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Saturn (The Planet)

Cassini's mission is over
Cassini: Saturn probe dives to destruction
By Jonathan AmosBBC Science Correspondent, Pasadena
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The American-led Cassini space mission to Saturn has just come to a spectacular end.

Controllers had commanded the probe to destroy itself by plunging into the planet's atmosphere.

It survived for about a minute before being broken apart.
http://www.bbc.co.uk/news/science-environment-41207827
 
About Cassini's speed as it entered Saturn's atmosphere - is this the fastest a man made object has ever travelled?
 
Up until the end I was hoping they'd actually slingshot it out of the solar system so it could roam the stars.
 
About Cassini's speed as it entered Saturn's atmosphere - is this the fastest a man made object has ever travelled?

No.

'Speed' is a relative measure, so it needs to be qualified with respect to whatever specific astronomical body (e.g., earth, Saturn, sun) is the reference point.

According to the NASA / JPL 'Quick Facts' on Cassini:

Spacecraft speed at loss of signal (relative to Saturn): 69,368 mph (111,637 kph)

SOURCE: https://saturn.jpl.nasa.gov/mission/grand-finale/cassini-quick-facts/

According to Guinness:

Defined by its heliocentric velocity (i.e., relative to our Sun), the fastest spacecraft in the Solar System was Helios 2, a joint venture between NASA and old West Germany's space agency, DFVLR. Launched into a solar orbit on 15 January 1976, the satellite orbited the Sun for almost four years, sending back valuable data on our nearest star. It was on 16 April 1976, as it passed closest to the Sun, that Helios 2 achieved a maximum velocity of 68.6 km/s (246,960 km/h; 153,453 miles per hour). Helios 2 is likely to hold this record until NASA launches the Solar Probe Plus mission in 2018, when velocities of 200 km/s (447,387 miles per hour) are expected.

SOURCE: http://www.guinnessworldrecords.com/world-records/66135-fastest-spacecraft-speed
 
Absolutely amazing! Thanks for the info.
 
Astronomers are nearing completion of a survey of our solar system's planetary satellites (i.e., moons). It's now been announced that Saturn is confirmed as the planet with the most moons.
Scientists Just Discovered 20 Previously Unknown Moons Orbiting Saturn

Saturn has unseated Jupiter as the Solar System's most moon-bearing planet, the Carnegie Institution for Science announced on Monday.

Scientists discovered 20 previously unknown moons orbiting Saturn, which gives Saturn a grand total of 82 moons, flying past Jupiter's 79. ...

"Using some of the largest telescopes in the world, we are now completing the inventory of small moons around the giant planets," Scott Sheppard, a Carnegie astronomer who led the discovery team, said in a press release. "They play a crucial role in helping us determine how our Solar System's planets formed and evolved."

Each of the newly discovered moons is about 3 miles (5 kilometers) in diameter, and 17 of them orbit in retrograde, or in the opposite direction of Saturn's rotation. One of them is now the farthest known moon from Saturn.

The discoveries join three groups of Saturn's outer moons, clustered by the angles at which they orbit the planet. The retrograde moons join the Norse group (all named after Norse mythology), while two others join the Inuit group (named for Inuit mythology), and the final moon goes with the Gallic group (again, mythology).

Scientists think each of those groups may have come from a larger moon that broke apart into smaller bodies. ...
FULL STORY: https://www.sciencealert.com/twenty-new-discoveries-brings-saturn-s-moon-total-to-a-whopping-82
 
New computer modeling research is providing an updated explanation for Saturn's mysterious polar hexagon feature.
We May Finally Understand How Saturn's Giant Hexagonal Storm Came to Be

A turbulent hexagon-shaped storm has been raging near Saturn's north pole for at least four decades - we first discovered it in 1981 during the Voyager mission. Even with a front-row view from the Cassini probe however, details on Saturn's hexagon have been scant.

A new atmospheric model, tested in the lab, now suggests the storm goes very deep, potentially thousands of kilometres. This finding could help to explain why the storm has remained a relatively stable feature since we first caught sight of it. ...

In the past, direct observations and lab experiments have produced two leading hypotheses as to why Saturn's hexagonal storm exists.

On the one hand, it might have formed from shallow, alternating jets in the gas giant's atmosphere, hundreds of kilometres deep where pressure sits at about 10 bars or so, and where gas is more turbulent.

On the other hand, it might be more deeply rooted, coming from deep zonal jets extending thousands of kilometres down, where pressure is tens of thousands of times greater and where the planet's rotation and topography might be whipping up a frenzy. ...

In fact, just before Cassini took its final plunge into retirement, we discovered Saturn's zonal jets retain their strength down to altitudes where the pressure is an astonishing 100,000 bars or more. To put that in perspective, sunlight penetrates not much deeper than a single bar on Saturn; these vortices are deeper and more stable than they appear at first.

Simulating what happens to deep turbulent convections in a rotating spherical shell, researchers at Harvard University now think they have a plausible explanation for why Saturn's hexagon exists.

Their 3D model shows that deep thermal convection in the outer layers of gas giants can spontaneously give rise to giant polar cyclones, fierce alternating zonal flows, and a high-latitude eastward jet pattern.

What's more, these zonal jets are both qualitatively and quantitatively similar to what has been observed on Saturn.

"The analysis of the simulation suggests that self-organised turbulence in the form of giant vortices pinches the eastward jet, forming polygonal shapes," the authors explain.

"We argue that a similar mechanism is responsible for exciting Saturn's hexagonal flow pattern." ...

FULL STORY: https://www.sciencealert.com/astron...urn-s-giant-hexagonal-storm-could-have-formed
 
Newly reported research indicates Saturn's internal structure is quite different from what was long presumed. The planet's core is diffuse rather than a concentrated ball of rock and ice, and it spans most of Saturn's diameter. This research indicates or suggests other revisions in our understanding of how Saturn formed and why it radiates more energy than it is believed to absorb.

The full research report is accessible at the second link below.
Saturn has a fuzzy core, spread over more than half the planet’s diameter

One of Saturn’s rings has revealed properties of its core, hidden deep beneath the planet’s golden atmosphere.

That core isn’t the lump of rock and ice that many scientists had envisioned, the new study finds. Instead, the core is diffuse, pervaded by huge amounts of hydrogen and helium and so spread out that it spans 70,000 kilometers, or about 60 percent of the planet’s diameter, researchers report April 28 at arXiv.org.

The new intel should help planetary scientists better understand not only how giant planets formed in our solar system but also the nature of such worlds orbiting other stars.

To ascertain the structure of Saturn’s core, astronomer Christopher Mankovich and astrophysicist Jim Fuller, both at Caltech, examined the giant planet’s rings. Just as earthquakes help seismologists probe Earth’s interior, oscillations inside Saturn can reveal its internal composition. ...

By analyzing a wave in that ring, along with data on Saturn’s gravity field from the now-defunct Cassini spacecraft (SN: 9/15/17), Mankovich and Fuller found that the core has about 17 Earth masses of rock and ice. But there’s so much hydrogen and helium mixed in, the core encompasses 55 Earth masses altogether — more than half of Saturn’s total, which is equivalent to the mass of 95 Earths. ...
FULL STORY: https://www.sciencenews.org/article/saturn-planet-core-fuzzy-ring-astronomy-space

PUBLISHED RESEARCH REPORT:
A diffuse core in Saturn revealed by ring seismology
Christopher Mankovich, Jim Fuller
https://arxiv.org/abs/2104.13385
 
Saturn’s rings could be remains of moon that strayed too close, say scientists.

Theory of inner satellite ripped apart by gas giant’s gravity 100-200m years ago also explains rings’ relative youth.

Saturn’s famous rings could be the aftermath of a moon that was ripped apart by the planet’s gravity, according to scientists.

The research, based on data from the final stage of Nasa’s Cassini mission, suggests that Saturn may have been ringless for almost all of its 4.5bn-year existence. But about 160m years ago, an inner moon strayed too close to the gas giant causing it to be pulled apart, painting out its own orbit in a trail of shattered icy fragments.

The hypothetical lost moon has been nicknamed Chrysalis.

“Just like a butterfly’s chrysalis, this satellite was long dormant and suddenly became active, and the rings emerged,” said Jack Wisdom, a professor of planetary science at Massachusetts Institute of Technology and lead author of the study.
(C) The Guardian. '22.
 
https://www.cnn.com/2023/02/13/world/hubble-saturn-rings-spokes-scn/index.html

Hubble captures mysterious ‘spokes’ gliding across Saturn’s rings



By Jackie Wattles, CNN

CNN —

The Hubble Space Telescope captured images of a mysterious show playing out on Saturn’s rings — ghostly, fleeting “spokes” that appear to move along the planet’s rings. And scientists can’t yet explain why the phenomena happen.

The return of the spokes is one of the earliest signs that Saturn is entering a new season as it approaches the autumnal equinox of its northern hemisphere, which is expected to occur on May 6, 2025, for the first time in about 15 years.

Scientists have long known about the perplexing spokes, which look like apparitions skating along Saturn’s rings and can be seen around the planet during equinox time. The first evidence was captured by NASA’s Voyager mission in the 1980s.

Exactly what causes the events still eludes scientists. But this time around, NASA researchers are hoping to finally solve the mystery.

Hubble will continue observing the spokes, which are expected to grow more prominent in the lead-up to the 2025 equinox, providing more data about the intriguing occurrences.

“The suspected culprit for the spokes is the planet’s variable magnetic field,” according to a NASA news release. “Planetary magnetic fields interact with the solar wind, creating an electrically charged environment.

“On Earth, when those charged particles hit the atmosphere this is visible in the northern hemisphere as the aurora borealis, or northern lights.”

Essentially, scientists suspect that tiny particles can become charged by this activity, causing them to briefly rise up higher than surrounding material and creating an apparent bulge.

Scientists hope that forthcoming Hubble data will prove or disprove that theory once and for all, building on observations collected by Voyager and Cassini, the dedicated Saturn probe that observed the spoke phenomena during its last appearance in the late 2000s.

“Despite years of excellent observations by the Cassini mission, the precise beginning and duration of the spoke season is still unpredictable, rather like predicting the first storm during hurricane season,” said Amy Simon, a senior planetary scientist at NASA who heads the Hubble Outer Planet Atmospheres Legacy program, in a statement.


The spokes are only visible around Saturn’s equinox when the planet’s rings are tilted toward the sun, according to NASA. The markings can appear as bright spots of light or as black splotches, depending on the vantage point of the viewing instrument.

It’s possible other planets with rings experience similar events, though they’ve so far only been observed on Saturn’s densely packed and very prominent rings.

“It’s a fascinating magic trick of nature we only see on Saturn — for now at least,” Simon said.

 
Death Star moon may be 'wonky or watery'
By Jonathan Webb, Science reporter, BBC News

The internal structure of one of Saturn's moons is either wonky or awash with water, according to a new study.

Mimas is nicknamed the Death Star because it resembles the infamous Star Wars space station.
It has a tell-tale wobble that is twice as big as expected for a moon with a regular, solid structure.
The researchers offer two explanations: either it has a vast ocean beneath its surface, or a rocky core with a weird shape resembling a rugby ball.

The study appears in Science Magazine.
Its authors are astronomers in the US, France and Belgium, who based their calculations on high-resolution photos of Mimas snapped by the Cassini spacecraft.
Cassini was sent to Saturn in 1997 to explore the planet and its many moons, which so far number 62 (53 with names).

The researchers built a detailed 3D model of Mimas using images taken from various angles, and tracked the movement of hundreds of reference points on its pockmarked surface.
"After carefully examining Mimas, we found it librates - that is, it subtly wobbles - around the moon's polar axis," said lead author Dr Radwan Tajeddine, who works at Cornell University in the US.

Apart from these gentle "librations", Mimas otherwise presents the same face to Saturn throughout its orbit.
Our own moon has a similar motion, with a small wobble that offers us slightly different views of the satellite over time.

But when Dr Tajeddine and his colleagues put all their measurements together, they found that the surface of Mimas swivels back and forth by 6km.
This is quite a wobble for a moon that measures less than 400km across. In fact, it is twice as much movement as expected, based on Mimas's size and its elliptical orbit.
"This is where we started thinking of more exotic interior models," Dr Tajeddine told BBC News.

First, the team tested whether the extra rotation could be explained by a deformity underneath the enormous Herschel Crater, one-third the size of Mimas itself, which gives the moon its signature appearance.
But even a "huge mass anomaly" created by the wallop that left the crater would not deliver the amount of movement that Dr Tajeddine's team had observed.

Instead, they wondered whether Mimas might be far from the simple, uniform sphere of ice and rock that most planetary scientists had previously assumed.
"Nature is essentially allowing us to do the same thing that a child does when she shakes a wrapped gift in hopes of figuring out what's hidden inside," Dr Tajeddine said.

His team settled on two likely plot twists, wrapped beneath Mimas's icy crust.
Firstly, their calculations suggested that the wobbles could arise from a core that was squashed or elongated by 20-60km: a huge, central rugby ball of rock.

Alternatively, the moon could have a normal spherical core and crust, but separated by a "global ocean". That way, Dr Tajeddine explained, "the shell can wobble more easily, because it's not attached to another mass".
Of the two explanations, he favours the subterranean sea.
"When we saw this wobbling, the first thing we thought of was an ocean," Dr Tajeddine said.

Either possibility would make Mimas a much more interesting research subject: "This brings the spotlight back to this moon, which was a little bit ignored."

Prof Chris Lintott, an astrophysicist at the University of Oxford, was surprised to hear of the new results.
"If you'd asked me before now, I would have said that Mimas is a boring, icy moon.

"If the ocean is really there, we're getting to the point where it's just completely standard for icy moons to have substantial bodies of water inside - and that could have interesting implications for how many of these things could support life." 8)

http://www.bbc.co.uk/news/science-environment-29613671

Looks like it's watery.

Hidden beneath the heavily cratered surface of Mimas, one of Saturn's smallest moons lies a secret: a global ocean of liquid water. This astonishing discovery, led by Dr. Valéry Lainey of the Observatoire de Paris-PSL and published in the journal Nature, reveals a "young" ocean formed just 5 to 15 million years ago, making Mimas a prime target for studying the origins of life in our solar system.

"Mimas is a small moon, only about 400 kilometers in diameter, and its heavily cratered surface gave no hint of the hidden ocean beneath," says Dr. Nick Cooper, a co-author of the study and Honorary Research Fellow in the Astronomy Unit of the School of Physical and Chemical Sciences at Queen Mary University of London.

"This discovery adds Mimas to an exclusive club of moons with internal oceans, including Enceladus and Europa, but with a unique difference: its ocean is remarkably young, estimated to be only 5 to 15 million years old."

This young age, determined through detailed analysis of Mimas's tidal interactions with Saturn, suggests the ocean formed recently, based on discovering an unexpected irregularity in its orbit. As a result, Mimas provides a unique window into the early stages of ocean formation and the potential for life to emerge.

"The existence of a recently formed liquid water ocean makes Mimas a prime candidate for study for researchers investigating the origin of life," explains Dr. Cooper. The discovery was made possible by analyzing data from NASA's Cassini spacecraft, which meticulously studied Saturn and its moons for over a decade. By closely examining the subtle changes in Mimas's orbit, the researchers were able to infer the presence of a hidden ocean and estimate its size and depth.

Dr. Cooper continues, "This has been a great team effort, with colleagues from five different institutions and three different countries coming together under the leadership of Dr. Valéry Lainey to unlock another fascinating and unexpected feature of the Saturn system, using data from the Cassini mission." ...

https://phys.org/news/2024-02-mimas-tiny-moon-young-ocean.html
 
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