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FEATURED NASA REPORT: Thanksgiving Celebrations in Space Bringing Family & Friends Together

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AceNewsDesk – The Thanksgiving holiday typically brings families and friends together in a celebration of common gratitude for all the good things that have happened during the previous year

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Ace Press News From Cutting Room Floor: Published: Nov.23: 2023: NASA News: TELEGRAM Ace Daily News Link https://t.me/+PuI36tlDsM7GpOJe

People celebrate the holiday in various ways, with parades, football marathons, and attending religious services, but food remains the over-arching theme. For astronauts embarked on long-duration space missions, separation from family and friends is inevitable and they rely on fellow crew members to share in the tradition and enjoy the culinary traditions as much as possible. In this most unusual of years when the pandemic may alter typical Thanksgiving gatherings, it seems appropriate to review how astronauts over the years have celebrated the holiday during their time in space. Enjoy the stories and photographs from orbital Thanksgiving celebrations over the years.

Skylab 4 astronauts Gerald P. Carr, Edward G. Gibson, and William R. Pogue
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Gibson, Pogue, and Carr demonstrate eating aboard Skylab
Thanksgiving 1973. Left: Skylab 4 astronauts Gerald P. Carr, Edward G. Gibson, and William R. Pogue, the first crew to celebrate Thanksgiving in space. Right: Gibson, left, Pogue, and Carr demonstrate eating aboard Skylab.

Skylab 4 astronauts Gerald P. Carr, Edward G. Gibson, and William R. Pogue were the first crew to celebrate Thanksgiving in space on Nov. 22, 1973. On that day, their seventh of an 84-day mission, Gibson and Pogue completed a 6-hour and 33-minute spacewalk, while Carr remained in the Multiple Docking Adaptor with no access to food. All three made up for missing lunch by consuming two meals at dinner time, although neither included special items for Thanksgiving.

STS-61B payload specialists Charles D. Walker and Rodolfo Neri Vela of Mexico enjoy the first Thanksgiving aboard a space shuttle in Atlantis’ middeck
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Image of the STS-61B crew enjoying their Thanksgiving dinner while floating in Atlantis’ middeck
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Mexican payload specialist Neri Vela
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Thanksgiving 1985. Left: STS-61B payload specialists Charles D. Walker, left, and Rodolfo Neri Vela of Mexico enjoy the first Thanksgiving aboard a space shuttle in Atlantis’ middeck. Middle: The STS-61B crew enjoying their Thanksgiving dinner while floating in Atlantis’ middeck. Right: Mexican payload specialist Neri Vela, who introduced tortillas to space menus.

Twelve years passed before the next orbital Thanksgiving celebration. On Nov. 28, 1985, the seven-member crew of STS-61B, NASA astronauts Brewster H. Shaw, Bryan D. O’Connor, Jerry L. Ross, Mary L. Cleave, and Sherwood C. β€œWoody” Spring, and payload specialists Charles D. Walker from the United States and Rodolfo Neri Vela from Mexico, feasted on shrimp cocktail, irradiated turkey, and cranberry sauce aboard the space shuttle Atlantis. Neri Vela introduced tortillas to space menus, and they have remained favorites among astronauts ever since. Unlike regular bread, tortillas do not create crumbs, a potential hazard in weightlessness, and have multiple uses for any meal of the day. The crew of STS-33, NASA astronauts Frederick D. Gregory, John E. Blaha, Manley L. β€œSonny” Carter, F. Story Musgrave, and Kathryn C. Thornton, celebrated Thanksgiving aboard space shuttle Discovery in 1989. Gregory and Musgrave celebrated their second Thanksgiving in space two years later, joined by fellow STS-44 NASA astronauts Terrence T. β€œTom” Henricks, James S. Voss, Mario Runco, and Thomas J. Hennen aboard space shuttle Atlantis.

STS-80 astronauts Tamara E. Jernigan, left, Kent V. Rominger, and Thomas D. Jones enjoy Thanksgiving dinner in Columbia’s middeck
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The STS-80 crew during aboard Columbia exchanging Thanksgiving greetings with John E. Blaha aboard the Mir space station
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Thanksgiving 1996. Left: STS-80 astronauts Tamara E. Jernigan, left, Kent V. Rominger, and Thomas D. Jones enjoy Thanksgiving dinner in Columbia’s middeck. Right: The STS-80 crew during aboard Columbia exchanging Thanksgiving greetings with John E. Blaha aboard the Mir space station.

In 1996, Blaha celebrated his second Thanksgiving in space with Russian cosmonauts Valeri G. Korzun and Aleksandr Y. Kaleri aboard the space station Mir. Blaha watched the beautiful Earth through the Mir windows rather than his usual viewing fare of football. The STS-80 crew of NASA astronauts Kenneth D. Cockrell, Kent V. Rominger, Tamara E. Jernigan, Thomas D. Jones, and Musgrave, now on his third turkey day holiday in orbit, celebrated Thanksgiving aboard space shuttle Columbia. Although the eight crew members were in different spacecraft in different orbits, they exchanged holiday greetings via space-to-space radio. This marked the largest number of people in space on Thanksgiving Day up to that time. One year later, NASA astronaut David A. Wolf celebrated Thanksgiving with his Russian crewmates Anatoli Y. Solovev, who translated the holiday into Russian as den blagodarenia, and Pavel V. Vinogradov aboard Mir. They enjoyed smoked turkey, freeze-dried mashed potatoes, peas, and milk. Also in orbit at the time was the crew of STS-87, NASA astronauts Kevin R. Kregel, Steven W. Lindsey, Kalpana Chawla, and Winston E. Scott, Takao Doi of the Japan Aerospace Exploration Agency, and Leonid K. Kadenyuk of Ukraine, aboard Columbia. The nine crew members aboard the two spacecraft broke the one-year-old record for the largest number of people in space at one time for Thanksgiving, also setting the record for the most nations represented, four.

NASA astronaut Frank L. Culbertson, left, and Vladimir N. Dezhurov of Roscosmos
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Dezhurov and Mikhail V. Tyurin of Roscosmos
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Mikhail V. Tyurin and Frank L. Culbertson
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Thanksgiving 2001, Expedition 3 crewmembers enjoying Thanksgiving dinner aboard the space station. Left: NASA astronaut Frank L. Culbertson, left, and Vladimir N. Dezhurov of Roscosmos. Middle: Dezhurov, left, and Mikhail V. Tyurin of Roscosmos. Right: Tyurin, left, and Culbertson.

The Expedition 1 crew of NASA astronaut William M. Shepherd, and Yuri P. Gidzenko and Sergei K. Krikalev of Roscosmos celebrated the first Thanksgiving aboard the International Space Station on Nov. 23, 2000, three weeks after their arrival aboard the facility. The crew took time out of their busy schedule to enjoy ham and smoked turkey and send words of thanks to people on the ground who provided excellent support to their flight. Crews have celebrated Thanksgiving in space every November since then. In 2001, Expedition 3 crew members NASA astronaut Frank L. Culbertson, and Vladimir N. Dezhurov and Mikhail V. Tyurin of Roscosmos enjoyed the first real Thanksgiving aboard the space station, complete with a cardboard turkey as decoration. The following year’s orbital Thanksgiving celebration included the largest number of people to that time, the combined 10 crewmembers of Expedition 5, STS-113, and Expedition 6.  After a busy day that included the first Thanksgiving Day spacewalk aboard the space station, the crews settled down to a dinner of smoked turkey, mashed potatoes, and green beans with mushrooms. Blueberry-cherry cobbler rounded out the meal.

Photo of the Thanksgiving dinner reheating in space shuttle Endeavour’s food warmer
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The crews of Expedition 18 and STS-126 share a meal in the space shuttle middeck
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Thanksgiving 2008. Left: The Thanksgiving dinner reheating in space shuttle Endeavour’s food warmer. Right: The crews of Expedition 18 and STS-126 share a meal in the space shuttle middeck.

Expedition 18 crew members NASA astronauts E. Michael Fincke and Gregory E. Chamitoff and Yuri V. Lonchakov representing Roscosmos, welcomed the STS-126 crew of NASA astronauts Christopher J. Ferguson, Eric A. Boe, Heidemarie M. Stefanyshyn-Piper, Donald R. Pettit, Stephen G. Bowen, R. Shane Kimbrough, and Sandra H. Magnus during Thanksgiving in 2008. They dined in the space shuttle Endeavour’s middeck on smoked turkey, candied yams, green beans and mushrooms, cornbread dressing and a cranapple dessert. 

Crew members from Expedition 21 and STS-129 share an early Thanksgiving meal
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Thanksgiving 2009. Left: Crew members from Expedition 21 and STS-129 share an early Thanksgiving meal. Right: The Thanksgiving dinner for the Expedition 21 and STS-129 crews.

The following year saw the largest and an internationally diverse group celebrating Thanksgiving in space. The six Expedition 21 crew members, NASA astronauts Jeffrey N. Williams and Nicole P. Stott, Roman Y. Romanenko and Maksim V. Suraev of Roscosmos, Frank L. DeWinne of the European Space Agency, and Robert B. Thirsk of the Canadian Space Agency hosted the six members of the STS-129 crew, NASA astronauts Charles O. Hobaugh, Barry E. Wilmore, Michael J. Foreman, Robert L. Satcher, Randolph J. Bresnik, and Leland D. Melvin. The twelve assembled crew members represented the United States, Russia, Belgium, and Canada. The celebration took place two days early, since the shuttle undocked from the space station on Thanksgiving Day.

Expedition 25 commander and NASA astronaut Scott J. Kelly awaits his crewmates at the Thanksgiving dinner table
The Expedition 25 crew of Oleg I. Skripochka of Roscosmos, left, Kelly, NASA astronaut Douglas H. Wheeler, Aleksandr Y. Kaleri and Fyodor N. Yurchikhin of Roscosmos, and NASA astronaut Shannon Walker sending Thanksgiving greetings to the ground before digging into their dinner

Thanksgiving 2010. Left: Expedition 25 commander and NASA astronaut Scott J. Kelly awaits his crewmates at the Thanksgiving dinner table. Right: The Expedition 25 crew of Oleg I. Skripochka of Roscosmos, left, Kelly, NASA astronaut Douglas H. Wheeler, Aleksandr Y. Kaleri and Fyodor N. Yurchikhin of Roscosmos, and NASA astronaut Shannon Walker sending Thanksgiving greetings to the ground before digging into their dinner.

Expedition 38 NASA astronauts Michael S. Hopkins, left, and Richard A. Mastracchio showing off food items destined for the Thanksgiving Day dinner
Close-up of the Thanksgiving dinner items, including turkey, ham, macaroni and cheese, green beans and mushrooms, and dressing

Thanksgiving 2013. Left: Expedition 38 NASA astronauts Michael S. Hopkins, left, and Richard A. Mastracchio showing off food items destined for the Thanksgiving Day dinner. Right: Close-up of the Thanksgiving dinner items, including turkey, ham, macaroni and cheese, green beans and mushrooms, and dressing.

Expedition 42 commander and NASA astronaut Barry E. β€œButch” Wilmore sets out his meal several days in advance
Expedition 42 crew members Wilmore, left, Samantha Cristoforetti of the European Space Agency, Aleksandr M. Samokutyayev and Anton N. Shkaplerov of Roscosmos, NASA astronaut Terry W. Virts, and Elena O. Serova of Roscosmos enjoy the Thanksgiving Day dinner

Thanksgiving 2014. Left: Eager for Thanksgiving, Expedition 42 commander and NASA astronaut Barry E. β€œButch” Wilmore sets out his meal several days in advance. Right: Expedition 42 crew members Wilmore, left, Samantha Cristoforetti of the European Space Agency, Aleksandr M. Samokutyayev and Anton N. Shkaplerov of Roscosmos, NASA astronaut Terry W. Virts, and Elena O. Serova of Roscosmos enjoy the Thanksgiving Day dinner.

Expedition 45 crew members Mikhail B. Korniyenko, left, Oleg D. Kononenko, and Sergei A. Volkov of Roscosmos, NASA astronaut Kjell N. Lindgren, Kimiya Yui of the Japan Aerospace Exploration Agency, and NASA astronaut Scott J. Kelly pose before the Thanksgiving dinner table
Kelly, left, and Lindgren show off the Thanksgiving dinner items
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Thanksgiving 2015. Left: Expedition 45 crew members Mikhail B. Korniyenko, left, Oleg D. Kononenko, and Sergei A. Volkov of Roscosmos, NASA astronaut Kjell N. Lindgren, Kimiya Yui of the Japan Aerospace Exploration Agency, and NASA astronaut Scott J. Kelly pose before the Thanksgiving dinner table. Right: Kelly, left, and Lindgren show off the Thanksgiving dinner items.

Expedition 50 crew members Oleg V. Novitsky, left, Sergei N. Ryzhikov, and Andrei I. Borisenko of Roscosmos, Thomas G. Pesquet of the European Space Agency, and NASA astronauts R. Shane Kimbrough and Peggy A. Whitson pose before the Thanksgiving dinner table
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Image of the Expedition 50 crew enjoying Thanksgiving feast
Thanksgiving 2016. Left: Expedition 50 crew members Oleg V. Novitsky, left, Sergei N. Ryzhikov, and Andrei I. Borisenko of Roscosmos, Thomas G. Pesquet of the European Space Agency, and NASA astronauts R. Shane Kimbrough and Peggy A. Whitson pose before the Thanksgiving dinner table. Right: The Expedition 50 crew tucks into the feast.
Thanksgiving table
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The Expedition 53 crew of Paolo A. Nespoli of the European Space Agency, left, NASA astronauts Joseph M. Acaba and Mark T. Vande Hei, Sergei N. Ryazansky and Aleksandr A. Misurkin of Roscosmos, and NASA astronaut Randolph J. Bresnik patiently awaits the start of the dinner
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The Expedition 53 crew eating Thanksgiving dinner
Thanksgiving 2017. Left: The Thanksgiving table is set. Middle: The Expedition 53 crew of Paolo A. Nespoli of the European Space Agency, left, NASA astronauts Joseph M. Acaba and Mark T. Vande Hei, Sergei N. Ryazansky and Aleksandr A. Misurkin of Roscosmos, and NASA astronaut Randolph J. Bresnik patiently awaits the start of the dinner. Right: The Expedition 53 crew digs in.
Image of turkey packages in the Galley Food Warmer
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Expedition 61 crew members NASA astronaut Christina H. Koch, left, Aleksandr A. Skvortsov of Roscosmos, NASA astronaut Jessica U. Meir, Oleg I. Skripochka of Roscosmos, NASA astronaut Andrew R. Morgan, and Luca S. Parmitano of the European Space Agency celebrate Thanksgiving aboard the space station
Thanksgiving 2019. Left: The turkey is in the oven, or more precisely the smoked turkey packages are in the Galley Food Warmer. Right: Expedition 61 crew members NASA astronaut Christina H. Koch, left, Aleksandr A. Skvortsov of Roscosmos, NASA astronaut Jessica U. Meir, Oleg I. Skripochka of Roscosmos, NASA astronaut Andrew R. Morgan, and Luca S. Parmitano of the European Space Agency celebrate Thanksgiving aboard the space station.
Expedition 64 NASA astronaut Kathleen H. β€œKate” Rubins prepares the Thanksgiving dinner
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The Expedition 64 crew of NASA astronaut Michael S. Hopkins, Soichi Noguchi of the Japan Aerospace Exploration Agency, Sergei V. Kud-Sverchkov and Sergei N. Ryzhikov of Roscosmos, and NASA astronauts K. Meghan McArthur, Victor J. Glover, and Rubins enjoying the Thanksgiving meal including frozen treats for dessert
Thanksgiving 2020. Left: Expedition 64 NASA astronaut Kathleen H. β€œKate” Rubins prepares the Thanksgiving dinner. Right: The Expedition 64 crew of NASA astronaut Michael S. Hopkins, Soichi Noguchi of the Japan Aerospace Exploration Agency, Sergei V. Kud-Sverchkov and Sergei N. Ryzhikov of Roscosmos, and NASA astronauts K. Meghan McArthur, Victor J. Glover, and Rubins enjoying the Thanksgiving meal including frozen treats for dessert.
Thanksgiving dinner cooking in the β€œoven” aboard the space station
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Expedition 66 crew members NASA astronauts Raja J. Chari, left, Kayla S. Barron, Mark T. Vande Hei, Thomas H. Marshburn, Russian cosmonauts Anton N. Shkaplerov and Pyotr V. Dubrov (partially visible), and European Space Agency astronaut Matthias J. Maurer (taking the photo) enjoy the Thanksgiving feast
Thanksgiving 2021. Left: Thanksgiving dinner cooking in the β€œoven” aboard the space station. Right: Expedition 66 crew members NASA astronauts Raja J. Chari, left, Kayla S. Barron, Mark T. Vande Hei, Thomas H. Marshburn, Russian cosmonauts Anton N. Shkaplerov and Pyotr V. Dubrov (partially visible), and European Space Agency astronaut Matthias J. Maurer (taking the photo) enjoy the Thanksgiving feast.
Expedition 68 crew members NASA astronauts Nicole A. Mann, left, Josh A. Cassada, and Francisco β€œFrank” C. Rubio, and Koichi Wakata of the Japan Aerospace Exploration Agency send Thanksgiving Day greetings
Thanksgiving 2022. Expedition 68 crew members NASA astronauts Nicole A. Mann, left, Josh A. Cassada, and Francisco β€œFrank” C. Rubio, and Koichi Wakata of the Japan Aerospace Exploration Agency send Thanksgiving Day greetings.
Expedition 70 crew members Andreas E. Mogensen, of the European Space Agency, front left, NASA astronauts Loral A. O’Hara and Jasmin Moghbeli, and Satoshi Furukawa of the Japan Aerospace Exploration Agency beam down their Thanksgiving message to everyone on the ground
Thanksgiving 2023. Expedition 70 crew members Andreas E. Mogensen, of the European Space Agency, front left, NASA astronauts Loral A. O’Hara and Jasmin Moghbeli, and Satoshi Furukawa of the Japan Aerospace Exploration Agency beam down their Thanksgiving message to everyone on the ground.

We hope you enjoyed these stories, photographs, and videos from Thanksgivings celebrated in space. We would like to wish everyone here on the ground and the seven-member crew of Expedition 70 aboard the space station a very happy Thanksgiving!

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Categories
Ace Breaking News

BREAKING NASA SPACE X REPORT: SpaceX loses contact with Starship mega rocket after explosions during second test flight

Starship launch
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AceBreakingNews – The Elon Musk-owned company says the latest mission will help improve the future reliability of the vehicle, which is a critical part of NASA’s ambitions to return astronauts to the moon.

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Ace Press News From Cutting Room Floor: Published: Nov.18: 2023: Sky News: TELEGRAM Ace Daily News Link https://t.me/+PuI36tlDsM7GpOJe

Starship launch
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SpaceX has lost contact with its Starship mega rocket following explosions during its second test flight from south Texas.

The two-stage 397ft rocket – the largest and most powerful ever built – arced out over the Gulf of Mexico after blasting off from the Elon Musk-owned company’s launch site near Boca Chica.

SpaceX was aiming for an altitude of 150 miles – just high enough for the spacecraft to travel around the globe before ditching into the Pacific near Hawaii 90 minutes after lift-off.

The two-stage 397ft rocket is the largest and most powerful ever built 

But while the super heavy first-stage booster appeared to have successfully separated it exploded a short time later.

The main Starship craft continued into space but a few moments later a company broadcaster said mission control had lost contact with the vehicle.

SpaceX’s livestream host John Insprucker said: “We have lost the data from the second stage… we think we may have lost the second stage.”

About eight minutes into the test mission, a camera view tracking the core Starship booster appeared to show an explosion that indicated the vehicle failed at that time on reaching an altitude of 91 miles (148km).

The company said in a post on the social media site X, formerly known as Twitter: “With a test like this, success comes from what we learn, and today’s test will help us improve Starship’s reliability as SpaceX seeks to make life multiplanetary.”

The Starship’s first flight, in April, lasted just four minutes before an explosion sent the wreckage crashing into the gulf.

The launch had been scheduled for Friday but was delayed by a day for a last-minute change of flight-control hardware.

Since then, SpaceX had made dozens of improvements to the booster and its 33 engines, as well as the launch pad.

The rocket is a critical part of NASA’s ambitions to return astronauts to the moon.

Mr Musk has also said that Starship could also be used for missions to Mars.

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Ace Daily News

FEATURED NASA NEWS & VIEWS REPORT: Will Saturn’s rings really ‘disappear’ by 2025? An astronomer explains

Saturn and its rings on a pitch black background.
As Saturn β€” seen here via NASA’s Cassini spacecraft β€” moves around the Sun, our viewpoint changes. (NASA/JPL-Caltech/Space Science Institute via Reuters )none

AceNewsDesk – If you can get your hands on a telescope, there are few sights more spectacular than the magnificent ringed planet β€” Saturn.

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Ace Press News From Cutting Room Floor: Published: Nov.12: 2023: Jonti Horner is professor of astrophysics at the University of Southern Queensland. This piece first appeared on The Conversation.TELEGRAM Ace Daily News Link https://t.me/+PuI36tlDsM7GpOJe

Saturn and its rings on a pitch black background.
As Saturn β€” seen here via NASA’s Cassini spacecraft β€” moves around the Sun, our viewpoint changes. (NASA/JPL-Caltech/Space Science Institute via Reuters )none

Currently, Saturn is clearly visible in the evening sky, at its highest just after sunset. It’s the ideal time to use a telescope or binoculars to get a good view of the Solar System’s sixth planet and its famous rings.

But in the past few days, a slew of articles have run like wildfire through social media. Saturn’s rings, those articles claim, are rapidly disappearing β€” and will be gone by 2025!

So what’s the story? Could the next couple of months, before Saturn drops out of view in the evening sky, really be our last chance to see its mighty rings?

The short answer is no. While it’s true the rings will become almost invisible from Earth in 2025, this is neither a surprise nor reason to panic. The rings will “reappear” soon thereafter. Here’s why.

Tipping and tilting Earth

To understand why our view of Saturn changes, let’s begin by considering Earth on its constant journey around the Sun. That journey takes us through the seasons β€” from winter to spring, summer and autumn, then back again.

What causes the seasons? Put simply, Earth is tilted towards one side, as seen from the Sun. Our equator is tilted by about 23.5 degrees from the plane of our orbit.Earth has seasons because its axis is tilted.

An illustration showing how the seasonal solstices occur as the Earth orbits the sun
The axis always points in the same direction as our planet orbits the Sun.(Supplied: Bureau of Meteorology)

The result?

As we move around the Sun, we alternately tip one hemisphere and then the other towards our star. When your home hemisphere is tilted more towards the Sun, you get longer days than nights and experience spring and summer. When you’re tilted away, you get shorter days and longer nights, and experience autumn and winter.

From the Sun’s viewpoint, Earth appears to “nod” up and down, alternately showing off its hemispheres as it moves around our star. Now, let’s move on to Saturn.

Saturn, a giant tilted world

Just like Earth, Saturn experiences seasons, but more than 29 times longer than ours. Where Earth’s equator is tilted by 23.5 degrees, Saturn’s equator has a 26.7 degree tilt. The result? As Saturn moves through its 29.4-year orbit around our star, it also appears to nod up and down as seen from both Earth and the Sun.

What about Saturn’s rings? The planet’s enormous ring system, comprised of bits of ice, dust and rocks, spreads out over a huge distance β€” just over 280,000km from the planet. But it’s very thin β€” in most places, just tens of metres thick. The rings orbit directly above Saturn’s equator and so they too are tilted to the plane of Saturn’s orbit.The planet’s enormous ring system β€” captured here by NASA’s Hubble Space Telescope β€” is comprised of bits of ice, dust and rocks.

A close up of Saturn's rings, which are beige on a black background.
(NASA, ESA, A Simon (GSFC), M H Wong (University of California, Berkeley) and the OPAL Team via Reuters )

So why do Saturn’s rings ‘disappear’?

The rings are so thin that, seen from a distance, they appear to vanish when edge on. You can visualise this easily by grabbing a sheet of paper, and rotating it until it is edge on β€” the paper almost vanishes from view.

As Saturn moves around the Sun, our viewpoint changes. For half of the orbit, its northern hemisphere is tilted towards us and the northern face of the planet’s rings is tipped our way.

When Saturn is on the other side of the Sun, its southern hemisphere is pointed our way. For the same reason, we see the southern face of the planet’s rings tilted our way.

The best way to illustrate this is to get your sheet of paper, and hold it horizontally β€” parallel to the ground β€” at eye level. Now, move the paper down towards the ground a few inches. What do you see? The upper side of the paper comes into view. Move the paper back up, through your eye line, to hold it above you and you can see the underside of the paper. But as it passes through eye level, the paper will all but disappear.

That’s what we see with Saturn’s rings. As the seasons on Saturn progress, we go from having the southern side of the rings tilted our way to seeing the northern side. Then, the planet tips back, revealing the southern side once more.

Twice per Saturnian year, we see the rings edge on and they all but vanish from view.

That’s what’s happening in 2025 β€” the reason Saturn’s rings will seemingly “disappear” is because we will be looking at them edge on.

This happens regularly. The last time was in 2009 and the rings gradually became visible again, over the course of a few months. The rings will be edge on once again in March 2025. Then they’ll gradually come back into view as seen through large telescopes, before sliding out of view again in November 2025.

Thereafter, the rings will gradually get more and more obvious, reappearing first to the largest telescopes over the months that follow. Nothing to worry about.

If you want to clearly see Saturn’s rings, now is your best chance, at least until 2027 or 2028!

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Global Warming & Climate Change

FEATURED NASA CLIMATE CHANGE WEATHER REPORT: Analysis Finds Strong El NiΓ±o Could Bring Extra Floods This Winter

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GlobalWarming & ClimateChange News Desk – An unusually high tide, called a King Tide, floods a highway on-ramp in Northern California in January 2023. Sea level rise and El NiΓ±os can exacerbate this type of flooding

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Ace Press News From Cutting Room Floor: Published: Nov.12: 2023: NASA Climate Change News: TELEGRAM Ace Daily News Link https://t.me/+PuI36tlDsM7GpOJe

California King Tides Project

Such high-tide flooding that inundates roads and buildings along the west coast of the Americas tends to be uncommon outside of El NiΓ±o years, but that could change by the 2030s.

An analysis by NASA’s sea level change science team finds that if a strong El NiΓ±o develops this winter, cities along the western coasts of the Americas could see an increase in the frequency of high-tide flooding that can swamp roads and spill into low-lying buildings.

El NiΓ±o is a periodic climate phenomenon characterized by higher-than-normal sea levels and warmer-than-average ocean temperatures along the equatorial Pacific. These conditions can spread poleward along the western coasts of the Americas. El NiΓ±o, which is still developing this year, can bring more rain than usual to the U.S. Southwest and drought to countries in the western Pacific like Indonesia. These impacts typically occur in January through March.

The NASA analysis finds that a strong El NiΓ±o could result in up to five instances of a type of flooding called a 10-year flood event this winter in cities including Seattle and San Diego. Places like La Libertad and Baltra in Ecuador could get up to three of these 10-year flood events this winter. This type of flooding doesn’t normally occur along the west coast of the Americas outside of El NiΓ±o years. The researchers note that by the 2030s, rising seas and climate change could result in these cities experiencing similar numbers of 10-year floods annually, with no El NiΓ±o required.

NASA/JPL-Caltech

Data from the SWOT satellite shows sea level anomalies – how much higher or lower sea levels are compared to the average height – off the coast of Ecuador and Peru on Aug. 12, 2023, and Oct. 3, 2023. The data indicates the development of an El NiΓ±o along the west coast of the Americas.

β€œI’m a little surprised that the analysis found these 10-year events could become commonplace so quickly,” said Phil Thompson, an oceanographer at the University of Hawaii and a member of NASA’s sea level change science team, which performed the analysis. β€œI would have thought maybe by the 2040s or 2050s.”

Ten-year floods are those that have a one in 10 chance of occurring in any given year. They’re a measure of how high local sea levels become: The extent of flooding in a particular city or community depends on several factors, including a region’s topography and the location of homes and infrastructure relative to the ocean. Ten-year floods can result in what the National Oceanic and Atmospheric Administration classifies as moderate flooding, with some inundation of roads and buildings, and the possible need to evacuate people or move belongings to higher ground.

NASA’s coastal flooding analysis finds that by the 2030s, during strong El NiΓ±o years, cities on the west coast of the Americas could see up to 10 of these 10-year flood events. By the 2050s, strong El NiΓ±os may result in as many as 40 instances of these events in a given year.

Watching Sea Levels Rise

Water expands as it warms, so sea levels tend to be higher in places with warmer water. Researchers and forecasters monitor ocean temperatures as well as water levels to spot the formation and development of an El NiΓ±o.

β€œClimate change is already shifting the baseline sea level along coastlines around the world,” said Ben Hamlington, a sea level researcher at NASA’s Jet Propulsion Laboratory in Southern California and lead for the agency’s sea level change science team.

Sea levels are rising in response to planetary warming, as Earth’s atmosphere and ocean are heating up and ice sheets and shelves melt. This has already increased the number of high-tide, or nuisance, flooding days coastal cities experience throughout the year. Phenomena like El NiΓ±os and storm surges, which temporarily boost sea levels, compound these effects.

Missions that monitor sea levels, including the Surface Water and Ocean Topography (SWOT) satellite and Sentinel-6 Michael Freilich, help to monitor El NiΓ±os in the near term. SWOT in particular, collects data on sea levels right up to the coast, which can help to improve sea level rise projections. That kind of information could aid policymakers and planners in preparing their communities for rising seas in the next decades.

β€œAs climate change accelerates, some cities will see flooding five to 10 times more often. SWOT will keep watch on these changes to ensure coastal communities are not caught off guard,” said Nadya Vinogradova Shiffer, SWOT program scientist and director of the ocean physics program at NASA Headquarters in Washington.  

To learn more about how NASA studies sea level, visit: https://sealevel.nasa.gov/

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Ace Breaking News

PRESS RELEASE NASA REPORT: First Science Images Released From ESA Mission Showing Galaxies 240 Million Light Years Away

A spiral galaxy is visible at the centre of the image. The galaxy is made up of spiral arms that wrap around a white central region. The arms are dusty and sprinkled with purple, pink, and white smudges. The background of space is filled with stars and points of light. A few of the stars are larger than the rest and have diffraction spikes.
ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi; CC BY-SA 3.0 IGO

AceBreakingNews – One of the first images captured by Euclid shows the Perseus cluster, a group of thousands of galaxies located 240 million light-years from Earth. The closest galaxies appear as swirling structures while hundreds of thousands of background galaxies are visible only as points of light

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Ace Press News From Cutting Room Floor: Published: Nov.08: 2023: NASA News: TELEGRAM Ace Daily News Link https://t.me/+PuI36tlDsM7GpOJe

The image shows thousands of galaxies across the black expanse of space. The closest thousand or so galaxies appear as small disks of spiraling material, surrounded by halos of yellow and white light. The background is scattered with a hundred thousand more distant galaxies of different shapes, ranging in color from white to yellow to red. Most galaxies are so far away they appear as single points of light.
ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi; CC BY-SA 3.0 IGO: The new images from the Euclid mission include a cluster of thousands of distant galaxies, demonstrating the spacecraft’s unique abilities.

The Euclid mission, which will investigate the mysteries of dark matter and dark energy, released its first five science images Tuesday, Nov. 7 The observatory, led by ESA (European Space Agency) with NASA contributions, is scheduled to begin regular science operations in early 2024.

The new images include views of a large cluster of thousands of distant galaxies, close-ups of two nearby galaxies, a gravitationally bound group of stars called a globular cluster, and a nebula (a cloud of gas and dust in space where stars form) – all depicted in vibrant colors.

β€œThe Euclid observatory will uncover a treasure trove of scientific discoveries that will be used across the world, including by U.S. scientists, for years to come,” said Nicola Fox, associate administrator, Science Mission Directorate, at NASA Headquarters in Washington. β€œTogether, NASA and ESA are paving the way for a new era of cosmology for NASA’s forthcoming Nancy Grace Roman Space Telescope, which will build upon what Euclid learns and will additionally survey objects on the outskirts of our solar system, discover thousands of new planets, explore nearby galaxies, and more.”

A spiral galaxy is visible at the centre of the image. The galaxy is made up of spiral arms that wrap around a white central region. The arms are dusty and sprinkled with purple, pink, and white smudges. The background of space is filled with stars and points of light. A few of the stars are larger than the rest and have diffraction spikes.
ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi; CC BY-SA 3.0 IGO

The spiral galaxy IC 342, located about 11 million light-years from Earth, lies behind the crowded plane of the Milky Way: Dust, gas, and stars obscure it from our view. Euclid used its near-infrared instrument to peer through the dust and study it.

Euclid launched on July 1 from Cape Canaveral, Florida, then traveled nearly 1 million miles to its vantage point. Following a period of commissioning (testing of the instruments and other components), the space telescope is performing as expected.

NASA’s Jet Propulsion Laboratory in Southern California delivered critical hardware for one of the Euclid spacecraft’s instruments. In addition, NASA has established a U.S.-based Euclid science data center, and NASA-funded science teams will join other Euclid scientists in studying dark energy, galaxy evolution, and dark matter. The agency’s Nancy Grace Roman mission will also study dark energy – in ways that are complementary to Euclid. Mission planners will use Euclid’s findings to inform Roman’s dark energy work.

Surveying the Dark Universe

During its planned six-year mission, Euclid will produce the most extensive 3D map of the universe yet, covering nearly one-third of the sky and containing billions of galaxies up to 10 billion light-years away from Earth.

ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi; CC BY-SA 3.0 IGO

The galaxy NGC 6822 is located 1.6 million light-years from Earth. Euclid was able to capture this view of the entire galaxy and its surroundings in high resolution in about one hour, which isn’t possible with ground-based telescopes or targeted telescopes (such as NASA’s Webb) that have narrower fields of view.

To do this, Euclid needs a wide field of view, which enabled these new images covering a relatively large area. In this way, Euclid differs from targeted observatories like NASA’s James Webb Space Telescope that focus on a smaller area of the sky at any one time but typically offer higher-resolution images. Wide-field observatories like Euclid can observe large sections of the sky much faster than targeted telescopes. In addition, Euclid has high resolution compared to previous survey missions, which means it will be able to see more galaxies in each image than previous telescopes.

For example, Euclid’s wide view was able to capture the entirety of the Perseus galaxy cluster, and many galaxies beyond it, in just one image. Located 240 million light-years from Earth, Perseus is among the most massive structures known in the universe. Euclid’s full survey will ultimately cover an area 30,000 times larger than this image.

This square astronomical image is divided horizontally by the edge of a white and orange cloud on the bottom half. Within this region is a section of cloud shaped like a horse’s head. The top half of the image contains a faint purple haze that fades away to reveal the blackness of space near the top of the image, which is speckled with stars.
ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi; CC BY-SA 3.0 IGO

The Horsehead Nebula, also known as Barnard 33, is part of the Orion constellation. About 1,375 light-years away, it is the closest giant star-forming region to Earth. With Euclid, which captured this image, scientists hope to find many dim and previously unseen Jupiter-mass planets in their celestial infancy, as well as baby stars. Full image here.

The telescope’s survey approach is necessary to study dark energy, the mysterious driver behind our universe’s accelerating expansion. While gravity should pull everything in the universe together, everything is instead moving apart faster and faster. β€œDark energy” is the term scientists use for this unexplained expansion.

To study the phenomenon, scientists will map the presence of another cosmic mystery, dark matter. This invisible substance can be observed only by its gravitational effect on β€œregular” matter and objects around it, like stars, galaxies, and planets. Dark matter is five times more common in the cosmos than regular matter, so if dark energy’s expansive influence on the universe has changed over time, the change should be recorded in how dark matter is distributed on large scales across the universe, and Euclid’s 3D map should capture it.

ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi; CC BY-SA 3.0 IGO

This sparkly image shows Euclid’s view of a globular cluster – a collection of gravitationally bound stars that don’t quite form a galaxy – called NGC 6397. No other telescope can capture an entire globular cluster in a single observation and distinguish so many stars within it.

β€œEuclid’s first images mark the beginning of a new era of studying dark matter and dark energy,” said Mike Seiffert, Euclid project scientist at JPL. β€œThis is the first space telescope dedicated to dark universe studies, and the sheer scale of the data we’re going to get out of this will be unlike anything we’ve had before. These are big mysteries, so it’s exciting for the international cosmology community to see this day finally arrive.”

NASA’s Roman mission will study a smaller section of sky than Euclid, but it will provide higher-resolution images of hundreds of millions of galaxies and peer deeper into the universe’s past, providing complementary information. Scheduled to launch by May 2027.

The data from the new Euclid images is now available to the scientific community, and scientific papers analysing that data are expected to follow. As the mission progresses, Euclid’s bank of data will grow. New batches will be released once per year and will be available to the global scientific community via the Astronomy Science Archives hosted at ESA’s European Space Astronomy Centre in Spain.

More About the Mission

Euclid is a European mission, built and operated by ESA, with contributions from NASA. The Euclid Consortium – consisting of more than 2,000 scientists from 300 institutes in 13 European countries, the U.S., Canada, and Japan – is responsible for providing the scientific instruments and scientific data analysis. ESA selected Thales Alenia Space as prime contractor for the construction of the satellite and its service module, with Airbus Defence and Space chosen to develop the payload module, including the telescope. NASA provided the detectors of the Near-Infrared Spectrometer and Photometer, NISP. Euclid is a medium-class mission in ESA’s Cosmic Vision Programme.

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A spiral galaxy is visible at the centre of the image. The galaxy is made up of spiral arms that wrap around a white central region. The arms are dusty and sprinkled with purple, pink, and white smudges. The background of space is filled with stars and points of light. A few of the stars are larger than the rest and have diffraction spikes.
ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre (CEA Paris-Saclay), G. Anselmi; CC BY-SA 3.0 IGO
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Ace Breaking News

NASA CLIMATE CHANGE WEATHER REPORT: International Ocean Satellite Monitors How El NiΓ±o Is Shaping Up

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AceBreakingNews – Sentinel-6 Michael Freilich is the latest satellite contributing to a 30-year sea level record that researchers are using to compare this year’s El NiΓ±o with those of the past.

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Ace Press News From Cutting Room Floor: Published: Nov.03: 2023: NASA News: TELEGRAM Ace Daily News Link https://t.me/+PuI36tlDsM7GpOJe

In Brief:

Not all El NiΓ±o events are created equal. Their impacts vary widely, and satellites like the U.S.-European Sentinel-6 Michael Freilich help anticipate those impacts on a global scale by tracking changes in sea surface height in the Pacific Ocean.

Water expands as it warms, so sea levels tend to be higher in places with warmer water. El NiΓ±os are characterized by higher-than-normal sea levels and warmer-than-average ocean temperatures along the equatorial Pacific. These conditions can then propagate poleward along the western coasts of the Americas. El NiΓ±os can bring wetter conditions to the U.S. Southwest and drought to regions in the western Pacific, including Indonesia. This year’s El NiΓ±o is still developing, but researchers are looking to the recent past for clues as to how it is shaping up.

There have been two extreme El NiΓ±o events in the past 30 years: the first from 1997 to 1998 and the second from 2015 to 2016. Both caused shifts in global air and ocean temperatures, atmospheric wind and rainfall patterns, and sea level. The maps above show sea levels in the Pacific Ocean during early October of 1997, 2015, and 2023, with higher-than-average ocean heights in red and white, and lower-than-average heights in blue and purple. Sentinel-6 Michael Freilich captured the 2023 data, the TOPEX/Poseidon satellite collected data for the 1997 image, and Jason-2 gathered data for the 2015 map.

By October 1997 and 2015, large areas of the central and eastern Pacific had sea levels more than 7 inches (18 centimeters) higher than normal. This year, sea levels are about 2 or 3 inches (5 to 8 centimeters) higher than average and over a smaller area compared to the 1997 and 2015 events. Both of the past El NiΓ±os reached peak strength in late November or early December, so this year’s event may still intensify.

β€œEvery El NiΓ±o is a little bit different,” said Josh Willis, Sentinel-6 Michael Freilich project scientist at NASA’s Jet Propulsion Laboratory in Southern California. β€œThis one seems modest compared to the big events, but it could still give us a wet winter here in the Southwest U.S. if conditions are right.”

More About the Mission

Launched in November 2020, Sentinel-6 Michael Freilich is named after former NASA Earth Science Division Director Michael Freilich. The satellite is one of two that compose the Copernicus Sentinel-6/Jason-CS (Continuity of Service) mission.

Sentinel-6/Jason-CS was jointly developed by ESA (European Space Agency), the European Organisation for the Exploitation of Meteorological Satellites (EUMETSAT), NASA, and the U.S. National Oceanic and Atmospheric Administration, with funding support from the European Commission and technical support on performance from the French space agency CNES (Centre National d’Études Spatiales).

To learn more about Sentinel-6 Michael Freilich, visit: https://www.nasa.gov/sentinel-6

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Global Warming & Climate Change

FEATURED NASA GLOBAL WARMING SWOT REPORT: See Mission’s Unprecedented View of Global Sea Levels

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AceNewsDesk – This animation shows global sea level data collected by the Surface Water and Ocean Topography satellite from July 26 to Aug. 16. Red and orange indicate higher-than-average ocean heights, while blue represents lower-than-average heights.

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Ace Press News From Cutting Room Floor: Published: Nov.03: 2023: NASA News: TELEGRAM Ace Daily News Link https://t.me/+PuI36tlDsM7GpOJe

Credit: NASA/JPL-Caltech

In Brief:

Data on sea surface heights around the world from the international Surface Water and Ocean Topography mission yields a mesmerizing view of the planet’s ocean.

The Surface Water and Ocean Topography (SWOT) satellite is sending down tantalizing views of Earth’s water, including a global composite of sea surface heights. The satellite collected the data visualized above during SWOT’s first full 21-day science orbit, which it completed between July 26 and Aug. 16.

SWOT is measuring the height of nearly all water on Earth’s surface, providing one of the most detailed, comprehensive views yet of the planet’s oceans and freshwater lakes and rivers. The satellite is a collaboration between NASA and the French space agency, CNES (Centre National d’Études Spatiales).

The animation shows sea surface height anomalies around the world: Red and orange indicate ocean heights that were higher than the global mean sea surface height, while blue represents heights lower than the mean.

Sea level differences can highlight ocean currents, like the Gulf Stream coming off the U.S. East Coast or the Kuroshio current off the east coast of Japan. Sea surface height can also indicate regions of relatively warmer water – like the eastern part of the equatorial Pacific Ocean during an El NiΓ±o – because water expands as it warms.

The SWOT science team made the measurements using the groundbreaking Ka-band Radar Interferometer (KaRIn) instrument. With two antennas spread 33 feet (10 meters) apart on a boom, KaRIn produces a pair of data swaths (tracks visible in the animation) as it circles the globe, bouncing radar pulses off the water’s surface to collect surface-height measurements.

β€œThe detail that SWOT is sending back on sea levels around the world is incredible,” said Parag Vaze, SWOT project manager at NASA’s Jet Propulsion Laboratory in Southern California. β€œThe data will advance research into the effects of climate change and help communities around the world better prepare for a warming world.”

More About the Mission

LaunchedΒ on Dec. 16, 2022, from Vandenberg Space Force Base in central California, SWOT is now in its operations phase, collecting data that will be used for research and other purposes.

SWOT was jointly developed by NASA and CNES, with contributions from CSA (Canadian Space Agency) and the UK Space Agency. JPL, which is managed for the agency by Caltech in Pasadena, California, leads the U.S. component of the project. For the flight system payload, NASA provided the KaRIn instrument, a GPS science receiver, a laser retroreflector, a two-beam microwave radiometer, and NASA instrument operations. CNES provided the Doppler Orbitography and Radioposition Integrated by Satellite (DORIS) system, the dual frequency Poseidon altimeter (developed by Thales Alenia Space), the KaRIn radio-frequency subsystem (together with Thales Alenia Space and with support from the UK Space Agency), the satellite platform, and ground operations. CSA provided the KaRIn high-power transmitter assembly. NASA provided the launch vehicle and the agency’s Launch Services Program, based at Kennedy Space Center, managed the associated launch services.

To learn more about SWOT, visit:
https://swot.jpl.nasa.gov/

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Ace Daily News

FEATURED NASA REPORT: Rocket to See Sizzling Edge of Star-Forming Supernova

This image taken by NASA’s Hubble Space Telescope shows part of the Veil Nebula or Cygnus Loop. To create this colorful image, observations were taken by Hubble’s Wide Field Camera 3 instrument using five different filters. New post-processing methods have further enhanced details of emissions from doubly ionized oxygen (shown here in shades of blue), ionized hydrogen, and ionized nitrogen (shown here in shades of red).

AceNewsDesk – A new sounding rocket mission is headed to space to understand how explosive stellar deaths lay the groundwork for new star systems. The Integral Field Ultraviolet Spectroscopic Experiment, or INFUSE, sounding rocket mission, will launch from the White Sands Missile Range in New Mexico on Oct. 29, 2023, at 9:35 p.m. MDT.

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Ace Press News From Cutting Room Floor: Published: Oct.28: 2023: NASA by Published: October 26, 2023 2.36pm BST: TELEGRAM Ace Daily News Link https://t.me/+PuI36tlDsM7GpOJe

Miles Hatfield
Miles Hatfield: OCT 27, 2023

For a few months each year, the constellation Cygnus (Latin for β€œswan”) swoops through the northern hemisphere’s night sky. Just above its wing is a favorite target for backyard astronomers and professional scientists alike: the Cygnus Loop, also known as the Veil Nebula.

This image shows an illustration of the constellation Cygnus, Latin for β€œswan,” in the night sky. The Cygnus Loop supernova remnant, also known as the Veil Nebula, is located near one of the swan’s wings, outlined here in a rectangular box

NASA: The Cygnus Loop is the remnant of a star that was once 20 times the size of our Sun. Some 20,000 years ago, that star collapsed under its own gravity and erupted into a supernova. Even from 2,600 light-years away, astronomers estimate the flash of light would have been bright enough to see from Earth during the day.

This image taken by NASA’s Hubble Space Telescope shows part of the Veil Nebula or Cygnus Loop. To create this colorful image, observations were taken by Hubble’s Wide Field Camera 3 instrument using five different filters. New post-processing methods have further enhanced details of emissions from doubly ionized oxygen (shown here in shades of blue), ionized hydrogen, and ionized nitrogen (shown here in shades of red).

ESA/Hubble & NASA, Z. Levay

Supernovae are part of a great life cycle. They spray heavy metals forged in a star’s core into the clouds of surrounding dust and gas. They are the source of all chemical elements in our universe heavier than iron, including those that make up our own bodies. From the churned-up clouds and star stuff left in their wake, gases and dust from supernovae gradually clump together to form planets, stars, and new star systems.

β€œSupernovae like the one that created the Cygnus Loop have a huge impact on how galaxies form,” said Brian Fleming, a research professor at the University of Colorado Boulder and principal investigator for the INFUSE mission.

The Cygnus Loop provides a rare look at a supernova blast still in progress. Already over 120 light-years across, the massive cloud is still expanding today at approximately 930,000 miles per hour (about 1.5 million kilometers per hour).

What our telescopes capture from the Cygnus Loop is not the supernova blast itself. Instead, we see the dust and gas superheated by the shock front, which glows as it cools back down.

β€œINFUSE will observe how the supernova dumps energy into the Milky Way by catching light given off just as the blast wave crashes into pockets of cold gas floating around the galaxy,” Fleming said.

To see that shock front at its sizzling edge, Fleming and his team have developed a telescope that measures far-ultraviolet light – a kind of light too energetic for our eyes to see. This light reveals gas at temperatures between 90,000 and 540,000 degrees Fahrenheit (about 50,000 to 300,000 degrees Celsius) that is still sizzling after impact.

INFUSE is an integral field spectrograph, the first instrument of its kind to fly to space. The instrument combines the strengths of two ways of studying light: imaging and spectroscopy. Your typical telescopes have cameras that excel at creating images – showing where light is coming from, faithfully revealing its spatial arrangement. But telescopes don’t separate light into different wavelengths or β€œcolors” – instead, all of the different wavelengths overlap one another in the resulting image.

Spectroscopy, on the other hand, takes a single beam of light and separates it into its component wavelengths or spectrum, much as a prism separates light into a rainbow. This procedure reveals all kinds of information about what the light source is made of, its temperature, and how it is moving. But spectroscopy can only look at a single sliver of light at a time. It’s like looking at the night sky through a narrow keyhole.

The INFUSE instrument captures an image and then β€œslices” it up, lining up the slices into one giant β€œkeyhole.” The spectrometer can then spread each of the slices into its spectrum. This data can be reassembled into a 3-dimensional image that scientists call a β€œdata cube” – like a stack of images where each layer reveals a specific wavelength of light.

PhD student Emily Witt installs the delicate image slicer – the core optical technology for INFUSE – onto its mount in a CU-LASP clean room ahead of integration into the payload.

CU Boulder LASP/Brian Fleming

Using the data from INFUSE, Fleming and his team will not only identify specific elements and their temperatures, but they’ll also see where those different elements lie along the shock front.

β€œIt’s a very exciting project to be a part of,” said lead graduate student Emily Witt, also at CU Boulder, who led most of the assembly and testing of INFUSE and will lead the data analysis. β€œWith these first-of-their-kind measurements, we will better understand how these elements from the supernova mix with the environment around them. It’s a big step toward understanding how material from supernovas becomes part of planets like Earth and even people like us.”

To get to space, the INFUSE payload will fly aboard a sounding rocket. These nimble, crewless rockets launch into space for a few minutes of data collection before falling back to the ground. The INFUSE payload will fly aboard a two-stage Black Brant 9 sounding rocket, aiming for a peak altitude of about 150 miles (240 kilometers), where it will make its observations, before parachuting back to the ground to be recovered. The team hopes to upgrade the instrument and launch again. In fact, parts of the INFUSE rocket are themselves repurposed from the DEUCE mission, which launched from Australia in 2022.

NASA’s Sounding Rocket Program is conducted at the agency’s Wallops Flight Facility at Wallops Island, Virginia, which is managed by NASA’s Goddard Space Flight Center in Greenbelt, Maryland. NASA’s Heliophysics Division manages the sounding rocket program for the agency. The development of the INFUSE payload was supported by NASA’s Astrophysics Division.


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