socially with the new recruits.

As NASA’s budgets decreased in the late 1960s and early 1970s, the era of Langley’s influence on Lewis came to a close. To reduce its payroll, NASA began to offer employees incentives to retire. The Langley expatriates—many of whom had over 30 years of service—ebbed away during the final years of the Apollo program. The Center struggled for nearly a decade to redefine itself and its culture.

Langley’s legacy is still visible at the Center today in its inductees into the Glenn Hall of Fame, a historic district containing the original facilities, and the campus’s lack of sidewalk plots or tree lawns. The Southerners had not anticipated the need to plow snow when designing the laboratory.

Robert S. Arrighi
NASA Glenn Research Center

This article originally appeared in NASA History News & Notes, Volume 33, Number 4, Fourth Quarter 2016.

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Robert S. Arrighi

Hubble Observes an Askew Galaxy Coaxing Star Formation from its Partner 

Hubble Observes an Askew Galaxy Coaxing Star Formation from its Partner 

2 min read

Hubble Observes an Askew Galaxy Coaxing Star Formation from its Partner 

This new NASA Hubble Space Telescope image features two interacting spiral galaxies collectively called Arp 300.
NASA, ESA, J. Dalcanton (University of Washington), and R. Windhorst (Arizona State University); Processing: Gladys Kober (NASA/Catholic University of America)

Arp 300 consists of two interacting galaxies, UGC 05028 (the smaller face-on spiral galaxy) and UGC 05029 (the larger face-on spiral). Likely due to its gravitational dance with its larger partner, UGC 05028 has an asymmetric, irregular structure, which is not as visible from ground-based telescopes but is quite distinct in this new image from NASA’s Hubble Space Telescope. The bright knot visible to the southeast of the center of UGC 05028 may be the remnant of another small galaxy that is in the process of merging with that galaxy. If this is the case, that remnant will eventually merge with the bar of stars visible in Hubble images of UGC 05028, forming a central bulge similar to that of Arp 300’s larger companion galaxy, UGC 05029.

UGC 05029 has a pronounced spiral structure and multiple hot, blue giant stars visible on the side facing UGC 05028. This enhanced star formation is likely due to the interaction between the two galaxies. Another edge-on spiral galaxy is visible in this image below UGC 05029 but is too faint to be resolved into star-forming regions, while the five objects strung out above it are probably a group of distant background galaxies.

Hubble looked at this galaxy pair to study the relationship between the overall physical characteristics of galaxies and their star formation.

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Media Contact:

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

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Jan 22, 2024
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Andrea Gianopoulos
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Four Ax-3 Astronauts Board Station and Meet Expedition 70 Crew

Four Ax-3 Astronauts Board Station and Meet Expedition 70 Crew

The four Axiom Mission 3 astronauts (front row) gather with the Expedition 70 crew inside the International Space Station's Harmony module. Credit: NASA TV
The four Axiom Mission 3 astronauts (front row) gather with the Expedition 70 crew inside the International Space Station’s Harmony module. Credit: NASA TV

Axiom Mission 3 (Ax-3) astronauts Michael López-Alegría, Walter Villadei, Marcus Wandt, and Alper Gezeravci are now aboard the International Space Station following Dragon’s hatch opening at 7:13 a.m. EST, Saturday, Jan. 20.

Ax-3 docked to the orbital complex at 5:42 a.m. while the spacecraft was flying 262 miles above the Pacific Ocean, west of South America. It is the third mission with an entirely private crew to arrive at the orbiting laboratory.

The Axiom Space crew are joining Expedition 70 crew members aboard station, including NASA astronauts Jasmin Moghbeli and Loral O’Hara, ESA (European Space Agency) astronaut Andreas Mogensen, JAXA (Japan Aerospace Exploration Agency) astronaut Furukawa Satoshi, and Roscosmos cosmonauts Konstantin Borisov, Oleg Kononenko, and Nikolai Chub.

Next up, the station crew members will take part in a welcome ceremony aboard the International Space Station.

Axiom Space astronauts are expected to depart the space station Feb. 3, pending weather, for a return to Earth and splashdown at a landing site off the coast of Florida.


Learn more about station activities by following the space station blog@space_station and @ISS_Research on X, as well as the ISS Facebook and ISS Instagram accounts.

Get weekly video highlights at: https://roundupreads.jsc.nasa.gov/videoupdate/

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Mark Garcia

Ax-3 Docks to Station Aboard Dragon Spacecraft

Ax-3 Docks to Station Aboard Dragon Spacecraft

The SpaceX Dragon Freedom spacecraft carrying four Axiom Mission 3 astronauts is pictured docked to the space station shortly after an orbital sunrise. Credit: NASA TV
The SpaceX Dragon Freedom spacecraft carrying four Axiom Mission 3 astronauts is pictured docked to the space station shortly after an orbital sunrise. Credit: NASA TV

Axiom Mission 3 astronauts Michael López-Alegría, Walter Villadei, Marcus Wandt, and Alper Gezeravci arrived at the International Space Station at 5:42 a.m. EST Saturday, Jan. 20. Dragon docked to the orbital complex while the spacecraft was flying about 262 miles over the Pacific Ocean, west of South America.

Live coverage continues on the NASA+ streaming service, NASA Television, the NASA app, and the agency’s website for hatch opening and crew remarks.


Learn more about station activities by following the space station blog@space_station and @ISS_Research on X, as well as the ISS Facebook and ISS Instagram accounts.

Get weekly video highlights at: https://roundupreads.jsc.nasa.gov/videoupdate/

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Mark Garcia