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Reentry of International Space Station (ISS) batteries into Earth’s atmosphere
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By NASA
ESA (European Space Agency) astronaut Samantha Cristoforetti pictured aboard the International Space Station on Dec. 20, 2014, during Expedition 42.Credit: NASA Crew members aboard the International Space Station celebrate the holiday season in a unique way while living and working at the orbiting laboratory. Each crew member, including the current Expedition 72, spends time enjoying the view of Earth from the space station, privately communicating with their friends and families, and sharing a joint meal with their expedition crewmates, while continuing experiments and station maintenance.
This view of the rising Earth greeted the Apollo 8 astronauts William Ander, Frank Borman, and James Lovell on Dec. 24, 1968, as they approached from behind the Moon after the fourth nearside lunar orbit.Credit: NASA As the first crew to spend Christmas in space and leave Earth orbit, Apollo 8 astronauts Frank Borman, James Lovell, and William Anders, celebrated while circling the Moon in December 1968. The crew commemorated Christmas Eve by reading opening verses from the Bible’s Book of Genesis as they broadcast scenes of the lunar surface below. An estimated one billion people across 64 countries tuned in to the crew’s broadcast.
Skylab 4 astronauts Gerald Carr, Edward Gibson, and William Pogue trim their homemade Christmas tree in December 1973. Credit: NASA In 1973, Skylab 4 astronauts Gerald Carr, Edward Gibson, and William Pogue celebrated Thanksgiving, Christmas, and New Year’s in space, as the first crew to spend the harvest festival and ring in the new year while in orbit. The crew built a homemade tree from leftover food containers, used colored decals as decorations, and topped it with a cardboard cutout in the shape of a comet. Carr and Pogue conducted a seven-hour spacewalk to change out film canisters and observe the passing Comet Kohoutek on Dec. 15, 1973. Once back inside the space station, the crew enjoyed a holiday dinner complete with fruitcake, communicated with their families, and opened presents.
NASA astronaut Jeffrey Hoffman pictured with a dreidel during Hanukkah in December 1993.Credit: NASA After NASA launched the agency’s Hubble Space Telescope into Earth’s orbit in 1990, NASA sent a space shuttle crew on a mission, STS-61, to service the telescope. In 1993, NASA astronaut Jeffrey Hoffman celebrated Hanukkah after completing the third spacewalk of the servicing mission. Hoffman celebrated with a traveling menorah and dreidel.
STS103-340-036 (19-27 December 1999) — Wearing Santa hats, astronauts John M. Grunsfeld and Steven L. Smith blend with the season for a brief celebration on the mid deck of the Space Shuttle Discovery. The interruption was very brief as the two mission specialists shortly went about completing their suit-up process in order to participate in STS-103 space walk activity, performing needed work on the Hubble Space Telescope (HST).Credit: NASA As NASA continued to support another Hubble Space Telescope servicing mission, the STS-103 crew celebrated the first space shuttle Christmas aboard Discovery in 1999. NASA astronauts Curtis Brown, Scott Kelly, Steven Smith, John Grunsfeld, and Michael Foale, along with ESA (European Space Agency) astronauts Jean-François Clervoy and Claude Nicollier enjoyed duck foie gras on Mexican tortillas, cassoulet, and salted pork with lentils. Smith and Grunsfeld completed repairs on the telescope during a spacewalk on Dec. 24, 1999, and at least one American astronaut has celebrated Christmas in space every year since.
Expedition 1 crew members Yuri Gidzenko of Roscosmos, left, NASA astronaut William Shepherd, and Sergei Krikalev of Roscosmos reading a Christmas message in December 2000.
Credit: NASA In November 2000, the arrival of Expedition 1 crew members, NASA astronaut William Shepherd and Roscosmos cosmonauts Yuri Gidzenko and Sergei Krikalev, aboard the International Space Station, marked the beginning of a continuous presence in space. As the first crew to celebrate the holiday season at the laboratorial outpost, they began the tradition of reading a goodwill message to those back on Earth. Shepherd honored a naval tradition of writing a poem as the first entry of the new year in the ship’s log.
For more than 24 years, NASA has supported a continuous U.S. human presence aboard the International Space Station, through which astronauts have learned to live and work in space for extended periods of time. As NASA supports missions to and from the station, crew members have continued to celebrate the holidays in space.
Expedition 4 crew members, NASA astronauts Daniel Bursch and Carl Walz, along with Roscosmos cosmonaut Yuri Onufriyenko, pose for a Christmas photo in December 2001. Credit: NASA Expedition 8 crew members, NASA astronaut Michael Foale, left, and Roscosmos cosmonaut Aleksandr Kaleri, right, celebrate Christmas in December 2003. Credit: NASA Expedition 10 crew members, Roscosmos cosmonaut Salizhan Sharipov, left, and NASA astronaut Leroy Chiao, right, celebrate New Year’s Eve in December 2004.Credit: NASA Expedition 12 crew members, Roscosmos cosmonaut Tokarev, left, and NASA astronaut William McArthur, pose with Christmas stockings in December 2005. NASA Expedition 14 crew members, Roscosmos cosmonaut Mikhail Tyurin, left, and NASA astronauts Michael Lopez-Alegria and Suni Williams pose wearing Santa hats in December 2006.Credit: NASA Expedition 16 crew members, Roscosmos cosmonaut Yuri Malenchenko, left, and NASA astronauts Peggy Whitson and Daniel Tani, with Christmas stockings and presents in December 2007. Expedition 18 crew members enjoy Christmas dinner in December 2008. Expedition 22 crew members gather around the dinner table in December 2009.Credit: NASA Expedition 26 crew members celebrates New Year’s Eve in December 2010.Credit: NASA Expedition 30 crew members pictured in December 2011.Credit: NASA Expedition 34 crew members pictured in December 2012. Credit: NASA Expedition 42 crew members leave milk and cookies for Santa and hang stockings using the airlock as a makeshift chimney in December 2013.Credit: NASA Expedition 50 crew members celebrate New Year’s Eve in December. Credit: NASA Expedition 54 crew member NASA astronaut Mark Vande Hei pictured as an elf for Christmas in December 2017.Credit: NASA Expedition 58 crew members inspect stockings for presents in December 2018 Expedition 61 crew member NASA astronaut Jessica Meir pictured with Hanukkah-themed socks in the cupola in December 2019. Expedition 61 crew members NASA astronauts Andrew Morgan, Christina Koch, and Jessica Meir, along with ESA (European Space Agency) astronaut Luca Parmitano share a holiday message on Dec. 23, 2019, from the International Space Station.Credit: NASA NASA astronaut Kayla Barron pictured with presents she wrapped for her crewmates in December 2021.Credit: NASA Expedition 68 crew members wear holiday outfits in December 2022.Credit: NASA Expedition 70 flight engineer NASA astronaut Jasmin Moghbeli’s husband and daughters made a felt menorah for her to celebrate Hanukkah during her mission. Since astronauts can’t light real candles aboard the space station, Moghbeli pinned felt “lights” for each night of the eight-day holiday. A dreidel spun in weightlessness will continue spinning until it comes in contact with another object but can’t land on any of its four faces. Expedition 70 crew members recorded a holiday message for those back on Earth.
Expedition 70 NASA astronaut Jasmin Moghbeli’s felt menorah and dreidel that she used to celebrate Hanukkah in December 2023. Credit: NASA NASA astronauts Don Pettit and Suni Williams, Expedition 72 flight engineer and commander respectively, pose for a fun holiday season portrait while speaking on a ham radio inside the International Space Station’s Columbus laboratory module. Credit: NASA To view this video please enable JavaScript, and consider upgrading to a web browser that supports HTML5 video
Expedition 72 video holiday message from the International Space Station. Credit: NASA The International Space Station is a convergence of science, technology, and human innovation that enables research not possible on Earth. The orbiting laboratory is a springboard for developing a low Earth economy and NASA’s next great leaps in exploration, including missions to the Moon under the Artemis campaign and, ultimately, human exploration of Mars.
Go here for more holiday memories onboard the space station. To learn more about the International Space Station, its research, and its crew, at:
https://www.nasa.gov/station
News Media Contacts:
Claire O’Shea
Headquarters, Washington
202-358-1100
claire.a.o’shea@nasa.gov
Sandra Jones
Johnson Space Center, Houston
281-483-5111
sandra.p.jones@nasa.gov
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By NASA
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
A crane lowers the steel reflector framework for Deep Space Station 23 into position Dec. 18 on a 65-foot-high (20-meter) platform above the antenna’s pedestal that will steer the reflector. Panels will be affixed to the structure create a curved surface to collect radio frequency signals.NASA/JPL-Caltech After the steel framework of the Deep Space Station 23 reflector dish was lowered into place on Dec. 18, a crew installed the quadripod, a four-legged support structure that will direct radio frequency signals from deep space that bounce off the main reflector into the antenna’s receiver.NASA/JPL-Caltech Deep Space Station 23’s 133-ton reflector dish was recently installed, marking a key step in strengthening NASA’s Deep Space Network.
NASA’s Deep Space Network, an array of giant radio antennas, allows agency missions to track, send commands to, and receive scientific data from spacecraft venturing to the Moon and beyond. NASA is adding a new antenna, bringing the total to 15, to support increased demand for the world’s largest and most sensitive radio frequency telecommunication system.
Installation of the latest antenna took place on Dec. 18, when teams at NASA’s Goldstone Deep Space Communications Complex near Barstow, California, installed the metal reflector framework for Deep Space Station 23, a multifrequency beam-waveguide antenna. When operational in 2026, Deep Space Station 23 will receive transmissions from missions such as Perseverance, Psyche, Europa Clipper, Voyager 1, and a growing fleet of future human and robotic spacecraft in deep space.
“This addition to the Deep Space Network represents a crucial communication upgrade for the agency,” said Kevin Coggins, deputy associate administrator of NASA’s SCaN (Space Communications and Navigation) program. “The communications infrastructure has been in continuous operation since its creation in 1963, and with this upgrade we are ensuring NASA is ready to support the growing number of missions exploring the Moon, Mars, and beyond.”
This time-lapse video shows the entire day of construction activities for the Deep Space Station 23 antenna at the NASA Deep Space Network’s Goldstone Space Communications Complex near Barstow, California, on Dec. 18. NASA/JPL-Caltech Construction of the new antenna has been under way for more than four years, and during the installation, teams used a crawler crane to lower the 133-ton metal skeleton of the 112-foot-wide (34-meter-wide) parabolic reflector before it was bolted to a 65-foot-high (20-meter-high) alidade, a platform above the antenna’s pedestal that will steer the reflector during operations.
“One of the biggest challenges facing us during the lift was to ensure that 40 bolt-holes were perfectly aligned between the structure and alidade,” said Germaine Aziz, systems engineer, Deep Space Network Aperture Enhancement Program of NASA’s Jet Propulsion Laboratory in Southern California. “This required a meticulous emphasis on alignment prior to the lift to guarantee everything went smoothly on the day.”
Following the main lift, engineers carried out a lighter lift to place a quadripod, a four-legged support structure weighing 16 1/2 tons, onto the center of the upward-facing reflector. The quadripod features a curved subreflector that will direct radio frequency signals from deep space that bounce off the main reflector into the antenna’s pedestal, where the antenna’s receivers are housed.
In the early morning of Dec. 18, a crane looms over the 112-foot-wide (34-meter-wide) steel framework for Deep Space Station 23 reflector dish, which will soon be lowered into position on the antenna’s base structure.NASA/JPL-Caltech Engineers will now work to fit panels onto the steel skeleton to create a curved surface to reflect radio frequency signals. Once complete, Deep Space Station 23 will be the fifth of six new beam-waveguide antennas to join the network, following Deep Space Station 53, which was added at the Deep Space Network’s Madrid complex in 2022.
“With the Deep Space Network, we are able to explore the Martian landscape with our rovers, see the James Webb Space Telescope’s stunning cosmic observations, and so much more,” said Laurie Leshin, director of JPL. “The network enables over 40 deep space missions, including the farthest human-made objects in the universe, Voyager 1 and 2. With upgrades like these, the network will continue to support humanity’s exploration of our solar system and beyond, enabling groundbreaking science and discovery far into the future.”
NASA’s Deep Space Network is managed by JPL, with the oversight of NASA’s SCaN Program. More than 100 NASA and non-NASA missions rely on the Deep Space Network and Near Space Network, including supporting astronauts aboard the International Space Station and future Artemis missions, monitoring Earth’s weather and the effects of climate change, supporting lunar exploration, and uncovering the solar system and beyond.
For more information about the Deep Space Network, visit:
https://www.nasa.gov/communicating-with-missions/dsn
News Media Contact
Ian J. O’Neill
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-2649
ian.j.oneill@jpl.nasa.gov
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Last Updated Dec 20, 2024 Related Terms
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By NASA
A method for evaluating thermophysical properties of metal alloys
Simulation of the solidification of metal alloys, a key step in certain industrial processes, requires reliable data on their thermophysical properties such as surface tension and viscosity. Researchers propose comparing predictive models with experimental outcomes as a method to assess these data.
Scientists use data on surface tension and viscosity of titanium-based alloys in industrial processes such as casting and crystal growth. Non-Equilibrium Solidification, Modelling for Microstructure Engineering of Industrial Alloys, an ESA (European Space Agency) investigation, examined the microstructure and growth of these alloys using the station’s Electromagnetic Levitator. This facility eliminates the need for containers, which can interfere with experiment results.
European Space Agency (ESA) astronaut Alexander Gerst is shown in the Columbus module of the International Space Station during the installation of the Electromagnetic Levitator.ESA/Alexander Gerst Overview of techniques for measuring thermal diffusion
Researchers present techniques for measuring thermal diffusion of molecules in a mixture. Thermal diffusion is measured using the Soret coefficient – the ratio of movement caused by temperature differences to overall movement within the system. This has applications in mineralogy and geophysics such as predicting the location of natural resources beneath Earth’s surface.
A series of ESA investigations studied diffusion, or how heat and particles move through liquids, in microgravity. Selectable Optical Diagnostics Instrument-Influence of VIbrations on DIffusion of Liquids examined how vibrations affect diffusion in mixtures with two components and SODI-DCMIX measured more-complex diffusion in mixtures of three or more components. Understanding and predicting the effects of thermal diffusion has applications in various industries such as modeling of underground oil reservoirs.
NASA astronaut Kate Rubins works on Selectable Optical Diagnostics Instrument Experiment Diffusion Coefficient Mixture-3 (SODI) DCMix-3 installation inside the station’s Microgravity Science Glovebox.JAXA (Japan Aerospace Exploration Agency)/Takuya Onishi Research validates ferrofluid technology
Researchers validated the concept of using ferrofluid technology to operate a thermal control switch in a spacecraft. This outcome could support development of more reliable and long-lasting spacecraft thermal management systems, increasing mission lifespan and improving crew safety.
Überflieger 2: Ferrofluid Application Research Goes Orbital analyzed the performance of ferrofluids, a technology that manipulates components such as rotors and switches using magnetized liquids and a magnetic field rather than mechanical systems, which are prone to wear and tear. This technology could lower the cost of materials for thermal management systems, reduce the need for maintenance and repair, and help avoid equipment failure. The paper discusses possible improvements to the thermal switch, including optimizing the geometry to better manage heat flow.
A view of the Ferrofluid Application Research Goes Orbital investigation hardware aboard the International Space Station. UAE (United Arab Emirates)/Sultan AlneyadiView the full article
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By NASA
NASA’s Dawn spacecraft captured this image of Vesta as it left the giant asteroid’s orbit in 2012. The framing camera was looking down at the north pole, which is in the middle of the image.NASA/JPL-Caltech/UCLA/MPS/DLR/IDA Known as flow formations, these channels could be etched on bodies that would seem inhospitable to liquid because they are exposed to the extreme vacuum conditions of space.
Pocked with craters, the surfaces of many celestial bodies in our solar system provide clear evidence of a 4.6-billion-year battering by meteoroids and other space debris. But on some worlds, including the giant asteroid Vesta that NASA’s Dawn mission explored, the surfaces also contain deep channels, or gullies, whose origins are not fully understood.
A prime hypothesis holds that they formed from dry debris flows driven by geophysical processes, such as meteoroid impacts, and changes in temperature due to Sun exposure. A recent NASA-funded study, however, provides some evidence that impacts on Vesta may have triggered a less-obvious geologic process: sudden and brief flows of water that carved gullies and deposited fans of sediment. By using lab equipment to mimic conditions on Vesta, the study, which appeared in Planetary Science Journal, detailed for the first time what the liquid could be made of and how long it would flow before freezing.
Although the existence of frozen brine deposits on Vesta is unconfirmed, scientists have previously hypothesized that meteoroid impacts could have exposed and melted ice that lay under the surface of worlds like Vesta. In that scenario, flows resulting from this process could have etched gullies and other surface features that resemble those on Earth.
To explore potential explanations for deep channels, or gullies, seen on Vesta, scientists used JPL’s Dirty Under-vacuum Simulation Testbed for Icy Environments, or DUSTIE, to simulate conditions on the giant asteroid that would occur after meteoroids strike the surface.NASA/JPL-Caltech But how could airless worlds — celestial bodies without atmospheres and exposed to the intense vacuum of space — host liquids on the surface long enough for them to flow? Such a process would run contrary to the understanding that liquids quickly destabilize in a vacuum, changing to a gas when the pressure drops.
“Not only do impacts trigger a flow of liquid on the surface, the liquids are active long enough to create specific surface features,” said project leader and planetary scientist Jennifer Scully of NASA’s Jet Propulsion Laboratory in Southern California, where the experiments were conducted. “But for how long? Most liquids become unstable quickly on these airless bodies, where the vacuum of space is unyielding.”
The critical component turns out to be sodium chloride — table salt. The experiments found that in conditions like those on Vesta, pure water froze almost instantly, while briny liquids stayed fluid for at least an hour. “That’s long enough to form the flow-associated features identified on Vesta, which were estimated to require up to a half-hour,” said lead author Michael J. Poston of the Southwest Research Institute in San Antonio.
Launched in 2007, the Dawn spacecraft traveled to the main asteroid belt between Mars and Jupiter to orbit Vesta for 14 months and Ceres for almost four years. Before ending in 2018, the mission uncovered evidence that Ceres had been home to a subsurface reservoir of brine and may still be transferring brines from its interior to the surface. The recent research offers insights into processes on Ceres but focuses on Vesta, where ice and salts may produce briny liquid when heated by an impact, scientists said.
Re-creating Vesta
To re-create Vesta-like conditions that would occur after a meteoroid impact, the scientists relied on a test chamber at JPL called the Dirty Under-vacuum Simulation Testbed for Icy Environments, or DUSTIE. By rapidly reducing the air pressure surrounding samples of liquid, they mimicked the environment around fluid that comes to the surface. Exposed to vacuum conditions, pure water froze instantly. But salty fluids hung around longer, continuing to flow before freezing.
The brines they experimented with were a little over an inch (a few centimeters) deep; scientists concluded the flows on Vesta that are yards to tens of yards deep would take even longer to refreeze.
The researchers were also able to re-create the “lids” of frozen material thought to form on brines. Essentially a frozen top layer, the lids stabilize the liquid beneath them, protecting it from being exposed to the vacuum of space — or, in this case the vacuum of the DUSTIE chamber — and helping the liquid flow longer before freezing again.
This phenomenon is similar to how on Earth lava flows farther in lava tubes than when exposed to cool surface temperatures. It also matches up with modeling research conducted around potential mud volcanoes on Mars and volcanoes that may have spewed icy material from volcanoes on Jupiter’s moon Europa.
“Our results contribute to a growing body of work that uses lab experiments to understand how long liquids last on a variety of worlds,” Scully said.
Find more information about NASA’s Dawn mission here:
https://science.nasa.gov/mission/dawn/
News Media Contacts
Gretchen McCartney
Jet Propulsion Laboratory, Pasadena, Calif.
818-287-4115
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NASA Headquarters, Washington
202-358-1600
karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov
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Last Updated Dec 20, 2024 Related Terms
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