Under the agency’s Announcement of Collaborative Opportunity, engineers from NASA’s Marshall Space Flight Center in Huntsville, Alabama, partnered with Elementum 3D, in Erie, Colorado, to create a weldable type of aluminum that is heat resistant enough for use on rocket engines. Compared to other metals, aluminum is lower density and allows for high-strength, lightweight components. However, due to its low tolerance to extreme heat and its tendency to crack during welding, aluminum is not typically used for additive manufacturing of rocket engine parts – until now.
Meet NASA’s latest development under the Reactive Additive Manufacturing for the Fourth Industrial Revolution, or RAMFIRE, project. Funded under NASA’s Space Technology Mission Directorate (STMD), RAMFIRE focuses on advancing lightweight, additively manufactured aluminum rocket nozzles. The nozzles are designed with small internal channels that keep the nozzle cool enough to prevent melting.
A scale model of the Mars Ascent Vehicle is tested for in the trisonic wind tunnel at Marshall. The tunnel’s test sections are only 14 inches in height and width but can achieve wind speeds of up to Mach 5.
The Mars Ascent Vehicle team recently completed testing at NASA facility that has been a critical part of missions going all the way back to the Apollo program. The same facility is now helping the agency prepare to launch the first rocket from Mars.
The MAV is an important part of the joint plan between NASA and ESA (European Space Agency) to bring scientifically selected Martian samples to Earth in the early 2030s.
Lucy is a NASA space probe on a twelve-year journey to eight different asteroids, visiting two main belt asteroids as well as six Jupiter trojans, asteroids which share Jupiter’s orbit around the Sun, orbiting either ahead of or behind the planet. All target encounters will be flyby encounters. The Lucy spacecraft is the centerpiece of a US$981 million mission.
On 4 January 2017, Lucy was chosen, along with the Psyche mission, as NASA’s Discovery Program missions 13 and 14 respectively.
The mission is named after the Lucy hominid fossils, because study of the trojans could reveal the “fossils of planet formation”: materials that clumped together in the early history of the Solar System to form planets and other bodies. The hominid was named after the 1967 Beatles song “Lucy in the Sky with Diamonds”. The spacecraft carries a disc made of lab-grown diamonds for its L’TES instrument.
Psyche is a NASA space mission launched on October 13, 2023 to explore the origin of planetary cores by orbiting and studying the metallic asteroid 16 Psyche beginning in 2029. NASA’s Jet Propulsion Laboratory (JPL) manages the project.
16 Psyche is the heaviest known M-type asteroid, and may be an exposed iron core of a protoplanet, the remnant of a violent collision with another object that stripped off its mantle and crust. On January 4, 2017, the Psyche mission was selected for NASA’s Discovery #14 mission. It was launched atop a SpaceX Falcon Heavy rocket.
16 Psyche is the heaviest known M-type asteroid, and may be an exposed iron core of a protoplanet, the remnant of a violent collision with another object that stripped off its mantle and crust.
Recent studies show that it is “a mixed metal and silicate world”. Another study considers it to be either a metal core of a protoplanet or “a differentiated world with a regolith composition … peppered with localized regions of high metal concentrations”. Radar observations of the asteroid from Earth indicate an iron–nickel composition.
The Psyche spacecraft is designed with solar electric propulsion, and the scientific payload includes a multispectral imager, a magnetometer, and a gamma-ray spectrometer.
The mission is designed to perform 21 months of science. The spacecraft was built by NASA Jet Propulsion Laboratory (JPL) in collaboration with SSL (formerly Space Systems/Loral) and Arizona State University.
It was proposed that the rocket launch might be shared with a separate mission named Athena, that would perform a single flyby of asteroid 2 Pallas, the third-largest asteroid in the Solar System.
In May 2020, it was announced that the Falcon Heavy carrying Psyche would include two smallsat secondary payloads to study the Martian atmosphere and binary asteroids, named EscaPADE (Escape and Plasma Acceleration and Dynamics Explorers) and Janus respectively, but in September 2020, the EscaPADE Mars atmosphere probe was removed from the plan.
Janus was later removed from the Psyche mission as well on November 18, 2022, after an assessment determined that it would not be on the required trajectory to meet its science requirements as a result of Psyche’s new launch period.
Using NASA’s Neil Gehrels Swift Observatory, which launched in 2004, scientists have discovered a black hole in a distant galaxy repeatedly nibbling on a Sun-like star. The object heralds a new era of Swift science made possible by a novel method for analyzing data from the satellite’s X-ray Telescope (XRT). When a star strays too close to a monster black hole, gravitational forces create intense tides that break the star apart into a stream of gas. The leading edge swings around the black hole, and the trailing edge escapes the system. These destructive episodes are called tidal disruption events. Astronomers see them as flares of multiwavelength light created when the debris collides with a disk of material already orbiting the black hole.
Recently, astronomers have been investigating variations on this phenomena, which they call partial or repeating tidal disruptions. During these events, every time an orbiting star passes close to a black hole, the star bulges outward and sheds material, but survives. The process repeats until the star looses too much gas and finally breaks apart. The characteristics of the individual star and black hole system determine what kind of emission scientists observe, creating a wide array of behaviors to categorize.
On June 22, 2022, XRT captured Swift J0230 for the first time. It lit up in a galaxy around 500 million light-years away in the northern constellation Triangulum. Swift’s XRT has observed nine additional outbursts from the same location roughly every few weeks. Scientists propose that Swift J0230 is a repeating tidal disruption of a Sun-like star orbiting a black hole with over 200,000 times the Sun’s mass. They estimate the star loses around three Earth masses of material on each pass. This system provides a bridge between other types of suspected repeating disruptions and allowed scientists to model how interactions between different star types and black hole sizes affect what we observe.
Swift J0230’s discovery was possible thanks to a new, automated search of XRT observations called the Swift X-ray Transient Detector. After the instrument observes a portion of the sky, the data is transmitted to the ground, and the program compares it to previous XRT snapshots of the same spot. If that portion of the X-ray sky has changed, scientists get an alert. In the case of Swift J0230, astronomers were able to rapidly coordinate additional observations of the region.
Video credit: NASA’s Goddard Space Flight Center/Producer: Sophia Roberts (AIMM)/Science writer: Jeanette Kazmierczak (University of Maryland College Park)/Editor: Sophia Roberts (AIMM)/Narrator: Sophia Roberts (AIMM)/Animator: Chris Smith (KBRwyle)/Project support: Scott Wiessinger (KBRwyle)
New NASA and Durham University simulations put forth a theory of the origin of Saturn’s rings and icy moons – they may have formed following a massive collision between two moons orbiting the gas giant. The simulations used in this research are some of the most detailed of their kind to study the formation of Saturn’s rings and potentially habitable icy moons.
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