OrbitalHub

NASA dicit:

NASA’s Starling mission is advancing the readiness of various technologies for cooperative groups of spacecraft – also known as distributed missions, clusters, or swarms. Starling will demonstrate technologies to enable multipoint science data collection by several small spacecraft flying in swarms. The six-month mission will use four CubeSats in low-Earth orbit to test four technologies that let spacecraft operate in a synchronized manner without resources from the ground. The technologies will advance the following capabilities: swarm maneuver planning and execution, communications networking, relative navigation, autonomous coordination between spacecraft.

The Starling mission will test whether the technologies work as expected, what their limitations are, and what developments are still needed for CubeSat swarms to be successful.

Distributed spacecraft are advantageous because they can act in unison to achieve objectives. Incorporating autonomy allows these missions to act cooperatively with minimal oversight from the ground. Autonomy ensures that a mission continues to perform through periods when communications with a spacecraft from the ground is temporarily unavailable because of distance or location. Spacecraft swarms operating at great distances from the Earth must act more autonomously due to the delays in time communicating with Earth ground stations.

Clustering satellites into a swarm requires planning and executing multiple maneuvers for each spacecraft. Managing these operations from the ground becomes impractical as the size of the swarm grows or the time delay in communicating with the spacecraft increases. The Starling mission will test technologies that traditionally run ground-oriented operations but are now shifted to operate onboard the spacecraft.

Having the spacecraft in a swarm operate autonomously is essential to making distributed spacecraft missions affordable and highly scaleable. Starling is a first step in developing this new mission architecture that could eventually allow for autonomous swarms of many spacecraft and at greater distances from Earth.

The four 6-unit CubeSats (each about the size of two stacked cereal boxes) will fly in a Sun-synchronous orbit more than 300 miles above Earth and no more than 170 miles apart from each other. The spacecraft will fly in two formations. First, they will begin in line, or in-train, like a string of pearls. Then, the CubeSats will move out of the in-train configuration and into a set of stable relative orbits known as passive safety ellipses.

The following four technologies will be tested:

Reconfiguration and Orbit Maintenance Experiments Onboard (ROMEO): In each phase, cluster flight control software will initially operate in shadow mode, autonomously planning maneuvers while the CubeSats are controlled from the ground. Once validated, ROMEO will demonstrate execution of swarm maintenance maneuvers from aboard the spacecraft without ground intervention. The performance of those maneuvers will then be evaluated.

Mobile Ad-hoc Network (MANET): The CubeSats will be able to communicate with each other via two-way S-band crosslink radios/antennas, adapting a ground-based network protocol for reliable space communication across any spacecraft node within the swarm. If one spacecraft communications node fails, the communications route automatically reconfigures to maintain full communication capabilities for the remaining operational swarm of spacecraft.

Starling Formation-Flying Optical Experiment (StarFOX): Using commercial star trackers, which are onboard cameras that measure the position of stars, each spacecraft determines its own orientation relative to the stars. An advanced navigation algorithm utilizes this orientation data and star tracker images to visually detect and track the other three spacecraft within the swarm to perform relative-position knowledge tests. The goal is for each spacecraft to achieve onboard awareness of its location as well as the location of the other three spacecraft.

Distributed Spacecraft Autonomy (DSA): This experiment will demonstrate autonomous monitoring of Earth’s ionosphere, the layer between our atmosphere and the beginning of space, with a spacecraft swarm. This is intended as a representative measurement to demonstrate autonomous reactive operations for future missions. Starling’s dual-band GPS receivers are used to measure the density of atmospheric regions. Each orbiting Starling spacecraft constantly changes position relative to the atmospheric phenomenon and the GPS satellites. Therefore, the most interesting source of information changes over time, requiring changes to the monitoring strategy in response to observations. DSA onboard software will autonomously coordinate the selection of the best GPS signals, across all Starling spacecraft, to accurately capture regions of higher or lower ionospheric density. This is accomplished by first sharing information over the crosslink network to maintain a consistent state, then selecting the GPS signals to prioritize and share in the future. The ability to evaluate data as it is collected, balance promising observations with coverage to ensure other interesting information is not missed, and autonomously coordinate measurements, is an enabling technology for future science missions.

It’s important to note that although Starling is being tested in low-Earth orbit, the technologies apply equally as well to deep space applications. In the future, constellation-like swarms of autonomously operating CubeSats could provide NASA and commercial missions in deep space with navigation services akin to GPS and communications relays provided by Earth’s network of communications satellites. Distributed spacecraft can also work together to collect multi-point science data and prepare for exploration missions by positioning multiple small spacecraft to function as one very large observation instrument. This could support the identification of resources for long-term presence on the Moon. Another example of this cooperative work might include telescopes mounted on multiple small spacecraft and trained on a particular observation target, creating a larger field of view than possible with a single telescope.

Video credit: NASA’s Ames Research Center

NASA dicit:

Teams at NASA’s Marshall Space Flight Center in Huntsville, Alabama, have completed applying a spray-on foam insulation to the launch vehicle stage adapter (LVSA) for the Artemis III mission. The LVSA is a cone-shaped piece of hardware that connects the SLS (Space Launch System) rocket’s upper and lower stages and partially encloses the engine of the interim cryogenic propulsion stage. The spray-on foam insulation is a type of thermal protection system that is used to protect the Moon rocket’s hardware from the extreme temperatures, forces, and sounds it’ll experience during launch and ascent. Unlike other parts of the mega rocket, the thermal protection system for the LVSA is applied entirely by hand using a tool similar to a spray gun. It is the largest piece of SLS hardware to be hand sprayed.

Video credit: NASA’s Marshall Space Flight Center

Wikipedia dicit:

SpaceX’s Dragon spacecraft successfully separates from the second stage of the company’s Falcon 9 rocket during NASA’s SpaceX 28th commercial resupply services mission to the International Space Station. Liftoff occurred at 11:47 a.m. EDT on June 5, 2023, from NASA Kennedy Space Center’s Launch Complex 39A in Florida.

SpaceX plans to reuse the Cargo Dragons up to five times. The Cargo Dragon launches without SuperDraco abort engines, without seats, cockpit controls and the life support system required to sustain astronauts in space.

Video credit: SpaceX

Wikipedia dicit:

Starship is a super heavy-lift space vehicle under development by SpaceX. At 120 metres (394 feet) in height and with a liftoff mass of 5,000 metric tons (11,023,000 pounds), Starship is the largest and most powerful rocket ever flown, surpassing the Saturn V rocket of the 1960s Apollo Program.

The space vehicle consists of the first-stage Super Heavy booster and the second-stage spacecraft also named Starship. Both stages are powered by Raptor rocket engines, which burn liquid oxygen and liquid methane propellants in a full-flow staged combustion power cycle. Both are designed to be fully reusable, performing controlled landings on the launch tower and reflown within hours. Starship is designed to have a payload capacity of 150 tonnes (330,000 lb) to low Earth orbit in a fully reusable configuration and 250 t (550,000 lb) when expended. Starship vehicles in low Earth orbit are planned to be refilled with propellant launched in tanker Starships to enable transit to higher energy destinations such as geosynchronous orbit, the Moon, and Mars.

Plans for a heavy-lift vehicle at SpaceX date to 2005, with the earliest concept resembling the modern vehicle announced in 2016. SpaceX’s Starship development follows an iterative and incremental approach involving frequent, and often destructive, test flights of prototype vehicles. The first orbital test flight was attempted on 20 April 2023, when an anomaly caused the vehicle to tumble out of control four minutes after launch. SpaceX activated the flight termination system, which fired the explosive charges but did not destroy the vehicle. Approximately 40 seconds later both stages were destroyed due to increased aerodynamic forces. After the test, the Federal Aviation Administration (FAA) grounded the launch program pending results of a standard “mishap investigation.”

SpaceX intends Starship to become its primary space vehicle, superseding the Falcon 9 and Falcon Heavy launch vehicles as well as the Dragon spacecraft currently used as part of NASA’s commercial crew program to the International Space Station. Starship is often coupled with the company’s Mars ambitions. Planned Starship flights include the development of SpaceX’s Starlink internet constellation, crewed flights under the Polaris and dearMoon programs, and a crewed lunar landing with a modified Starship spacecraft under the Artemis program.

Video credit: SpaceX

NASA dicit:

The animation highlights the “super” in supermassive black holes. These monsters lurk in the centers of most big galaxies, including our own Milky Way, and contain between 100,000 and tens of billions of times more mass than our Sun.

Any light crossing the event horizon – the black hole’s point of no return – becomes trapped forever, and any light passing close to it is redirected by the black hole’s intense gravity. Together, these effects produce a “shadow” about twice the size of the black hole’s actual event horizon.

The animation shows 10 supersized black holes that occupy center stage in their host galaxies, including the Milky Way and M87, scaled by the sizes of their shadows. Starting near the Sun, the camera steadily pulls back to compare ever-larger black holes to different structures in our solar system.

First up is 1601+3113, a dwarf galaxy hosting a black hole packed with the mass of 100,000 Suns. The matter is so compressed that even the black hole’s shadow is smaller than our Sun.

The black hole at the heart of our own galaxy, called Sagittarius A* (pronounced ay-star), boasts the weight of 4.3 million Suns based on long-term tracking of stars in orbit around it. It’s shadow diameter spans about half that of Mercury’s orbit in our solar system.

The animation shows two monster black holes in the galaxy known as NGC 7727. Located about 1,600 light-years apart, one weighs 6 million solar masses and the other more than 150 million Suns. Astronomers say the pair will merge within the next 250 million years.

At the animation’s larger scale lies M87’s black hole, now with a updated mass of 5.4 billion Suns. Its shadow is so big that even a beam of light – traveling at 670 million mph (1 billion kph) – would take about two and a half days to cross it.

The movie ends with TON 618, one of a handful of extremely distant and massive black holes for which astronomers have direct measurements. This behemoth contains more than 60 billion solar masses, and it boasts a shadow so large that a beam of light would take weeks to traverse it.

Video credit: NASA Goddard

NASA dicit:

The four members of NASA’s SpaceX Crew-6 mission move their Dragon Endeavour spacecraft between docking ports on the International Space Station. Aboard are: NASA astronauts Steve Bowen and Woody Hoburg, UAE astronaut Sultan Alneyadi, Roscosmos cosmonaut Andrey Fedyaev.

The crew will undock from the space-facing port of the station’s Harmony module, then dock at the station’s forward Harmony port. Endeavour is relocating to make room for SpaceX’s 28th cargo resupply mission, currently scheduled to arrive in June.

Video credit: NASA