Repost-Well, Maybe Attempt Some Kind Of Landing There-Some Europa Links

If you’d like a breakdown of the relative sizes of our planet, our moon and all these other moons, click through for a helpful visual.

Also, there’s a lot of space out there:

You’ll likely need an energy source (not necessarily our star, the warping effects of other massive bodies will do) and tens, if not hundreds, of millions of years to sustain an environment conducive to life.  You’ll likely need lots of protection from cosmic rays and short-wave radiation as some kind of shield.  If your planet, moon and/or body doesn’t possess an atmosphere, and is too small to maintain an electro-magnetic dynamo like Earth, then sub-surface water under a protective shell might be enough.

On the recent findings of at least 1/17 observational days of water plumes near the surface of the Jovian moon, Europa:

More here:

They used a spectrograph at the Keck Observatory that measures the chemical composition of planetary atmospheres through the infrared light they emit or absorb. Molecules such as water emit specific frequencies of infrared light as they interact with solar radiation.’

and:

‘Paganini and his team reported in the journal Nature Astronomy on November 18 that they detected enough water releasing from Europa (5,202 pounds, or 2,360 kilograms, per second) to fill an Olympic-size swimming pool within minutes. Yet, the scientists also found that the water appears infrequently, at least in amounts large enough to detect from Earth, said Paganini: “For me, the interesting thing about this work is not only the first direct detection of water above Europa, but also the lack thereof within the limits of our detection method.’

This is potentially good news for the upcoming Europa clipper mission.  Otherwise, how are you going to get at all that water beneath an icy shell at least 10-15 miles thick?

‘From its orbit of Jupiter, Europa Clipper will sail close by the moon in rapid, low-altitude flybys. If plumes are indeed spewing vapor from Europa’s ocean or subsurface lakes, Europa Clipper could sample the frozen liquid and dust particles. The mission team is gearing up now to look at potential orbital paths, and the new research will play into those discussions.

“If plumes exist, and we can directly sample what’s coming from the interior of Europa, then we can more easily get at whether Europa has the ingredients for life,” Pappalardo said. “That’s what the mission is after. That’s the big picture.”

Aren’t you getting a little excited at the prospect?:

Via Another Reader Via Youtube-BBC Interview With Various Cassini Mission Scientists

~25 minutes.  Well-edited.  Informative.

Both moons Enceladus (Saturn) and Europa (Jupiter) demonstrate evidence of huge oceans of liquid water protected by thick, icy crusts.  The Cassini probe passed through water plumes emanating high above Enceladus’ icy crust.  This water has been forced out of four long, deep cracks in the surface.

After analysis, the folks in the video above have discovered many chemicals within these Enceladus geysers (ammonia, carbon dioxide) but most importantly:  Possibly hydrogen they think might be coming from hydro-thermal vents on the rocky, ocean floor of Enceladus.

Well, Maybe Attempt Some Kind Of Landing There-Some Europa Links

If you’d like a breakdown of the relative sizes of our planet, our moon and all these other moons, click through for a helpful visual.

Also, there’s a lot of space out there:

You’ll likely need an energy source (not necessarily our star, the warping effects of other massive bodies will do) and tens, if not hundreds, of millions of years to sustain an environment conducive to life.  You’ll likely need lots of protection from cosmic rays and short-wave radiation as some kind of shield.  If your planet, moon and/or body doesn’t possess an atmosphere, and is too small to maintain an electro-magnetic dynamo like Earth, then sub-surface water under a protective shell might be enough.

On the recent findings of at least 1/17 observational days of water plumes near the surface of the Jovian moon, Europa:

More here:

‘They used a spectrograph at the Keck Observatory that measures the chemical composition of planetary atmospheres through the infrared light they emit or absorb. Molecules such as water emit specific frequencies of infrared light as they interact with solar radiation.’

and:

Paganini and his team reported in the journal Nature Astronomy on November 18 that they detected enough water releasing from Europa (5,202 pounds, or 2,360 kilograms, per second) to fill an Olympic-size swimming pool within minutes. Yet, the scientists also found that the water appears infrequently, at least in amounts large enough to detect from Earth, said Paganini: “For me, the interesting thing about this work is not only the first direct detection of water above Europa, but also the lack thereof within the limits of our detection method.’

This is potentially good news for the upcoming Europa clipper mission.  Otherwise, how are you going to get at all that water beneath an icy shell at least 10-15 miles thick?

From its orbit of Jupiter, Europa Clipper will sail close by the moon in rapid, low-altitude flybys. If plumes are indeed spewing vapor from Europa’s ocean or subsurface lakes, Europa Clipper could sample the frozen liquid and dust particles. The mission team is gearing up now to look at potential orbital paths, and the new research will play into those discussions.

“If plumes exist, and we can directly sample what’s coming from the interior of Europa, then we can more easily get at whether Europa has the ingredients for life,” Pappalardo said. “That’s what the mission is after. That’s the big picture.”

Aren’t you getting a little excited at the prospect?:

Venus & Enceladus-A Few Humble Links

Phosphine gas could still be produced by some yet unknown non-living process, but it’s an interesting, and potentially important, find.

From Nature:

Measurements of trace gases in planetary atmospheres help us explore chemical conditions different to those on Earth. Our nearest neighbour, Venus, has cloud decks that are temperate but hyperacidic. Here we report the apparent presence of phosphine (PH3) gas in Venus’s atmosphere, where any phosphorus should be in oxidized forms.

Despite being a near twin in size to Earth-mass and gravity, Venus spins too slowly for an electro-magnetic dynamo to create a EM field, enveloping and protecting the planet. With ninety times the surface pressure of Earth, and temperatures up to nine-hundred degrees Farenheit, to say it would be hellish would be an understatement.

Yet, it once harbored liquid water oceans, and maybe, just maybe, some kind of microbial life has migrated up into the fast-moving clouds. Click through for a visual.

Or listen to a podcast while you work, walk, or clean:

Addition: Anton Petrov sheds some light:

Next to Enceledaus, a tiny moon being warped by Saturn, this is probably the most important indicator of extra-terrestial life going right now:

Step By Step-Some Humble Space Links

Frank Drake brings some realism to the S.E.T.I. debate.  The space-time distances are a huge hurdle, and the challenges of becoming a spacefaring civilization make the journey to nearby star systems fairly impractical at the moment.

The less evidence and fewer data points there are, the more rampant the speculation, inventive the Sci-Fi imaginings, and important the foundation to create such new fields of knowledge.

There’s been an explosion of private entrepreneurship and NASA partnership lately (loosened regulations and better incentives) to help get cargo (things and people) into space much more cheaply than before.

What’s it like to be on a spacewalk?  In some ways, pretty normal and pretty not normal, apparently: Just pace yourself, focus, and get the job done in an unwieldy suit while you hover between everything you’ve ever known and an incomprensible abyss.

In addition to recent rapid advances in ‘seeing’ with radio waves, gravity waves and light, and we’ve got better tools to get a little further out into our own neighborhood.

This means we could find out if we can find some life on Mars (methane spikes), Jupiter’s icy moon Europa and Saturn’s icy moon Enceladus:

and:

and: