Tag Archives: Titan

NASA Space Place – Cassini Says Goodbye

Poster’s Note: One of the many under-appreciated aspects of NASA is the extent to which it publishes quality science content for children and Ph.D.’s alike. NASA Space Place has been providing general audience articles for quite some time that are freely available for download and republishing. Your tax dollars help promote science! The following article was provided for reprinting in September, 2017.

By Teagan Wall

2013february2_spaceplaceOn September 15th, the Cassini spacecraft will have its final mission. It will dive into the planet Saturn, gathering information and sending it back to Earth for as long as possible. As it dives, it will burn up in the atmosphere, much like a meteor. Cassini’s original mission was supposed to last four years, but it has now been orbiting Saturn for more than 13 years!

The spacecraft has seen and discovered so many things in that time. In 2010, Cassini saw a massive storm in Saturn’s northern hemisphere. During this storm, scientists learned that Saturn’s atmosphere has water vapor, which rose to the surface. Cassini also looked at the giant storm at Saturn’s north pole. This storm is shaped like a hexagon. NASA used pictures and other data from Cassini to learn how the storm got its six-sided shape.

Cassini also looked at some of Saturn’s moons, such as Titan and Enceladus. Titan is Saturn’s largest moon. Cassini carried a lander to Titan. The lander, called Huygens, parachuted from Cassini down to the surface of the moon. It turns out, Titan is quite an exciting place! It has seas, rivers, lakes and rain. This means that in some ways, Titan’s landscape looks a bit like Earth. However, its seas and rivers aren’t made of water—they’re made of a chemical called methane.

Cassini also helped us learn that Saturn’s moon Enceladus is covered in ice. Underneath the ice is a giant liquid ocean that covers the whole moon. Tall geysers from this ocean spray out of cracks in the ice and into space, like a giant sneeze. Cassini flew through one of these geysers. We learned that the ocean is made of very salty water, along with some of the chemicals that living things need.

If there is life on Enceladus, NASA scientists don’t want life from Earth getting mixed in. Tiny living things may have hitched a ride on Cassini when it left Earth. If these germs are still alive, and they land on Enceladus, they could grow and spread. We want to protect Enceladus, so that if we find life, we can be sure it didn’t come from Earth. This idea is called planetary protection.

Scientists worry that when Cassini runs out of fuel, it could crash into Titan or Enceladus. So years ago, they came up with a plan to prevent that from happening. Cassini will complete its exploration by diving into Saturn—on purpose. The spacecraft will burn up and become part of the planet it explored. During its final plunge, Cassini will tell us more about Saturn’s atmosphere, and protect the moons at the same time. What an exciting way to say goodbye!

To learn more about Saturn, check out NASA Space Place: https://spaceplace.nasa.gov/all-about-saturn

This article was provided by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.

Caption: This image of the hexagonal storm on Saturn’s north pole was taken by Cassini in 2013. Image credit: NASA/JPL-Caltech/Space Science Institute

About NASA Space Place

With articles, activities, crafts, games, and lesson plans, NASA Space Place encourages everyone to get excited about science and technology. Visit spaceplace.nasa.gov (facebook|twitter) to explore space and Earth science!

Free Astronomy Magazine – September-October 2017 Issue Available For Reading And Download

Greetings, fellow astrophiles!

The most recent issue of Free Astronomy Magazine (September-October, 2017) is available for your reading and downloading pleasure at www.astropublishing.com (click the link to go directly to the issue).

Free Astronomy Magazine was featured as the first of a series of articles on great free online content for amateur astronomers (see A Universe Of Free Resources Part 1) and we’ll be keeping track of future publications under the Online Resources category on the CNYO website.

You can find previous Free Astronomy Magazine issues by checking out our Free Astronomy Magazine Category (or look under the Education link in our menu).

For those wanting a quick look at what the issue has to offer, the Table of Contents is reproduced below.

September-October 2017

The web browser-readable version of the issue can be found here:

September-October 2017 – www.astropublishing.com/5FAM2017/

For those who want to jump right to the PDF download (27 MB), Click here: September-October 2017

NASA Space Place – The Fizzy Seas of Titan

Poster’s Note: One of the many under-appreciated aspects of NASA is the extent to which it publishes quality science content for children and Ph.D.’s alike. NASA Space Place has been providing general audience articles for quite some time that are freely available for download and republishing. Your tax dollars help promote science! The following article was provided for reprinting in May, 2017.

By Marcus Woo

2013february2_spaceplaceWith clouds, rain, seas, lakes and a nitrogen-filled atmosphere, Saturn’s moon Titan appears to be one of the worlds most similar to Earth in the solar system. But it’s still alien; its seas and lakes are full not of water but liquid methane and ethane.

At the temperatures and pressures found on Titan’s surface, methane can evaporate and fall back down as rain, just like water on Earth. The methane rain flows into rivers and channels, filling lakes and seas.

Nitrogen makes up a larger portion of the atmosphere on Titan than on Earth. The gas also dissolves in methane, just like carbon dioxide in soda. And similar to when you shake an open soda bottle, disturbing a Titan lake can make the nitrogen bubble out.

But now it turns out the seas and lakes might be fizzier than previously thought. Researchers at NASA’s Jet Propulsion Laboratory recently experimented with dissolved nitrogen in mixtures of liquid methane and ethane under a variety of temperatures and pressures that would exist on Titan. They measured how different conditions would trigger nitrogen bubbles. A fizzy lake, they found, would be a common sight.

On Titan, the liquid methane always contains dissolved nitrogen. So when it rains, a methane-nitrogen solution pours into the seas and lakes, either directly from rain or via stream runoff. But if the lake also contains some ethane—which doesn’t dissolve nitrogen as well as methane does—mixing the liquids will force some of the nitrogen out of solution, and the lake will effervesce.

“It will be a big frothy mess,” says Michael Malaska of JPL. “It’s neat because it makes Earth look really boring by comparison.”

Bubbles could also arise from a lake that contains more ethane than methane. The two will normally mix, but a less-dense layer of methane with dissolved nitrogen—from a gentle rain, for example–could settle on top of an ethane layer.

In this case, any disturbance—even a breeze—could mix the methane with dissolved nitrogen and the ethane below. The nitrogen would become less soluble and bubbles of gas would fizz out.

Heat, the researchers found, can also cause nitrogen to bubble out of solution while cold will coax more nitrogen to dissolve. As the seasons and climate change on Titan, the seas and lakes will inhale and exhale nitrogen.

But such warmth-induced bubbles could pose a challenge for future sea-faring spacecraft, which will have an energy source, and thus heat. “You may have this spacecraft sitting there, and it’s just going to be fizzing the whole time,” Malaska says. “That may actually be a problem for stability control or sampling.”

Bubbles might also explain the so-called magic islands discovered by NASA’s Cassini spacecraft in the last few years. Radar images revealed island-like features that appear and disappear over time. Scientists still aren’t sure what the islands are, but nitrogen bubbles seem increasingly likely.

To know for sure, though, there will have to be a new mission. Cassini is entering its final phase, having finished its last flyby of Titan on April 21. Scientists are already sketching out potential spacecraft—maybe a buoy or even a submarine—to explore Titan’s seas, bubbles and all.

To teach kids about the extreme conditions on Titan and other planets and moons, visit the NASA Space Place: spaceplace.nasa.gov/planet-weather/

This article was provided by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.

Caption: Radar images from Cassini showed a strange island-like feature in one of Titan’s hydrocarbon seas that appeared to change over time. One possible explanation for this “magic island” is bubbles. Image credits: NASA/JPL-Caltech/ASI/Cornell

About NASA Space Place

With articles, activities, crafts, games, and lesson plans, NASA Space Place encourages everyone to get excited about science and technology. Visit spaceplace.nasa.gov (facebook|twitter) to explore space and Earth science!

CNYO Observing Log: “Stars And S’mores” At Green Lakes State Park, 10 July 2015

Greetings, fellow astrophiles!

I’ve had few chances to provide write-ups of observing sessions in 2015 due to CNY skies not agreeing with we amateur astronomers. Fortunately, Bob Piekiel’s yearly 2015 Green LakesStars and S’mores” Summer Session (on the books for 6 months now) landed on an excellent summer night, providing a large crowd some excellent views of some (sadly, not all) of the Solar System’s best sights.

2015july13_greenlakes

Part of the crowd at Green Lakes. Click for a larger view.

There were roughly 120 people in attendance at the start of the session (by the car/people count of the Green Lakes staff. They estimate 3.5 people per car on average, which sounds like quite a mess in the back seat), making this the largest public CNY session I’ve attended since the Transit of Venus in 2012. To Bob’s SCT and my NMT 12.5” Dob was added guest attendee and the IOTA’s own Ted Blank with his (I’m pretty sure, anyway) Orion 120mm ST Refractor. We had one last work-in-progress scope in attendance with the arrival of fellow CNYO’ers Kirk Frisch (his work-in-progress) and Chris Schuck. As usual, the setup of the scopes cut into our collective s’mores time.

Bob had already aligned his SCT and started close to 8:00 p.m. on the viewing of Venus after a quick welcome and safety lecture. I had someone with great eyesight point out Venus near my scope, after which the line behind my Dob hit +50 people. Sadly, with a +50 person line at each of the scopes and all pointed at Venus to give the attendees that view, you take quite a bit of time to show the planet to everyone (and for the motor-less scopes, additional time re-nudging Venus back into the eyepiece. Stupid Earth rotation…). For us, that meant that Jupiter, the next to appear after sunset, was already obscured in the high tree line to the West of the Green Lakes field. Bob had a short-but-heroic catch between branches, but Ted and I were left to wait for Saturn.

Another search by the same woman at my scope (someone had a big piece of carrot cake earlier, I guess) pointed out Saturn midway above another high tree patch. We all then spent a good 30 minutes on Saturn, comparing views and encouraging people to spend a little time trying to pull additional detail out – namely, Titan and the Cassini Division. Finally well after sunset, the stars began to then appear behind Saturn, so person #40 had a more engaging view than person #1.

Venus and Saturn viewing for the whole group took about an hour, after which the youngest members of the crowd headed home and a few others showed in time for some non-planetary viewing that went until about 11:00 p.m. My observing list for the night (a recurring theme for all of the Summer public viewing sessions) was as follows:

* Saturn and Venus

* Albireo in Cygnus – a Summer favorite to show people that stars are actually quite colored when you find the right ones (and binaries make it all the more interesting)

* Alcor and Mizar in Ursa Major – first as a Naked Eye test for attendees, then on to the discussion of the complexities of a 6-star (!) system

* M57, the Ring Nebula in Lyra – a real standout at near-zenith, as well as a preview of what our own Sun will look like in 5-ish billion years

* Herschel’s Garnet Star in Cepheus – the first of the closers for the evening, showing that some stars are very intensely colored

* Zubeneschamali (?! Let’s go with beta Librae) in Libra – the second of the closers in my scope (at Bob’s request). Some people see this as a faintly green star, which makes it quite noteworthy (Bob and I have decided it’s actually blue-ish instead. According to wikipedia, “There seems to be no generally accepted explanation for why some observers see it as green.” Perhaps someone could do the study to see if these people also see the dress as black and blue).

The Andromeda Galaxy (M31) and M32 – a final view just above the horizon (so all had to stoop low to see into the eyepiece) to take the final 5 attendees outside of the Milky Way. At the risk of starting an argument, I would argue that M31 is best viewed through 25×100 binoculars, giving you the best combination of field of view (this galaxy is six Full Moons across and any significant magnification causes you to miss lots of the trailing starlight around the core) and spiral detail. In fact, M31 is a prime reminder to all that a good pair of binos is a must-have for the dedicated observer.

Those interested in some additional summertime viewing are welcome to join us at Bob Piekiel’s Baltimore Woods session this coming Friday, July 17th (18th as the weather-alternate) and solar session at Clark Reservation on Saturday. Check cnyo.org on Friday afternoon for an official announcement. We hope you can join us!

NASA News Digest: Space Science For 23 June – 10 July 2014

Greetings fellow astrophiles,

The NASA News service provides up-to-date announcements of NASA policy, news events, and space science. A recent selection of space science articles are provided below, including direct links to the full announcements. Those interested in receiving these news announcements directly from NASA can subscribe to their service by sending an email to:

hqnews-request@newsletters.nasa.gov?subject=subscribe

NASA’s Mars Curiosity Rover Marks First Martian Year with Mission Successes

RELEASE 14-177 (Click here for the full article) – 23 June 2014

2014july10_14_177_0_smallNASA’s Mars Curiosity rover will complete a Martian year — 687 Earth days — on June 24, having accomplished the mission’s main goal of determining whether Mars once offered environmental conditions favorable for microbial life.

One of Curiosity’s first major findings after landing on the Red Planet in August 2012 was an ancient riverbed at its landing site. Nearby, at an area known as Yellowknife Bay, the mission met its main goal of determining whether the Martian Gale Crater ever was habitable for simple life forms. The answer, a historic “yes,” came from two mudstone slabs that the rover sampled with its drill. Analysis of these samples revealed the site was once a lakebed with mild water, the essential elemental ingredients for life, and a type of chemical energy source used by some microbes on Earth. If Mars had living organisms, this would have been a good home for them. 

For more information about Curiosity, visit:
www.nasa.gov/msl and mars.jpl.nasa.gov/msl/

You can follow the mission on Facebook at:
www.facebook.com/marscuriosity and on Twitter at: www.twitter.com/marscuriosity.

Ocean on Saturn Moon Could be as Salty as the Dead Sea

RELEASE 14-185 (Click here for the full article) – 2 July 2014

2014july10_dead_sea_titan_oceanandice_main_0_smallScientists analyzing data from NASA’s Cassini mission have firm evidence the ocean inside Saturn’s largest moon, Titan, might be as salty as the Earth’s Dead Sea.

The new results come from a study of gravity and topography data collected during Cassini’s repeated flybys of Titan during the past 10 years. Using the Cassini data, researchers presented a model structure for Titan, resulting in an improved understanding of the structure of the moon’s outer ice shell. The findings are published in this week’s edition of the journal Icarus.

For more information about Cassini, visit www.nasa.gov/cassini and saturn.jpl.nasa.gov.

Testing Completed on NASA’s James Webb Space Telescope Backplane

RELEASE 14-178 (Click here for the full article) – 8 July 2014

2014july10_14_178_smallNASA’s James Webb Space Telescope has reached another development milestone with the completion of static load testing of its primary mirror backplane support structure (PMBSS) moving the telescope one step closer to its 2018 launch.

The PMBSS is the stable platform that holds the telescope’s science instruments and the 18 beryllium mirror-segments that form the 21-foot-diameter primary mirror nearly motionless while the telescope peers into deep space. The primary mirror is the largest mirror in the telescope — the one starlight will hit first.

For more information about NASA’s James Webb Space Telescope, visit: www.nasa.gov/webb

Hubble Spots Spiral Bridge of Young Stars Linking Two Ancient Galaxies

RELEASE 14-188 (Click here for the full article) – 10 July 2014

2014july10_14_188_0_smallNASA’s Hubble Space Telescope has photographed an unusual structure 100,000 light years long, which resembles a corkscrew-shaped string of pearls and winds around the cores of two colliding galaxies.

The unique structure of the star spiral may yield new insights into the formation of stellar superclusters that result from merging galaxies and gas dynamics in this rarely seen process.

“We were surprised to find this stunning morphology. We’ve long known that the ‘beads on a string’ phenomenon is seen in the arms of spiral galaxies and in tidal bridges between interacting galaxies. However, this particular supercluster arrangement has never been seen before in giant merging elliptical galaxies,” said Grant Tremblay of the European Southern Observatory in Garching, Germany.

For images and more information about Hubble, visit: www.nasa.gov/hubble and hubblesite.org/news/2014/26.

To learn more about gravitational lensing, visit: go.nasa.gov/1pUWl6f

NASA Spacecraft Observes Further Evidence of Dry Ice Gullies on Mars

RELEASE 14-191 (Click here for the full article) – 10 July 2014

2014july10_14_191_0_smallRepeated high-resolution observations made by NASA’s Mars Reconnaissance Orbiter (MRO) indicate the gullies on Mars’ surface are primarily formed by the seasonal freezing of carbon dioxide, not liquid water.

The first reports of formative gullies on Mars in 2000 generated excitement and headlines because they suggested the presence of liquid water on the Red Planet, the eroding action of which forms gullies here on Earth. Mars has water vapor and plenty of frozen water, but the presence of liquid water on the neighboring planet, a necessity for all known life, has not been confirmed. This latest report about gullies has been posted online by the journal Icarus.

For more information about HiRISE, visit: hirise.lpl.arizona.edu

Additional information about MRO is online at: www.nasa.gov/mro

For recent findings suggesting the presence of liquid water on Mars, visit: go.nasa.gov/1q1VRLS