Monday, November 18, 2024

SpaceX: Making Life Multi-Planetary | November 2024 Update

SpaceX: Making Life Multi-Planetary | November 2024 Update

"SpaceX was founded to increase access to space and [to] help make life multiplanetary. In just this year, we’ve launched 114 successful Falcon missions and counting for our commercial and government customers, deployed  ~1,700 Starlink satellites to provide high-speed Internet for millions of people all around the world, and made extraordinary strides developing Starship’s capability to return humanity to the Moon and ultimately send people to Mars."

The primary goal of SpaceX is to build a fully reusable transportation system designed to carry crew and cargo to Earth orbit, the Moon, Mars and beyond.

"Starship is essential to both SpaceX’s plans to deploy its next-generation Starship system as well as for NASA, which will use a lunar lander version of Starship for landing astronauts on the Moon during the Artemis III mission through the Human Landing System (HLS) program."

If you want to join the team and help build a more exciting future, check out the latest job openings across the company → https://www.spacex.com/careers


Video Credit: Space Exploration Technologies Corporation (SpaceX)
Duration: 1 minute, 24 seconds
Release Date: Nov. 18, 2024

#NASA #SpaceX #Space #Earth #Mars #Moon #MoonToMars #ArtemisProgram #ArtemisIII #Starship #Spacecraft #HeavyBooster #SuperHeavyRocket #ElonMusk #GwynneShotwell #Engineering #SpaceTechnology #HumanSpaceflight #CommercialSpace #SpaceExploration #Starbase #Texas #Careers #UnitedStates #STEM #Education #HD #Video

NASA’s Curiosity Mars Rover Takes a Last Look at Mysterious Sulfur | JPL

NASA’s Curiosity Mars Rover Takes a Last Look at Mysterious Sulfur | JPL

NASA’s Curiosity Mars rover captured this panorama using its Mastcam while heading west away from Gediz Vallis channel on Nov. 2, 2024
NASA’s Curiosity Mars rover captured this last look at a field of bright white sulfur stones on Oct. 11, before leaving Gediz Vallis channel. The field was where the rover made the first discovery of pure sulfur on Mars. Scientists are still unsure exactly why theses rocks formed here.
Scientists think that ancient groundwater formed this weblike pattern of ridges, called boxwork, that were captured by NASA’s Mars Reconnaissance Orbiter on Dec. 10, 2006. The agency’s Curiosity rover will study ridges similar to these up close in 2025.

NASA’s Curiosity rover is preparing for the next leg of its journey, a monthslong trek to a formation called the boxwork. It is a set of weblike patterns on Mars’ surface that stretches for miles. It will soon leave Gediz Vallis channel. How the channel formed so late during a transition to a drier climate remains a key question for the science team. Another interesting find is the field of white sulfur stones the rover discovered this past summer.

The rover is searching for evidence that ancient Mars had the right ingredients to support microbial life, if any formed billions of years ago, when the Red Planet held lakes and rivers. Located in the foothills of Mount Sharp, a 3-mile-tall (5-kilometer-tall) mountain, Gediz Vallis channel may help tell a related story—what the area was like as water was disappearing on Mars. Although older layers on the mountain had already formed in a dry climate, the channel suggests that water occasionally coursed through the area as the climate was changing.

Scientists are still piecing together the processes that formed features within the channel, including the debris mound nicknamed “Pinnacle Ridge." It appears that rivers, wet debris flows, and dry avalanches all left their mark. The science team is now constructing a timeline of events from Curiosity’s observations.

The science team is also trying to answer important questions about the sprawling field of sulfur stones. Images of the area from NASA’s Mars Reconnaissance Orbiter (MRO) showed what looked like an unremarkable patch of light-colored terrain. It turns out that the sulfur stones were too small for MRO’s High-Resolution Imaging Science Experiment (HiRISE) to see, and Curiosity’s team was intrigued to find them when the rover reached the patch. They were even more surprised after Curiosity rolled over one of the stones, crushing it to reveal yellow crystals inside.

Science instruments on the rover confirmed the stone was pure sulfur—something no mission has seen before on Mars. The team cannot yet explain why the sulfur formed there. On Earth, it is associated with volcanoes and hot springs, and no evidence exists of Mount Sharp having either of those causes present.

“We looked at the sulfur field from every angle—from the top and the side—and looked for anything mixed with the sulfur that might give us clues as to how it formed. We’ve gathered a ton of data, and now we have a fun puzzle to solve,” said Curiosity’s project scientist Ashwin Vasavada at NASA’s Jet Propulsion Laboratory in Southern California.

Spiderwebs on Mars

Curiosity has traveled about 20 miles (33 kilometers) since landing in 2012. It is now driving along the western edge of the Gediz Vallis channel, gathering a few more panoramas to document the region before traveling to the boxwork.

Viewed by MRO, the boxwork looks like spiderwebs stretching across the surface. It is believed to have formed when minerals carried by Mount Sharp’s last pulses of water settled into fractures in surface rock and then hardened. As portions of the rock eroded away, what remained were the minerals that had cemented themselves in the fractures, leaving the weblike boxwork.

On Earth, boxwork formations have been seen on cliffsides and in caves. However, Mount Sharp’s boxwork structures stand apart from those because they formed as water was disappearing from Mars and because they are so extensive, spanning an area of 6 to 12 miles (10 to 20 kilometers).

“These ridges will include minerals that crystallized underground, where it would have been warmer, with salty liquid water flowing through,” said Kirsten Siebach of Rice University in Houston, a Curiosity scientist studying the region. “Early Earth microbes could have survived in a similar environment. That makes this an exciting place to explore.”

More About Curiosity

Curiosity was built by NASA’s Jet Propulsion Laboratory, which is managed by Caltech in Pasadena, California. JPL leads the mission on behalf of NASA’s Science Mission Directorate in Washington.

The University of Arizona, in Tucson, operates HiRISE, which was built by BAE Systems (formerly Ball Aerospace & Technologies Corp.), in Boulder, Colorado. JPL manages the Mars Reconnaissance Orbiter Project for NASA’s Science Mission Directorate in Washington.


Credit: NASA's Jet Propulsion Laboratory/Caltech/MSSS/University of Arizona
Release Date: Nov. 18, 2024

#NASA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #CuriosityRover #MSL #GedizVallisChannel #Sulphur #MountSharp #GaleCrater #MROSpacecraft #HiRISE #Robotics #SpaceTechnology #SpaceEngineering #JPL #Caltech #UnitedStates #STEM #Education

NASA's Curiosity Mars Rover Leaves Gediz Vallis Channel: 360 View | JPL

NASA's Curiosity Mars Rover Leaves Gediz Vallis Channel: 360 View | JPL

Support FriendsofNASA.org: Drag your mouse or move your phone to explore this 360-degree panorama provided by NASA’s Curiosity Mars rover. This view was captured just before the rover exited Gediz Vallis channel. It was likely formed by ancient floodwaters and landslides.

Visible in this scene is the field of sulfur stones where the rover rolled over a rock and cracked it open, revealing yellow crystals inside and marking the first time scientists have seen pure sulfur on Mars. Note: The rover has discovered lots of sulfur-based minerals in the past, however, not pure sulfur. In this video, a close-up of the sulfur field is embedded roughly where it is located in the landscape.

Also look for rover tracks, a dusty view of Gale Crater’s rim in the distance, and the route Curiosity is taking away from the channel toward new adventures.

The rover used its Mast Camera, or Mastcam, to take this panorama on Sept. 21 and 22, 2024, the 4,311st and 4,312nd Martian day, or sol, of Curiosity’s surface mission. It is made up of 341 individual images that were stitched together. The color has been adjusted to match lighting conditions as the human eye would see them on Earth. 

Note on best viewing: Not all browsers support 360-degree videos. YouTube supports playback on computers using Chrome, Firefox, MS Edge, and Opera browsers. For the best experience on a mobile device, play this video in the YouTube app. To improve the resolution, open the video settings (using the gear icon) and select the highest quality available.

Celebrating 12+ Years on Mars (2012-2024)

Mission Name: Mars Science Laboratory (MSL)
Rover Name: Curiosity
Main Job: To determine if Mars was ever habitable to microbial life. 
Launch: Nov. 6, 2011
Landing Date: Aug. 5, 2012, Gale Crater, Mars

For more about Curiosity, visit: 

For more information on NASA's Mars missions, visit: mars.nasa.gov

Credit: NASA/JPL-Caltech/MSSS
Duration: 2 minutes, 14 seconds
Release Date: Nov. 18, 2024

#NASA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #CuriosityRover #MSL #GedizVallisChannel #Sol4311 #Sol4312 #MountSharp #GaleCrater #Robotics #SpaceTechnology #SpaceEngineering #JPL #Caltech #UnitedStates #STEM #Education #360Video #HD #Video

New Shenzhou-19 Crew Adapts to Work & Living Conditions | China Space Station

New Shenzhou-19 Crew Adapts to Work & Living Conditions | China Space Station 

China's Shenzhou-19 crew aboard the orbiting Tiangong Space Station have adapted to their new environment and have started to engage in their daily routines after they boarded the station over 2 weeks ago, according to the China Manned Space Agency (CMSA).

The crew members, Cai Xuzhe, Song Lingdong, and Wang Haoze, were launched to the China Space Station on Oct. 30, 2024, for a six-month mission.

In close coordination with ground researchers, the Shenzhou-19 crew have completed their first full-system pressure emergency drill and in-orbit medical training since their arrival.

The drill simulated the process of the crew members responding to an internal depressurization scenario at the space station. This involves astronauts and ground personnel collaborating in emergency response throughout the entire process.

The in-orbit medical training simulated the procedures for providing medical assistance in the event of sudden illness or injury among astronauts. This is aimed to help the crew become more familiar with the locations of medical devices in the space station, to review usage methods, and to reinforce operational processes and skills.

During the mission, the crew will carry out extravehicular activities—spacewalks, including the installation of space debris protection devices.

Last week, the three astronauts completed routine checks and maintenance of their spacesuits, and confirmed their storage conditions, ensuring that the suits are in good condition.

While in orbit, the crew are required to regularly conduct environmental monitoring and equipment maintenance within the space station.

Last week, Shenzhou-19 commander Cai Xuzhe inspected the cabin's acoustic environment.

Additionally, the crew completed inspections and maintenance of the regenerative life support system equipment.

Furthermore, the crew regularly carried out tasks, such as cleaning, supplies arranging and transfer, and garbage transfer and storage to maintain a clean environment in the space station.

Moreover, the astronauts also underwent regular medical checks to monitor their health and they performed routine physical exercises.

Shenzhou-19 Crew:
Commander Cai Xuzhe (蔡旭哲)
Mission Specialist Wang Haoze (王浩泽)
Mission Specialist Song Lingdong (宋令东)


Video Credit: CCTV
Duration: 2 minutes, 11 seconds
Release Date: Nov. 18, 2024

#NASA #Space #Science #Earth #China #中国 #Shenzhou19 #神舟十九号 #Taikonauts #Astronauts #CSS #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #SpaceLaboratory #MicrogravityExperiments #CMSA #国家航天局 #LongDurationMissions #HumanSpaceflight #STEM #Education #HD #Video

Pan of Spiral Galaxy UGC 10043 in Serpens | Hubble Space Telescope

Pan of Spiral Galaxy UGC 10043 in Serpens | Hubble Space Telescope

What kind of astronomical object is this? It does not look quite like the kinds of galaxies, nebulae, star clusters or galaxy clusters that Hubble normally brings us images of. In fact, this is a spiral galaxy, named UGC 10043—we just happen to be seeing it directly from the side. Located roughly 150 million light-years from Earth in the constellation Serpens, UGC 10043 is one of the rare spiral galaxies that are seen edge-on from our perspective.

From this point of view, we see the galaxy’s disc as a sharp line through space, overlain with a prominent dust lane. This dust is spread across the spiral arms of UGC 10043, but it looks very thick and cloudy when viewed from the side. You can even see the lights of active star-forming regions in the arms, shining out from behind the dust. Strikingly, we can also see that the center of the galaxy sports a glowing, almost egg-shaped ‘bulge’, rising far above and below the disc. 

All spiral galaxies have a bulge like this one as part of their structure, containing stars that orbit the galactic center on paths above and below the whirling disc; it is a feature that is not normally obvious in pictures of galaxies. The unusually large size of this bulge compared to the galaxy’s disc is possibly thanks to UGC 10043 siphoning material from a nearby dwarf galaxy. This may also be why the disc is warped, bending up at one end and down at the other.

Like most full-color Hubble images, this is a composite, made up of several individual snapshots capturing unique light wavelengths. 

Image Description: A spiral galaxy seen directly from the side, such that its disc looks like a narrow diagonal band across the image. A band of dark dust covers the disc in the center most of the way out to the ends, and the disc glows around that. In the center a whitish circle of light bulges out above and below the disc. The tips of the disc are a bit bent. The background is black and mostly empty.


Credit: European Space Agency (ESA)/Hubble & NASA, R. Windhorst, W. Keel
Duration: 30 seconds
Release Date: Nov. 18, 2024


#NASA #ESA #Astronomy #Space #Hubble #Galaxies #Galaxy #UGC10043 #SpiralGalaxy #GalacticBulge #InteractingGalaxies #DwarfGalaxy #SerpensCaput #Constellation #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

Spiral Galaxy UGC 10043 in Serpens: Side Profile & Central Bulge | Hubble

Spiral Galaxy UGC 10043 in Serpens: Side Profile & Central Bulge | Hubble


What kind of astronomical object is this? It does not look quite like the kinds of galaxies, nebulae, star clusters or galaxy clusters that Hubble normally brings us images of. In fact, this is a spiral galaxy, named UGC 10043—we just happen to be seeing it directly from the side. Located roughly 150 million light-years from Earth in the constellation Serpens, UGC 10043 is one of the rare spiral galaxies that are seen edge-on from our perspective.

From this point of view, we see the galaxy’s disc as a sharp line through space, overlain with a prominent dust lane. This dust is spread across the spiral arms of UGC 10043, but it looks very thick and cloudy when viewed from the side. You can even see the lights of active star-forming regions in the arms, shining out from behind the dust. Strikingly, we can also see that the center of the galaxy sports a glowing, almost egg-shaped ‘bulge’, rising far above and below the disc. 

All spiral galaxies have a bulge like this one as part of their structure, containing stars that orbit the galactic center on paths above and below the whirling disc; it is a feature that is not normally obvious in pictures of galaxies. The unusually large size of this bulge compared to the galaxy’s disc is possibly thanks to UGC 10043 siphoning material from a nearby dwarf galaxy. This may also be why the disc is warped, bending up at one end and down at the other.

Like most full-color Hubble images, this is a composite, made up of several individual snapshots capturing unique light wavelengths. 

Image Description: A spiral galaxy seen directly from the side, such that its disc looks like a narrow diagonal band across the image. A band of dark dust covers the disc in the center most of the way out to the ends, and the disc glows around that. In the center a whitish circle of light bulges out above and below the disc. The tips of the disc are a bit bent. The background is black and mostly empty.


Credit: European Space Agency (ESA)/Hubble & NASA, R. Windhorst, W. Keel
Release Date: Nov. 18, 2024


#NASA #ESA #Astronomy #Space #Hubble #Galaxies #Galaxy #UGC10043 #SpiralGalaxy #GalacticBulge #InteractingGalaxies #DwarfGalaxy #SerpensCaput #Constellation #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #Europe #STEM #Education

Leonids Meteor Shower Peaks November 18-24, 2024 | BBC Star Diary

Leonids Meteor Shower Peaks November 18-24, 2024 | BBC Star Diary

The Leonids meteor shower reaches the peak of activity this week. It might not be the best year for the shower, but fortunately we are on hand with many more stargazing highlights in this week’s Star Diary podcast, from the makers of BBC Sky at Night Magazine.

The Leonids, peaking during mid-November each year, are considered to be a major shower though meteor rates are often as low as about 15 meteors per hour. The Leonids are bright meteors and can also be colorful. They are also fast: Leonids travel at speeds of 44 miles (71 kilometers) per second, and they are considered to be some of the fastest meteors.

Every 33 years, or so, viewers on Earth may experience a Leonid storm that can peak with hundreds to thousands of meteors seen per hour depending on the location of the observer.

A meteor storm versus a shower is defined as having at least 1,000 meteors per hour. Viewers in 1966 experienced a spectacular Leonid storm: thousands of meteors per minute fell through Earth's atmosphere during a 15-minute period. There were so many meteors seen that they appeared to fall like rain. The last Leonid meteor storm took place in 2002.

Leonids are also known for their fireballs and Earth-grazer meteors. Fireballs are larger explosions of light and color that can persist longer than an average meteor streak. This is due to the fact that fireballs originate from larger particles of cometary material. Fireballs are also brighter with magnitudes brighter than -3. Earth-grazers are meteors that streak close to the horizon and are known for their long and colorful tails.

Where Do Meteors Come From?

Meteors come from leftover comet particles and bits from broken asteroids. When comets come around the Sun, the dust they emit gradually spreads into a dusty trail around their orbits. Every year the Earth passes through these debris trails, which allows the bits to collide with our atmosphere where they disintegrate to create fiery and colorful streaks in the sky.

The Comet

The pieces of space debris that interact with our atmosphere to create the Leonids originate from comet 55P/Tempel-Tuttle. It takes comet Tempel-Tuttle 33 years to orbit the sun once.

Comet Tempel-Tuttle was discovered twice independently—in 1865 and 1866 by Ernst Tempel and Horace Tuttle, respectively. Tempel-Tuttle is a small comet—its nucleus measures only about 2.24 miles (3.6 kilometers) across.

Learn more about the Leonids Meteor Shower:

https://science.nasa.gov/solar-system/meteors-meteorites/leonids/


Video Credit: BBC Sky at Night Magazine
Caption Credit: NASA Goddard/BBC
Duration: 16 minutes
Release Date: Nov. 17, 2024


#NASA #Space #Astronomy #Science #Earth #Meteors #Fireballs #MeteorShowers #Leonids #LeonidMeteorShower #Leo #Constellations #Planets #SolarSystem #Stars #StarClusters #MilkyWayGalaxy #Universe #Skywatching #BBC #UK #Britain #Europe #UnitedStates #Canada #NorthernHemisphere #STEM #Education #Podcast #HD #Video

Sunday, November 17, 2024

Wide-field view: Cosmic Bat Nebula (NGC 1788) in Orion | Digitized Sky Survey 2

Wide-field view: Cosmic Bat Nebula (NGC 1788) in Orion | Digitized Sky Survey 2

The delicate nebula NGC 1788 is located in a dark and often neglected corner of the constellation Orion. Although this ghostly cloud is rather isolated from Orion’s bright stars, their powerful winds and light have a strong impact on the nebula, forging its shape and making it a home to a multitude of infant suns. This image from the Digitized Sky Survey 2 covers a field of view of 3 x 2.9 degrees, and shows that the Bat Nebula is part of much larger nebulosity.

Distance: 1,300 light years

The Digitized Sky Survey (DSS) is a ground-based imaging survey of the entire sky in several colors of light produced by the Space Telescope Science Institute through its Guide Star Survey group.


Image Credit: European Southern Observatory (ESO)/Digitized Sky Survey 2
Acknowledgement: Davide de Martin
Release Date: March 3, 2010


#NASA #ESO #Astronomy #Space #Science #Nebulae #Nebula #NGC1788 #ReflectionNebula #Orion #Cosmos #Universe #Chile #Europe #DSS2 #STScI #UnitedStates #STEM #Education

Journey to The Cosmic Bat Nebula: NGC 1788 in Orion | MPG/ESO Telescope

Journey to The Cosmic Bat Nebula: NGC 1788 in Orion | MPG/ESO Telescope


This zoom video starts with a wide view of the Milky Way and ends with a close-up look at the reflection nebula NGC 1788. Hidden in one of the darkest corners of the Orion constellation, this Cosmic Bat is spreading its hazy wings through interstellar space 1,300 light years away.

Although this ghostly cloud is rather isolated from Orion’s bright stars, their powerful winds and light have a strong impact on the nebula, forging its shape and making it a home to a multitude of infant suns.

The final close-up image was obtained using the Wide Field Imager on the MPG/ESO 2.2-meter telescope at the European Southern Observatory’s La Silla Observatory in Chile. It combines images taken through blue, green and red filters, as well as a special filter designed to let through the light of glowing hydrogen. The field is about 30 arcminutes across; North is up, and East to the left.


Credit: European Southern Observatory (ESO)/Digitized Sky Survey 2/N. Risinger
Duration: 50 seconds
Release Date: March 14, 2019

#NASA #ESO #Astronomy #Space #Science #Nebulae #Nebula #NGC1788 #ReflectionNebula #Orion #Cosmos #Universe #MPGESOTelescope #LaSillaObservatory #Chile #Europe #DSS2 #STScI #UnitedStates #STEM #Education #HD #Video

Close-up View of The Cosmic Bat Nebula: NGC 1788 in Orion | MPG/ESO Telescope

Close-up View of The Cosmic Bat Nebula: NGC 1788 in Orion | MPG/ESO Telescope


This video pans across the reflection nebula NGC 1788. Hidden in one of the darkest corners of the Orion constellation, this Cosmic Bat is spreading its hazy wings through interstellar space 1,300 light years away.

Although this ghostly cloud is rather isolated from Orion’s bright stars, their powerful winds and light have a strong impact on the nebula, forging its shape and making it a home to a multitude of infant suns.

This image has been obtained using the Wide Field Imager on the MPG/ESO 2.2-meter telescope at the European Southern Observatory’s La Silla Observatory in Chile. It combines images taken through blue, green and red filters, as well as a special filter designed to let through the light of glowing hydrogen. The field is about 30 arcminutes across; North is up, and East to the left.


Credit: European Southern Observatory (ESO)
Duration: 25 seconds
Release Date: March 14, 2019

#NASA #ESO #Astronomy #Space #Science #Nebulae #Nebula #NGC1788 #ReflectionNebula #Orion #Cosmos #Universe #MPGESOTelescope #LaSillaObservatory #Chile #Europe #STEM #Education #HD #Video

The Cosmic Bat: Nebula NGC 1788 in Orion | ESO MPG/ESO Telescope

The Cosmic Bat: Nebula NGC 1788 in Orion | MPG/ESO Telescope

The delicate nebula NGC 1788, located in a dark and often neglected corner of the Orion constellation, is revealed in this finely nuanced image. Although this ghostly cloud is rather isolated from Orion’s bright stars, their powerful winds and light have a strong impact on the nebula, forging its shape and making it a home to a multitude of infant suns.

Distance: 1,300 light years

This image has been obtained using the Wide Field Imager on the MPG/ESO 2.2-meter telescope at the European Southern Observatory’s La Silla Observatory in Chile. It combines images taken through blue, green and red filters, as well as a special filter designed to let through the light of glowing hydrogen. The field is about 30 arcminutes across; North is up, and East to the left.


Credit: European Southern Observatory (ESO)
Release Date: March 3, 2010


#NASA #ESO #Astronomy #Space #Science #Nebulae #Nebula #NGC1788 #ReflectionNebula #Orion #Cosmos #Universe #MPGESOTelescope #LaSillaObservatory #Chile #Europe #STEM #Education

Aurora over Scotland

Aurora over Scotland



On Earth, auroras are mainly created by particles originally emitted by the Sun in the form of solar wind. When this stream of electrically charged particles gets close to our planet, it interacts with the magnetic field, which acts as a gigantic shield. While it protects Earth’s environment from solar wind particles, it can also trap a small fraction of them. Particles trapped within the magnetosphere—the region of space surrounding Earth in which charged particles are affected by its magnetic field—can be energized and then follow the magnetic field lines down to the magnetic poles. There, they interact with oxygen and nitrogen atoms in the upper layers of the atmosphere, creating the flickering, colorful lights visible in the polar regions here on Earth.

Earth auroras have different names depending on which pole they occur at. Aurora Borealis, or the northern lights, is the name given to auroras around the north pole and Aurora Australis, or the southern lights, is the name given for auroras around the south pole.

Learn more:
The Colors of the Aurora (National Park Service)
https://www.nps.gov/articles/-articles-aps-v8-i1-c9.htm

Image Credit & Copyright: Alan Tough
Location: Bishopmill, Scotland, United Kingdom
Image Dates: Nov. 8, 2024 


#NASA #Space #Science #Earth #Planet #Aurora #AuroraBorealis #NorthernLights #MagneticField #Magnetosphere #SolarWind #Sun #Astrophotography #Astrophotographer #AlanTough #Bishopmill #Scotland #UK #UnitedKingdom #STEM #Education

Saturday, November 16, 2024

Shenzhou-19 Crew Transfers Tianzhou-8 Cargo | China Space Station

Shenzhou-19 Crew Transfers Tianzhou-8 Cargo | China Space Station

China's Shenzhou-19 astronauts opened the hatch door of the Tianzhou-8 cargo spacecraft and began to move supplies and equipment to the Tiangong Space Station in orbit on the morning of Saturday, November 16. Tianzhou-8 carries about 6 tons of supplies, including provisions for the crew’s in-orbit stay, propellant, experimental devices, and over 400 kilograms of scientific materials. New Year gifts for the crew, celebrating the Year of the Snake, were also delivered. The delivery of Tianzhou-8 took a total of 3 hours and 17 minutes.

Alongside astronaut supplies and experimental equipment, the Tianzhou-8 cargo spacecraft carries bricks made of varying compositions from simulated lunar soil. These bricks will undergo exposure tests to assess their durability in extreme conditions and their potential use in constructing lunar stations.

The Long March-7 Y9 rocket carrying the spacecraft blasted off at 11:13 p.m. Beijing time on Friday, November 15, 2024, from the Wenchang Spacecraft Launch Site in south China's Hainan island province. About three hours later, the cargo spacecraft successfully docked with the China Space Station. 

Shenzhou-19 Crew:
Commander Cai Xuzhe (蔡旭哲)
Mission Specialist Wang Haoze (王浩泽)
Mission Specialist Song Lingdong (宋令东)

Video Credit: CCTV
Duration: 1 minute, 20 seconds
Release Date: Nov. 16, 2024

#NASA #Space #Science #Earth #China #中国 #Tianzhou8 #CargoSpacecraft #Shenzhou19 #神舟十九号 #Taikonauts #Astronauts #CSS #ChinaSpaceStation #中国空间站 #TiangongSpaceStation #SpaceLaboratory #CMSA #国家航天局 #HumanSpaceflight #CLEP #STEM #Education #HD #Video

The Soap Bubble Nebula: PN G75.5+1.7 in Cygnus | Mayall Telescope

The Soap Bubble Nebula: PN G75.5+1.7 in Cygnus | Mayall Telescope

Informally known as the "Soap Bubble Nebula", this planetary nebula (officially known as PN G75.5+1.7) was discovered by amateur astronomer Dave Jurasevich on July 6th, 2008. It was noted and reported by Keith Quattrocchi and Mel Helm on July 17, 2008. 

PN G75.5+1.7 is located in the constellation of Cygnus, not far from the Crescent Nebula (NGC 6888). It is embedded in a diffuse nebula which, in conjunction with its faintness, is the reason it was not discovered until recently. The spherical symmetry of the shell is remarkable, making it very similar to Abell 39.

This image was obtained with the 4-meter Kitt Peak Mayall Telescope on June 19th, 2009 in the H-alpha (orange) and [OIII] (blue) narrowband filters. In this image, north is to the left and east is down.


Credit: T. A. Rector/University of Alaska Anchorage, H. Schweiker/WIYN and NOIRLab/NSF/AURA
Release Date: Oct. 15, 2009


#NASA #Astronomy #Space #Science #Nebulae #Nebula #PlanetaryNebula #SoapBubbleNebula #PNG75517 #Cygnus #Constellation #MilkyWayGalaxy #Universe #MayallTelescope #KPNO #Arizona #NSF #AURA #UnitedStates #STEM #Education

Tianzhou-8 Cargo Spacecraft Supply Mission Recap | China Space Station

Tianzhou-8 Cargo Spacecraft Supply Mission Recap | China Space Station


China's Tianzhou-8 cargo spacecraft successfully docked with the orbiting Tiangong Space Station on Saturday, November 16, 2024, at 2:32am Beijing time, the China Manned Space Agency (CMSA) announced. Tianzhou-8 completed a 3-hour rapid autonomous rendezvous and docking approach. This will mark the establishment of a standard docking mode for future missions that combines efficiency with reliability. The Shenzhou-19 crew, sent to the China Space Station on October 30, have entered the cargo spacecraft and begun to transfer items as scheduled.

China launched the Tianzhou-8 cargo spacecraft from the Wenchang Satellite Launch Center in its southern island province of Hainan using a Long March-7 Y9 carrier rocket on Friday night, November 15, 2024 at 11:32pm Beijing time. After about 10 minutes, the Tianzhou-8 separated from the rocket and entered its designated orbit. Its solar panels then unfolded. Tianzhou-8 has delivered supplies for the orbiting Tiangong Space Station, according to the China Manned Space Agency (CMSA). 

Alongside astronaut supplies and experimental equipment, the Tianzhou-8 cargo spacecraft carries bricks made of varying compositions from simulated lunar soil to the Tiangong Space Station. These bricks will undergo exposure tests to assess their durability in extreme conditions and their potential use in constructing lunar stations.

Compared to its predecessors, Tianzhou-6 and Tianzhou-7, the Tianzhou-8 cargo spacecraft boasts a larger cargo capacity—an increase of more than 200 more liters of space and more than 100 kilograms of cargo load.

Shenzhou-19 Crew:
Commander Cai Xuzhe (蔡旭哲)
Mission Specialist Wang Haoze (王浩泽)
Mission Specialist Song Lingdong (宋令东)

Video Credit: CCTV
Duration: 1 minute, 47 seconds
Release Date: Nov. 16, 2024

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Enter The Dragon | International Space Station

Enter The Dragon | International Space Station

NASA astronaut Don Pettit: "Floating down the dark tunnel leading to Crew-9 Dragon last month, when it was docked to the International Space Station. Node 2 forward."

The SpaceX Dragon Freedom crew spacecraft is assigned to NASA's SpaceX Crew-9 Mission.

Learn more about SpaceX's Dragon Spacecraft:

https://www.spacex.com/vehicles/dragon/

Enter the Dragon (Chinese: 龍爭虎鬥) is a 1973 martial arts film directed by Robert Clouse and written by Michael Allin. The film stars Bruce Lee, John Saxon, Ahna Capri, Bob Wall, Shih Kien and Jim Kelly. Enter the Dragon was Bruce Lee's final completed film appearance before his death on July 20, 1973, at the age of 32. An American-Hong Kong co-production, the film was premiered in Los Angeles on August 19, 1973, one month after Lee's death.

Expedition 72 Updates:


Expedition 72 Crew
Station Commander: Suni Williams
Roscosmos (Russia): Alexey Ovchinin, Ivan Vagner, Aleksandr Gorbunov
NASA: Butch Wilmore, Don Pettit, Nick Hague

An international partnership of space agencies provides and operates the elements of the International Space Station (ISS). The principals are the space agencies of the United States, Russia, Europe, Japan, and Canada.


Video Credit: NASA's Johnson Space Center (JSC)/D. Pettit
Duration: 22 seconds
Release Date: Nov. 15, 2024


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