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“We’re coming up on the plumes!” The co-pilot announced over the intercom.

The other six passengers and I took our positions along the viewing cupola at the belly of the “Tour Bus”, and each grabbed on to the hand and foot restraints to keep ourselves in place in the weightlessness. We were traveling about 1000 miles above the south pole of Enceladus looking down at the highly reflective surface that was so bright it took about a minute for our eyes to adjust. We all remained silent, and my heart was pounding in anticipation. The Tour Bus silently coasted for a few more minutes as we took in the breathtaking view of Saturn’s sixth-largest moon.

plumes 1
The water vapor plumes of Saturn’s moon Enceladus. (Credit: NASA/JPL/Space Science Institute)

Just then, tink. Another tink. Then another. We knew something was hitting the spacecraft, but we weren’t sure what. I got a sudden rush of fear and felt my heart jump to my throat. What was hitting us, and will it get bigger? Are we in danger? Why hasn’t the captain ordered us back to our seats? The sound got louder and more frequent and some of the passengers started to panic.

That was when we all saw it, the first of three “tiger stripes” that marked the south pole of Enceladus. Just then a small object the size of a pea struck the cupola directly in front of my face and caused me to jump back, but I forced myself to hold on to the restraints. Another one struck. Then another. This was when we all realized the initial sounds were ice particles emanating from the plumes and striking the Tour Bus, all being catapulted out of the moon through the stripes and into space. The particles continued to strike the cupola and harmlessly bounce off while we watched in amazement. The Tour Bus continued to pass over the three stripes one at a time as we gazed down into the giant fissures where the particles came from, knowing that mere seconds earlier they were liquid water that swirled around inside the icy moon. We all strained to see down into the fissures to try and see the bottom, but to no avail. What was down there in the swirling depths? Was there life? Was it like life on Earth, or something more different? More alien? All we knew was these ice particles were from an alien world.

These are the Plumes of Enceladus.

—————————————————–

While Enceladus was first discovered by William Herschel in 1789, it didn’t get its first closeup study until it was visited by NASA’s Voyager 2 spacecraft, which revealed a differentiated surface with some heavily crated areas while other areas appeared to be crater-free. The plumes themselves went unnoticed until NASA’s Cassini spacecraft first imaged water and other volatiles erupting from the south pole in January and February 2005.

Cassini’s mass spectrometer ultimately detected an abundance of organic molecules—the building blocks of life—emanating from the satellite’s interior ocean. In March 2008, Cassini flew through the plumes and identified methane, molecular hydrogen, carbon dioxide, and rock fragments while measuring the speed of the material being catapulted from the moon at 1,300 km/hour (800 miles/hour). The source of the plumes is from the three “tiger stripes” at the south pole, which are four linear fractures generally measuring 130 km (80 miles) in length, 2 km (1.2 miles) wide, and 500 meters (1640 feet) deep, and bordered by 100-meter-high (328-feet-high) ridges.

tiger stripes
“Tiger stripes” of Enceladus. (Credit: NASA/European Space Agency/JPL/Cassini Imaging Team)

While existence of the plumes is indicative of an interior ocean, there has been debate on how much of an ocean exists beneath
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Day Has Returned, but India’s Lander and Rover have Failed to Wake Up

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8 hours ago

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September 27, 2023

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India Moon Rover Traverse

It looks like India’s Chandrayaan-3 succumbed to the cold, and its mission is over. The frigid lunar night lasted about two weeks, and a new day has dawned. With that day came hopes of a sunlit revival for the lander and the rover, but the India Space Research Organization (ISRO) says the chances of the spacecraft awakening in the Sun are diminishing by the hour.

The lunar night that wrapped its cold arms around the lander and rover lasted 14 days, and so will the current lunar day. When the day dawned last Friday, ISRO began trying to communicate with the lander. There’s been no response so far, as both explorers may be forever entombed about 600km (373 mi) from the Moon’s south pole.

Even though things don’t look good for the mission, it’s still a success. It’s the first spacecraft to land in the Moon’s south pole region. The area is critical because it contains vast quantities of frozen water in its permanently shadowed crater. That water is a valuable resource for astronauts who’ll visit the Moon in the future and set up bases. It’s also the first time ISRO successfully landed a rover and lander on the Moon after its predecessor, Chandrayaan-2, crashed into the surface.

But it’s encouraging that Vikram and Pragyaan are still intact. ISRO hoped that the Sun would bring both back to life after the agency put them into sleep mode as night fell. There’s a chance that the sunlight would recharge the batteries.

“Once there is sufficient solar generation, they are expected to come back to life provided that they have survived the night.”

M Srikanth, Chandrayaan-3 Mission Operations Director.

ISRO released an update on Friday, the beginning of the new lunar day. Unfortunately, there was no response from either the lander or the rover.

Chandrayaan-3 Mission:
Efforts have been made to establish communication with the Vikram lander and Pragyan rover to ascertain their wake-up condition.

As of now, no signals have been received from them.

Efforts to establish contact will continue.

— ISRO (@isro) September 22, 2023

When night falls on the Moon’s south pole, temperatures plummet as low as -200C to -250C (-328F to -418F.) The lander and rover were never designed to handle these temperatures. The rover has only a small battery—10 amp-hours—that provides the necessary power to deploy its solar array. It was also included to help the rover survive a periodic eclipse. The small battery was fully charged when night came, and the solar panels were positioned to receive incoming starlight when morning came. The Vikram lander was also ready for the morning, and its 62.5 amp hour was fully charged.

Both vehicles are pre-programmed to come back to life as the Sun reappears. “When sunlight comes back, there’s an autonomous logic pre-loaded on both the lander and rover,” said M Srikanth, Chandrayaan-3 Mission Operations Director, in an interview with the Times of India. “Once there is sufficient solar generation, they are expected to come back to life provided that they have survived the night.”

If ISRO's Chandrayaan-3 mission is truly over, it was still a success. It was the first spacecraft to land at the Moon's south pole region. Image Credit: ISRO
If ISRO’s Chandrayaan-3 mission is truly over, it was still a success. It was the first spacecraft to land at the Moon’s south pole region. Image Credit: ISRO

But according to Isro chief AS Kiran Kumar, the “chances of reawakening are dimming with each passing hour.” In an interview with the BBC, Kumar added, “The lander and rover have so many components which may not have survived the frigid temperatures on the Moon.” In fairness, they were never designed to.

It’s all up to the lander’s transmitter now. It’s ISRO’s link with the mission, and if it won’t function, it won’t matter if some of the spacecraft’s other systems are somehow still working. “It has to tell us that it’s alive. Even if all other sub-systems work, we have no way of knowing that,” Kumar added.

Some of ISRO’s hopefulness is based on China’s successful Chang’e 4 mission. It landed on the lunar far side and was plunged into darkness and freezing temperatures, too. It woke up with the sunrise more than once.
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Review: Patagonia R1 Air Full-Zip Hoody

Published

17 hours ago

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September 27, 2023

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Tet19 047 Me on Teton Crest Trail copy cropped 8

Hooded Fleece Jacket
Patagonia R1 Air Full-Zip Hoody
$179, 12.5 oz./354g (men’s medium)
Sizes: men’s XS-XXL, women’s XXS-XL, kids XS-XXL
backcountry.com

As I’ve repeatedly written at this blog, virtually no piece of outdoor apparel offers more versatility than a highly breathable, midweight insulation layer; arguably, the only “layer” you will wear more is your skin. Find a highly breathable midweight jacket that’s soft and fits like it was custom made for your torso and you have a winner. Patagonia’s R1 Air Full-Zip Hoody could play that role for almost any outdoor user, from hard-core backpackers, climbers, and backcountry skiers to the average dayhiker and fitness walker, as I found wearing it on backpacking trips in Glacier National Park and the Canadian Rockies, not to mention countless days around town and at home.

At 12.5 ounces/354 grams (men’s medium), this midweight fleece is designed for wearing as an outer or middle layer in a huge range of cool to cold temperatures, including activities and seasons as diverse as hiking or climbing in virtually any mountains in any month of the year, southern climes from fall through spring, or for any winter activity—skiing, hiking, running, walking, you pick.

Tet19 047 Me on Teton Crest Trail copy cropped 9
Hi, I’m Michael Lanza, creator of The Big Outside. Click here to sign up for my FREE email newsletter. Join The Big Outside to get full access to all of my blog’s stories. Click here for my e-guides to classic backpacking trips. Click here to learn how I can help you plan your next trip.

The Patagonia R1 Air Full-Zip Hoody.
” data-image-caption=”The Patagonia R1 Air Full-Zip Hoody.
” data-medium-file=”https://i0.wp.com/thebigoutside.com/wp-content/uploads/2023/09/Patagonia-R1-Air-Full-Zip-Hoody.jpg?fit=300%2C200&ssl=1″ data-large-file=”https://i0.wp.com/thebigoutside.com/wp-content/uploads/2023/09/Patagonia-R1-Air-Full-Zip-Hoody.jpg?fit=900%2C600&ssl=1″ src=”https://i0.wp.com/thebigoutside.com/wp-content/uploads/2023/09/Patagonia-R1-Air-Full-Zip-Hoody.jpg?resize=900%2C600&ssl=1″ alt=”The Patagonia R1 Air Full-Zip Hoody.” class=”wp-image-60252″ srcset=”https://i0.wp.com/thebigoutside.com/wp-content/uploads/2023/09/Patagonia-R1-Air-Full-Zip-Hoody.jpg?resize=1024%2C683&ssl=1 1024w, https://i0.wp.com/thebigoutside.com/wp-content/uploads/2023/09/Patagonia-R1-Air-Full-Zip-Hoody.jpg?resize=300%2C200&ssl=1 300w, https://i0.wp.com/thebigoutside.com/wp-content/uploads/2023/09/Patagonia-R1-Air-Full-Zip-Hoody.jpg?resize=768%2C512&ssl=1 768w, https://i0.wp.com/thebigoutside.com/wp-content/uploads/2023/09/Patagonia-R1-Air-Full-Zip-Hoody.jpg?resize=150%2C100&ssl=1 150w, https://i0.wp.com/thebigoutside.com/wp-content/uploads/2023/09/Patagonia-R1-Air-Full-Zip-Hoody.jpg?w=1200&ssl=1 1200w” sizes=”(max-width: 900px) 100vw, 900px” data-recalc-dims=”1″ />The Patagonia R1 Air Full-Zip Hoody.

It kept me warm without overheating—rarely even breaking a sweat—wearing it over one base layer while hiking with a full pack, uphill and downhill, on cool, generally calm mornings and some windy afternoons during a weeklong, nearly 70-mile September backpacking trip in Glacier National Park, and hiking in chilly, very strong wind on three-day hikes on both the Skyline Trail in Jasper National Park and the Nigel, Cataract, and Cline Passes Route in the White Goat Wilderness of the Canadian Rockies in the first week of August.

On those backpacking trips, I also wore it in camp both as an outer layer and, when temps dropped, under a down jacket—meaning the R1 Air Hoody doubled as an on-trail layer and a camp layer that allowed me to bring a lighter puffy and forego a midweight, long-sleeve shirt. To frame it another way: The R1 Air Hoody cut my layering system weight by replacing or reducing two other layers. Few pieces of apparel offer more versatility while reducing your pack weight.

I also wore it on breezy, cool evenings in the 50s between waves of thunderstorms
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Gaia is Now Finding Planets. Could it Find Another Earth?

Published

2 days ago

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September 26, 2023

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Giant Planet Detection

The ESA launched Gaia in 2013 with one overarching goal: to map more than one billion stars in the Milky Way. Its vast collection of data is frequently used in published research. Gaia is an ambitious mission, though it seldom makes headlines on its own.

But that could change.

Gaia relies on astrometry for much of its work, and astrometry is the measurement of the position, distance, and motions of stars. It’s so sensitive that it can sometimes detect the slight wobble a planet imparts to its much more massive star. Gaia detected its first two transiting exoplanets in 2021, and it’s expected to find thousands of Jupiter-size exoplanets beyond our Solar System.

But new research takes it even further. It shows that Gaia should be able to detect Earth-like planets up to 30 light-years away.

The new paper is “The Possibility of Detecting our Solar System Through Astrometry,” and is available on the pre-press site arxiv.org. It has a single author: Dong-Hong Wu from the Department of Physics, Anhui Normal University, Wuhu, Anhui, China.

Astronomers find most exoplanets with the transit method. A spacecraft like TESS monitors a section of the sky and looks at many stars at once. When a planet passes between us and one of the stars, it’s called a transit. It creates a dip in starlight that TESS’s sensitive instruments can detect. When TESS detects multiple, predictable dips, it signifies a planet.

But that’s not the only way to detect them. Astrometry can do it too, and that’s Gaia’s way.

Astrometry has an advantage over other methods. Gaia can more accurately determine an exoplanet’s orbital parameters. This doesn’t mean the other methods aren’t valuable. They obviously are. But as the paper’s author explains, “Neither the transit nor radial velocity method provides complete physical parameters of one planet, and both methods prefer to detect planets close to the central star. On the contrary, the astrometry method can provide a three-dimensional characterization of the orbit of one planet and has the advantage of detecting planets far away from the host star.” Astrometry’s advantages are clear.

If other technological planetary civs exist—and that’s a big if—then it’s not outrageous to think they have technology similar to Gaia’s. While Gaia is impressive, there are improvements on the horizon that will make astrometry even more precise. The author asks a question in his paper: If ETIs (ExtraTerrestrial Intelligences) are using advanced astrometry equal to or even surpassing Gaia’s, “…which of them could discover the planets in the solar system, even the Earth?”

Astrometrical precision is calculated in microarcseconds, and precision decreases with distance. The ESA says that Gaia can measure a star’s position within 24 microarcseconds for objects 4000 times fainter than the naked eye. That’s like measuring the thickness of a human hair from 1000 km away. But that’s not precise enough for Wu’s scenario. His work is based on even more advanced astrometry, the type we’ll likely have in the near future. “If the astrometry precision is equal to or better than ten microarcseconds, all 8,707 stars located within 30 pcs of our solar system possess the potential to detect the four giant planets within 100 years.”

This is the heart of Wu’s paper. The 30-parsec (approx. 100 light-years) region contains almost 9,000 stars, and if an ETI from one of those stars has powerful enough astrometry, then it could detect Jupiter, Saturn, Uranus, and Neptune. The only drawback is they’d have to observe our Solar System for nearly a century to make sure the signal was clear.

This figure from the research shows how long it would take for an ETI with advanced astrometry to detect our Solar System's four giant planets. 1,” the author writes. Image Credit: Wu 2023.” class=”wp-image-163369″ srcset=”https://www.universetoday.com/wp-content/uploads/2023/09/Giant-Planet-Detection.png 492w, https://www.universetoday.com/wp-content/uploads/2023/09/Giant-Planet-Detection-374×580.png 374w, https://www.universetoday.com/wp-content/uploads/2023/09/Giant-Planet-Detection-161×250.png 161w” sizes=”(max-width: 492px) 100vw, 492px” />
This figure from the research shows how long it would take for an ETI with advanced astrometry to detect our Solar System’s four giant planets. “We find that all the four giants in our solar system could be detected and well-characterized as long as they are observed for at least 90 years with SNR > 1,” the author writes. Image Credit: Wu 2023.

There are 8707 stars within 100

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