Anonymous ID: 344c0a Aug. 31, 2023, 6:52 a.m. No.19465584   🗄️.is 🔗kun   >>5596 >>5743 >>5873 >>5881

NASA Astronomy Picture of the Day

Aug 31, 2023

 

The Crew-7 Nebula

 

Not the James Webb Space Telescope's latest view of a distant galactic nebula, this illuminated cloud of gas and dust dazzled early morning spacecoast skygazers on August 26. The snapshot was taken about 2 minutes after the launch of of a Falcon 9 rocket on the SpaceX Crew-7 mission, the seventh commercial crew rotation mission for the International Space Station. It captures drifting plumes and exhaust from the separated first and second stage illuminated against the still dark skies. Near the center of the image, within the ragged blueish ring, are two bright points of light. The lower one is the second stage of the rocket carrying 4 humans to space in a Crew Dragon spacecraft. The bright point above is the Falcon 9 first stage booster orienting itself for the trip back to Landing Zone-1 at Cape Canaveral, planet Earth.

 

https://apod.nasa.gov/apod/astropix.html?

Anonymous ID: 344c0a Aug. 31, 2023, 6:58 a.m. No.19465607   🗄️.is 🔗kun   >>5615 >>5743 >>5873 >>5881

India's Chandrayaan-3 moon rover reveals surprising sulfur find in lunar south pole soil

Aug 30, 2023

 

India's Chandrayaan-3 Vikram lander became the first craft to ever touch down at the lunar south pole on Aug. 23 — and the probe has wasted very little time scientifically exploring an environment that no mission from any country has ever visited.

 

Now, one instrument aboard the Chandrayaan-3 mission's moon rover Pragyan has found surprising traces of sulfur within the lunar south pole's soil.

 

Called Laser-Induced Breakdown Spectroscopy (LIBS) and created by the Laboratory for Electro-Optics Systems in Bangalore, that instrument probes the lunar surface by quite literally obliterating it. To observe a substance, LIBS fires laser pulses at a sample, which then vaporizes the substance into a brief plasma. The instrument picks up light emitted from that plasma and analyzes the wavelengths to discern what elements lie within.

 

When LIBS turned its laser onto the lunar south pole's soil, the instrument found the expected mélange of aluminum, calcium, chromium, iron, manganese, oxygen, titanium and silicon — but with an added dash of sulfur. Orbiting probes crossing over the moon's south pole had never previously detected sulfur, nor did they have the feasibility to do so, according to a statement by the Indian Space Research Organization (ISRO).

 

Chandrayaan-3 is leading the way for future missions, such as Artemis 3, to land at the lunar south pole. This region on the moon is an attractive place for humans to build a lasting presence due to the fact that water ice is located underfoot. Future moon-dwellers can potentially tap into that water for consumption, or even to create rocket propellant, instead of depending on water shipped from Earth.

 

Having a more complete chemical composition of the lunar south pole area means future travelers to — and possible inhabitants of — the region can also plan for what else they don’t need to bring from Earth. In particular, some scientists have suggested moon-dwellers could use sulfur in bits of infrastructure such as building materials, solar cells and batteries.

 

During the brief few days that Vikram and Pragyan have been on the moon, the mission has kept both the machines and their operators busy. For instance, over the weekend, the mission took the first-ever temperature measurements of the lunar south pole region's soil.

 

As for LIBS itself, ISRO says scientists are now using the instrument to search for another key element: Hydrogen.

 

https://www.space.com/chandrayaan-3-sulfur-surprising-composition-lunar-south-pole-soil

Anonymous ID: 344c0a Aug. 31, 2023, 7:09 a.m. No.19465643   🗄️.is 🔗kun   >>5743 >>5873 >>5881

Last Super Blue Moon until 2037 lights up skies around the world

Aug 31, 2023

 

The Super Blue Moon — one of the biggest and brightest moons of the year — rose on Aug. 30; inspiring skywatchers around the world to reach for their cameras and capture some incredible photographs.

 

The last Super Blue Moon for 14 years rose over the eastern horizon in the Aquarius constellation just after sunset tonight at around 7:10 p.m. EDT (2310 GMT). It then set just before sunrise on Thursday, Aug. 31 at around 06:46 EDT (1046 GMT).

 

The latest full moon is referred to as a Blue Moon, a term that can represent one of two things: Either the third full moon in a season that has four full moons; or, more commonly, the second of two full moons that fall in a calendar month. And similar to the previous full moon on Aug. 1, this Blue Moon was a "supermoon," a popular term for a full moon that occurs when our natural satellite is closer to Earth, making it appear just slightly larger and brighter in the sky.

 

Here we've rounded up some of the best Super Blue Moon photos from around the world.

 

https://www.space.com/rare-super-blue-moon-2023-photos

Anonymous ID: 344c0a Aug. 31, 2023, 7:21 a.m. No.19465691   🗄️.is 🔗kun   >>5743 >>5873 >>5881

A FEAST for the eyes

29 August 2023, 10:00

 

The graceful winding arms of the grand-design spiral galaxy M51 stretch across this image from the NASA/ESA/CSA James Webb Space Telescope. Unlike the menagerie of weird and wonderful spiral galaxies with ragged or disrupted spiral arms, grand-design spiral galaxies boast prominent, well-developed spiral arms like the ones showcased in this image. This galactic portrait is a composite image that integrates data from Webb’s Near-InfraRed Camera (NIRCam) and Mid-InfraRed Instrument (MIRI).

 

In this image the dark red regions trace the filamentary warm dust permeating the medium of the galaxy. The red regions show the reprocessed light from complex molecules forming on dust grains, while colours of orange and yellow reveal the regions of ionised gas by the recently formed star clusters. Stellar feedback has a dramatic effect on the medium of the galaxy and create complex network of bright knots as well as cavernous black bubbles.

 

M51 — also known as NGC 5194 — lies about 27 million light-years away from Earth in the constellation Canes Venatici, and is trapped in a tumultuous relationship with its near neighbour, the dwarf galaxy NGC 5195. The interaction between these two galaxies has made these galactic neighbours one of the better-studied galaxy pairs in the night sky. The gravitational influence of M51’s smaller companion is thought to be partially responsible for the stately nature of the galaxy’s prominent and distinct spiral arms. If you would like to learn more about this squabbling pair of galactic neighbours, you can explore earlier observations of M51 by the NASA/ESA Hubble Space Telescope here.

 

This Webb observation of M51 is one of a series of observations collectively titled Feedback in Emerging extrAgalactic Star clusTers, or FEAST. The FEAST observations were designed to shed light on the interplay between stellar feedback and star formation in environments outside of our own galaxy, the Milky Way. Stellar feedback is the term used to describe the outpouring of energy from stars into the environments which form them, and is a crucial process in determining the rates at which stars form. Understanding stellar feedback is vital to building accurate universal models of star formation.

 

The aim of the FEAST observations is to discover and study stellar nurseries in galaxies beyond our own Milky Way. Before Webb became operative, other observatories such as the Atacama Large Millimetre Array in the Chilean desert and Hubble have given us a glimpse of star formation either at the onset (tracing the dense gas and dust clouds where stars will form) or after the stars have destroyed with their energy their natal gas and dust clouds. Webb is opening a new window into the early stages of star formation and stellar light, as well as the energy reprocessing of gas and dust. Scientists are seeing star clusters emerging from their natal cloud in galaxies beyond our local group for the first time. They will also be able to measure how long it takes for these stars to pollute with newly formed metals and to clean out the gas (these time scales are different from galaxy to galaxy). By studying these processes, we will better understand how the star formation cycle and metal enrichment are regulated within galaxies as well as what are the time scales for planets and brown dwarfs to form. Once dust and gas is removed from the newly formed stars, there is no material left to form planets.

 

[Image Description: A large spiral galaxy takes up the entirety of the image. The core is mostly bright white, but there are also swirling, detailed structures that resemble water circling a drain. There is white and pale blue light that emanates from stars and dust at the core’s centre, but it is tightly limited to the core. The rings feature colours of deep red and orange and highlight filaments of dust around cavernous black bubbles.]

 

https://esawebb.org/images/potm2308a/

Anonymous ID: 344c0a Aug. 31, 2023, 7:23 a.m. No.19465705   🗄️.is 🔗kun   >>5743 >>5873 >>5881

Space Development Agency’s Second Tranche 0 Mission

 

SpaceX is targeting Thursday, August 31 at 8:25 a.m. PT (15:25 UTC) for a Falcon 9 launch of the Space Development Agency’s second Tranche 0 mission to low-Earth orbit from Space Launch Complex 4E (SLC-4E) at Vandenberg Space Force Base in California. If needed, a backup opportunity is available on Friday, September 1 at 7:26 a.m. PT (14:26 UTC).

 

The Falcon 9 first stage booster supporting this mission previously launched Sentinel-6 Michael Freilich, DART, Transporter-7, Iridium OneWeb, and eight Starlink missions. Following stage separation, the first stage will land on Landing Zone 4 (LZ-4) at Vandenberg Space Force Base.

 

The space vehicles launched during this mission will serve a part of SDA’s Proliferated Warfighter Space Architecture, a new layered network of satellites in low-Earth orbit and supporting elements that will provide global military communication and missile warning, indication, and tracking capabilities.

 

https://www.spacex.com/launches/mission/?missionId=SDA-Tranche0B

https://www.youtube.com/watch?v=685772KBdCo

Anonymous ID: 344c0a Aug. 31, 2023, 7:33 a.m. No.19465750   🗄️.is 🔗kun

Pentagon's UFO chief separates science from fiction

August 30, 2023

 

Dr. Sean Kirkpatrick, who leads the Pentagon's "All-domain Anomaly Resolution Office," talks about efforts to determine the truth behind "unidentified aerial phenomena" sightings around the planet.

 

https://abcnews.go.com/Nightline/video/pentagons-ufo-chief-separates-science-fiction-102667104

https://www.youtube.com/watch?v=uYignoEW_0s

Anonymous ID: 344c0a Aug. 31, 2023, 7:42 a.m. No.19465791   🗄️.is 🔗kun   >>5795 >>5873 >>5881

NASA gears up for return of OSIRIS-REx asteroid sample

August 31, 2023

 

WASHINGTON — NASA is making the final preparations to recover samples from an asteroid that a spacecraft will bring back to Earth in September.

 

Teams conducted a dress rehearsal Aug. 30 of the recovery of the sample return capsule from NASA’s OSIRIS-REx mission. In the test, a helicopter dropped a replica of the capsule from an altitude of more than 2,000 meters. The capsule descended under a parachute to land at the Utah Test and Training Range west of Salt Lake City, where personnel went through procedures to get the capsule ready for transport to NASA’s Johnson Space Center.

 

“We put our teams in the field, in the environment they’re going to be in, using the communications tools and the equipment they’re actually going to use on the day of recovery,” said Rich Burns, OSIRIS-REx project manager at NASA’s Goddard Space Flight Center, during a briefing after the rehearsal.

 

The rehearsal was part of final planning for the return of the actual OSIRIS-REx capsule, which will arrive early Sept. 24. The capsule is carrying an estimated 250 grams of material from the asteroid Bennu that the spacecraft collected during a “touch-and-go” collection process in October 2020.

 

The goal of the mission, whose full name is Origins, Spectral Interpretation, Resource Identification, and Security – Regolith Explorer, is to return those samples to Earth for analysis by scientists, who hope the material will offer new insights into the formation of the solar system.

 

“Boy, is the science team excited to get that,” said Dante Lauretta, principal investigator for OSIRIS-REx at the University of Arizona, of the samples. “We’re going back to the dawn of the solar system.”

 

There are still several key milestones before those samples are in the labs of Lauretta and other scientists. The spacecraft is scheduled to perform a maneuver Sept. 10 that will line its trajectory up with the Utah Test and Training Range. Another maneuver a week later will further refine its trajectory, aiming for an elliptical region of 650 square kilometers within the range. “We have a relatively small area to fit in, but we’re highly confident we’ll hit that,” Burns said.

 

A final go/no-go decision will come just a few hours before OSIRIS-REx releases the capsule at about 108,000 kilometers from the Earth. “We have a very long four hours from release until reentry,” said Sandra Freund, OSIRIS-REx program manager at Lockheed Martin. The capsule will reenter at more than 43,000 kilometers per hour, slowing down during reentry and deployment of drogue and main parachutes to less than 20 kilometers per hour for landing, 13 minutes after reentry.

 

The main OSIRIS-REx spacecraft will perform a “divert” maneuver about 20 minutes after releasing the capsule to avoid reentering itself. It will pass the Earth at a distance of 800 kilometers, putting it on a trajectory for an extended mission to visit the asteroid Apophis shortly after it makes a close flyby of Earth in 2029.

 

If something goes wrong with the maneuvers setting up the reentry that might cause it to miss the landing ellipse or otherwise jeopardize safety of the capsule or people on the ground, NASA will not release the capsule, Burns said. In that case, OSIRIS-REx will swing by the Earth on a trajectory that will bring it back in two years to make another attempt.

 

Mission teams are preparing for other problems that might come up during reentry and landing, including those that cause the capsule to crash into the ground at high speed. That is not unprecedented: NASA’s Genesis mission collected samples of the solar wind, but its parachutes failed to deploy on reentry, causing the capsule to crash in Utah upon its return in 2004.

 

“We learned a lot from Genesis,” said Freund. “We are very confident that we have taken the lessons learned forward from Genesis into OSIRIS-REx.” However, she said that the team has trained for various contingencies if the capsule does not land intact to preserve as much of the sample as possible.

 

If all goes well, though, analysis of the samples will begin almost immediately after the sample container is delivered to a clean room at a curation facility at JSC. Lauretta said an Oct. 11 press conference will discuss initial analysis of the samples, followed by presentations at the Fall Meeting of the American Geophysical Union in December.

 

Lauretta, who has been involved with OSIRIS-REx since the mission was proposed nearly two decades ago, said he will be part of the teams in Utah recovering the samples. “I wanted to personally be out there to greet these pieces of Bennu to our home planet, welcome them to the curation facility at Johnson Space Center and get them ready for the adventure we’re about to put them on.”

 

https://spacenews.com/nasa-gears-up-for-return-of-osiris-rex-asteroid-sample/

Anonymous ID: 344c0a Aug. 31, 2023, 7:44 a.m. No.19465799   🗄️.is 🔗kun   >>5873 >>5881

Webb Reveals New Structures Within Iconic Supernova

Aug 31, 2023

 

NASA’s James Webb Space Telescope has begun the study of one of the most renowned supernovae, SN 1987A (Supernova 1987A). Located 168,000 light-years away in the Large Magellanic Cloud, SN 1987A has been a target of intense observations at wavelengths ranging from gamma rays to radio for nearly 40 years, since its discovery in February of 1987. New observations by Webb’s NIRCam (Near-Infrared Camera) provide a crucial clue to our understanding of how a supernova develops over time to shape its remnant.

 

This image reveals a central structure like a keyhole. This center is packed with clumpy gas and dust ejected by the supernova explosion. The dust is so dense that even near-infrared light that Webb detects can’t penetrate it, shaping the dark “hole” in the keyhole.

 

A bright, equatorial ring surrounds the inner keyhole, forming a band around the waist that connects two faint arms of hourglass-shaped outer rings. The equatorial ring, formed from material ejected tens of thousands of years before the supernova explosion, contains bright hot spots, which appeared as the supernova’s shock wave hit the ring. Now spots are found even exterior to the ring, with diffuse emission surrounding it. These are the locations of supernova shocks hitting more exterior material.

 

While these structures have been observed to varying degrees by NASA’s Hubble and Spitzer Space Telescopes and Chandra X-ray Observatory, the unparalleled sensitivity and spatial resolution of Webb revealed a new feature in this supernova remnant – small crescent-like structures. These crescents are thought to be a part of the outer layers of gas shot out from the supernova explosion. Their brightness may be an indication of limb brightening, an optical phenomenon that results from viewing the expanding material in three dimensions. In other words, our viewing angle makes it appear that there is more material in these two crescents than there actually may be.

 

The high resolution of these images is also noteworthy. Before Webb, the now-retired Spitzer telescope observed this supernova in infrared throughout its entire lifespan, yielding key data about how its emissions evolved over time. However, it was never able to observe the supernova with such clarity and detail.

 

Despite the decades of study since the supernova’s initial discovery, there are several mysteries that remain, particularly surrounding the neutron star that should have been formed in the aftermath of the supernova explosion. Like Spitzer, Webb will continue to observe the supernova over time. Its NIRSpec (Near-Infrared Spectrograph) and MIRI (Mid-Infrared Instrument) instruments will offer astronomers the ability to capture new, high-fidelity infrared data over time and gain new insights into the newly identified crescent structures. Further, Webb will continue to collaborate with Hubble, Chandra, and other observatories to provide new insights into the past and future of this legendary supernova.

 

https://www.nasa.gov/feature/goddard/2023/webb-reveals-new-structures-within-iconic-supernova