OrbitalHub

NASA dicit:

SpaceX CRS-23, also known as SpX-23, is a Commercial Resupply Service mission to the International Space Station. The mission was contracted by NASA and was flown by SpaceX using the Cargo Dragon C208. This was the third flight for SpaceX under NASA’s CRS Phase 2 contract awarded in January 2016. A NASA Flight Planning Integration Panel (FPIP) from 2019 indicates that SpaceX cargo missions will begin to extend their duration to 60 days and beyond starting with CRS-23.

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. This newer design provides several benefits, including a faster process to recover, refurbish and re-fly versus the earlier Dragon CRS design used for ISS cargo missions.

The GITAI S1 Robotic Arm Tech Demo will test GITAI Japan Inc.’s microgravity robot by placing the arm inside the newly added Nanoracks Bishop Airlock, which was carried to the station by Dragon C208.2 during the SpaceX CRS-21 mission last year. Once inside the airlock, the arm will perform numerous tests to demonstrate its versatility and dexterity.

Designed by GITAI Japan Inc., the robot will work as a general-purpose helper under the pressurized environment inside the Bishop Airlock. It will operate tools and switches and run scientific experiments. The next step will be to test it outside the ISS in the harsh space environment. The robot will be able to perform tasks both autonomously and via teleoperations. Its arm has eight degrees of freedom and a 1-meter reach. GITAI S1 is a semi-autonomous/semi-teleoperated robotic arm designed to conduct specified tasks internally and externally on space stations, on-orbit servicing, and lunar base development. By combining autonomous control via AI and teleoperations via the specially designed GITAI manipulation system H1, GITAI S1 on its own, possesses the capability to conduct generous-purpose tasks (manipulation of switches, tools, soft objects; conducting science experiments and assembly; high-load operations; etc.) that were extremely difficult for industrial robots such as task specific robotic arms to do.

Video credit: NASA/SpaceX

NASA dicit:

Hurricanes are some of the most powerful and destructive weather events on Earth. To help study these powerful storms, NASA is launching TROPICS (Time-Resolved Observations of Precipitation structure and storm Intensity with a Constellation of Smallsats), a collection of six small satellites designed to measure storm strength by detecting the thermal radiation naturally emitted by the oxygen and water vapor in the air.

In June 2021, NASA launched a test version of the satellite, called a pathfinder, ahead of the constellation of six weather satellites planned for launch in 2022. When launched, the TROPICS satellites will work together to provide near-hourly microwave observations of a storm’s precipitation, temperature, and humidity. The mission is expected to help scientists understand the factors driving tropical cyclone intensification and to improve forecasting models.

Video credit: NASA’s Goddard Space Flight Center/Scientific Visualization Studio/Katie Jepson (KBRwyle): Producer/Ellen T. Gray (ADNET): Writer/William Blackwell (MIT): Scientist/Jonathan North (KBRwyle): Animator/Adriana Manrique Gutierrez (USRA): Animator/Katie Jepson (KBRwyle): Animator/Taylor Johnson: Narration

NASA dicit:

Hundreds of meltwater lakes hide deep beneath the expanse of Antarctica’s ice sheet. With a powerful laser altimeter system in space, NASA’s Ice Cloud and land Elevation Satellite-2 (ICESat-2) is helping scientists “see” under the ice.

Video credit: NASA’s Goddard Space Flight Center/Scientific Visualization Studio/Jefferson Beck (KBRwyle): Lead Producer/Roberto Molar Candanosa (KBR): Lead Writer/Helen-Nicole Kostis (USRA): Lead Visualizer/Helen Amanda Fricker (Scripps Institution of Oceanography, University of California, San Diego): Lead Scientist/Matthew R. Siegfried (Colorado School of Mines): Lead Scientist

NASA dicit:

How close can spacecraft get to the Sun without burning up? That may be a topic of hot debate but researchers are working on a concept to get closer than ever before. This is the NASA Innovative Advanced Concept (NIAC) that explores the capabilities and benefits of a new solar protection system.

This video represents a research study within the NASA Innovative Advanced Concepts (NIAC) program. NIAC is a visionary and far-reaching aerospace program, one that has the potential to create breakthrough technologies for possible future space missions. However, such early stage technology developments may never become actual NASA missions.

Video credit: NASA 360

NASA dicit:

Scientists have reached a new frontier in our understanding of pulsars, the dense, whirling remains of exploded stars, thanks to observations from NASA’s Neutron star Interior Composition Explorer (NICER). Data from this X-ray telescope aboard the International Space Station has produced the first precise and dependable measurements of both a pulsar’s size and its mass.

The pulsar in question, J0030+0451 (J0030 for short), is a solitary pulsar that lies 1,100 light-years away in the constellation Pisces. While measuring the pulsar’s heft and proportions, NICER revealed that the shapes and locations of million-degree hot spots on the pulsar’s surface are much stranger than generally thought.

Using NICER observations, two groups of scientists mapped J0030’s hot spots using independent methods and converged on nearly identical results for its mass and size. One team, led by researchers at the University of Amsterdam, determined the pulsar is around 1.3 times the Sun’s mass, 15.8 miles (25.4 kilometers) across and has two hot spots — one small and circular, the other long and crescent-shaped. A second team found J0030 is about 1.4 times the Sun’s mass, about 16.2 miles (26 kilometers) wide and has two or three oval-shaped hot spots. All spots in all models are in the pulsar’s southern hemisphere — unlike textbook images where the spots lie on opposite sides other at each magnetic poles.

Video credit: NASA’s Goddard Space Flight Center/Scott Wiessinger (USRA): Producer/Jeanette Kazmierczak (University of Maryland College Park): Science Writer/Francis Reddy (University of Maryland College Park): Science Writer/Michael Lentz (USRA): Animator/Barb Mattson (University of Maryland College Park): Narrator/Zaven Arzoumanian (NASA/GSFC): Scientist

NASA dicit:

Unprecedented observations of a nova outburst in 2018 by a trio of satellites, including NASA’s Fermi and NuSTAR space telescopes, have captured the first direct evidence that most of the explosion’s visible light arose from shock waves — abrupt changes of pressure and temperature formed in the explosion debris.

A nova is a sudden, short-lived brightening of an otherwise inconspicuous star. It occurs when a stream of hydrogen from a companion star flows onto the surface of a white dwarf, a compact stellar cinder not much larger than Earth.

The 2018 outburst originated from a star system later dubbed V906 Carinae, which lies about 13,000 light-years away in the constellation Carina. Over time — perhaps tens of thousands of years for a so-called classical nova like V906 Carinae — the white dwarf’s deepening hydrogen layer reaches critical temperatures and pressures. It then erupts in a runaway reaction that blows off all of the accumulated material.

Fermi detected its first nova in 2010 and has observed 14 to date. Gamma rays the highest-energy form of light require processes that accelerate subatomic particles to extreme energies, which happens in shock waves. When these particles interact with each other and with other matter, they produce gamma rays. Because the gamma rays appear at about the same time as a nova’s peak in visible light, astronomers concluded that shock waves play a more fundamental role in the explosion and its aftermath.

The Fermi and BRITE data show flares in both wavelengths at about the same time, so they must share the same source shock waves in the fast-moving debris.

Observations of one flare using NASA’s NuSTAR space telescope showed a much lower level of X-rays compared to the higher-energy Fermi data, likely because the nova ejecta absorbed most of the X-rays. High-energy light from the shock waves was repeatedly absorbed and reradiated at lower energies within the nova debris, ultimately only escaping at visible wavelengths.

Video credit: NASA’s Goddard Space Flight Center/Chris Smith (USRA): Lead Animator/Chris Smith (USRA): Producer/Scott Wiessinger (USRA): Producer/Francis Reddy (University of Maryland College Park): Lead Science Writer/Scott Wiessinger (USRA): Narrator/Scott Wiessinger (USRA): Editor