Water Worlds in the Solar System

There is new evidence for the existence of liquid water in the cold outer regions of our solar system. Astronomers using the Hubble Telescope see plumes of water erupting from the surface of Jupiter’s moon Europa, and measurements of Saturn’s little moon Dione indicate that it must have a substantial layer of liquid water deep underground.

In recent years, more and more evidence has accumulated that liquid water exists among the moons of the giant planets. We have known for a while that there is likely to be an underground ocean of water beneath the icy crust of Jupiter’s moon Europa, and perhaps also under the surface of its moon Ganymede (the largest moon in the solar system.)

Then the Cassini mission found great geysers of salt water emerging from the icy cracks on Saturn’s moon Enceladus, a world much smaller than the Jupiter moons we just discussed. The big deal here is not that there is water, since water ice makes up a large part of many of the solid worlds in the outer solar system. The big discovery is that, even in those icy realms, enough heat can be generated inside these moons to have oceans of liquid water.

The Hubble work is the second report of plumes coming out of cracks in the ice of Europa. Earlier work, also done with the Hubble, also hinted at such plumes, but now astronomers have observed them in ultraviolet light as Europa was crossing the face of Jupiter. Our top image shows you what was observed, with a visible-light picture of Europa photoshopped in to show you what the moon looks like. A short NASA movie explaining the discovery can be seen at:
https://www.youtube.com/watch?v=4QJS9LcB66g

The work on Dione was more indirect. This moon of Saturn’s is about 700 mi across, more than twice as big as Enceladus. The presence of water was suggested by measurement of the gravity of Dione, as the Cassini spacecraft flew by it. The gravity measurements fit with the presence of a water layer deep inside the moon, perhaps 60 mi beneath the surface.

(The bottom image shows a very detailed image of Dione's surface from the Cassini spacecraft.  You see many icy cracks and fractures, whose sides show as white cliffs.)

Something must heat the buried “oceans” in these moons to keep them liquid. In some cases, it is a tug of war between the gravity of the mother planet on one side, and a large moon on the other. Or it may be some kind of rocking back and forth, which scientists call “libration”. Whatever allows liquid water layers to exist out there, the fact that they do makes them an interesting place to look for the beginnings of life.

Water Worlds in the Solar System

There is new evidence for the existence of liquid water in the cold outer regions of our solar system. Astronomers using the Hubble Telescope see a plume of water erupting from the surface of Jupiter’s moon Europa, and measurements of Saturn’s little moon Dione indicate that it must have a substantial layer of liquid water deep underground.

In recent years, more and more evidence has accumulated that liquid water exists among the moons of the giant planets. We have known for a while that there is likely to be an underground ocean of water beneath the icy crust of Jupiter’s moon Europa, and perhaps also under the surface of its moon Ganymede (the largest moon in the solar system.)

Then the Cassini mission found great geysers of salt water emerging from the icy cracks on Saturn’s moon Enceladus, a world much smaller than the Jupiter moons we just discussed. The big deal here is not that there is water, since water ice makes up a large part of many of the solid worlds in the outer solar system. The big discovery is that, even in those icy realms, enough heat can be generated inside these moons to have oceans of liquid water.

The Hubble work is the second report of plumes coming out of cracks in the ice of Europa. Earlier work, also done with the Hubble, also hinted at such plumes, but now astronomers have observed them in ultraviolet light as Europa was crossing the face of Jupiter. Our top image shows you what was observed, with a visible-light picture of Europa photoshopped in to show you what the moon looks like. A short NASA movie explaining the discovery can be seen at:
https://www.youtube.com/watch?v=4QJS9LcB66g

The work on Dione was more indirect. This moon of Saturn’s is about 700 mi across, more than twice as big as Enceladus. The presence of water was suggested by measurement of the gravity of Dione, as the Cassini spacecraft flew by it. The gravity measurements fit with the presence of a water layer deep inside the moon, perhaps 60 mi beneath the surface.

(The bottom image shows a very detailed image of Dione's surface from the Cassini spacecraft.  You see many icy cracks and fractures, whose sides show as white cliffs.)

Something must heat the buried “oceans” in these moons to keep them liquid. In some cases, it is a tug of war between the gravity of the mother planet on one side, and a large moon on the other. Or it may be some kind of rocking back and forth, which scientists call “libration”. Whatever allows liquid water layers to exist out there, the fact that they do makes them an interesting place to look for the beginnings of life.

Ringshine on the Night Side of Saturn

A spectacular new image of the night side of Saturn and its shining rings in sunlight was released recently by the Cassini mission. You can also see the shadow Saturn casts on its rings.

This August 2016 view shows the complex structure of the planet's rings clearly. You can see the two gaps in the rings, one wider and one narrower (in the outer part of the outer ring.) Close-ups have revealed fainter rings and moons in the gaps, so they are not really as empty as they might seem.

The sunlight reflected from the rings keeps the night side of Saturn from being as dark as it could be, much as moonshine keeps the nights on Earth from being completely dark. One scientist calculated that if you could float in the upper cloud layers of Saturn (which has no solid surface), you could read an astronomy book by ringshine.

Look at the complexity of Saturn's rings -- ringlet after ringlet can be seen in each main ring. And each ringlet consists of millions of icy chunks, all orbiting together around the equator of Saturn. The main composition of these icy chunks is water -- making the rings a significant reservoir of water for future explorers. (Although two of Saturn's moons, Enceladus and Dione, are now thought to have liquid oceans of water under their icy crusts. Perhaps we can siphon some of that instead of melting ring chunks.)

The image was taken from a distance of 870,000 miles (which seems far, but Saturn was about 850 million miles from Earth at that time, so Cassini definitely had the better view.)

A Great New Image of Saturn

NASA has recently released a spectacular new image of the planet Saturn, seen when it's summer in the Northern Hemisphere. (A year on Saturn is about 30 Earth years, so each season there lasts about 7.5 of our years! Saying goodbye for summer vacation is a big deal there.)

The rings are seen in fine detail with the shadow of the planet toward the left side. The mysterious hexagon-shaped storm at the north pole is also clearly visible. You are seeing Saturn from a distance of about 1.9 million miles.

The image was taken with the Cassini spacecraft that has orbited Saturn and shown us the planet, its rings, and its fantastic moons since 2004.

Enjoy. (Click on the image to see it bigger.)

Planet Discovered Around the Nearest Star

Astronomers at the European Southern Observatory are announcing today that they have found an Earth-sized planet orbiting the nearest star to the Sun, Proxima Centauri.  The star is only 4.2 light years away (which is roughly 25 thousand billion miles – that’s close for astronomers!)

The newly found planet takes 11 days to orbit its reddish star (compare that to Mercury, the closest planet in OUR solar system, which takes 88 days to go around the Sun.)   You might think that a planet that takes only a week and a half to orbit its star must be outrageously hot, but the difference is that Proxima Centauri is a much fainter and cooler star than the Sun.  So the planet could be in the star's habitable zone (liquid water may possibly exist on its surface.)

We found this planet, as we have many others, not by getting a picture of it, but by measuring the pull of the planet on the star.  As the planet circles the star, from one side of it to the other, the planet’s gravity, small as it is, makes the star wiggle just a little bit.  And it’s this wiggling of the star that we can detect from Earth and use it to estimate the mass (gravity) of the planet.

This method can only tell us the minimum mass that the planet must have, and that turns out to be 1.3 times the mass of the Earth. (The wiggle, by the way, only changes the motion of the star by about 3 miles per hour, toward us and then away from us.  That’s a tiny change, but modern instruments are able to make out changes in speed that small.)

A planet with that low a mass is most likely a solid rocky planet, like ours.  Being so much in the gravity embrace of the star, the planet may have one side permanently pointed toward it, much like our Moon has one side permanently pointed toward the Earth as it goes around us. The Proxima Centauri planet would then also rotate in 11 days, making its day and its year the same length!   That’s weird to think about.

The fastest planetary probe we have built so far would take something like 80,000 years to get to Proxima Centauri.   It’s hard to get graduate students to volunteer for that kind of trip!  But, as you may have heard, Yuri Milner, the Russian-American billionaire physicst, has, earlier this year, pledged a hundred million dollars for a research effort to develop a mini-probe, smaller than the smallest cell phone, yet with working instruments, that could ride powerful laser beams and get to the nearest star system in only 20 to 25 years.

Clearly, Project Breakthrough Starshot, as it’s called, will now focus on Proxima Centauri, the nearest of the three stars in the closest star system.  Bets have been on one of the other two stars (called Alpha Centauri, after the brightest in the pair) to have planets, but the first discovery belongs to Proxima.  What an exciting time to be alive.

Above is an artist's conception of what Proxima would look like from the planet's vantage point, and below is a diagram with key characteristics of the Proxima system compared to our own.

Happy One Year Pre-Anniversary of the All-American Eclipse of the Sun

August 21 is exactly one year before the 2017 eclipse of the Sun which will sweep across one country and one country only -- the US. On a Monday morning (Aug. 21, 2017) this "All-American" eclipse (as it's being called) will begin on a beach in Oregon and cross the country diagonally to end in the afternoon on a beach in South Carolina.  See the map below.

The eclipse will be total (moon covering the Sun completely) only in a path about 60 miles wide and we expect huge crowds and traffic jams in that zone. The rest of North America (500 million people) will see a partial eclipse, with a big bite taken out of the Sun. Special eclipse glasses or ways of projecting an image of the Sun will be needed to see the partial eclipse safely.

The full story,in everyday language, with a map and times for major cities, and safe viewing guidance, can be found in a free 8-page excerpt from a book, called Solar Science, that Dennis Schatz and I wrote for teachers. It is at: http://bit.ly/2bkGSvA

There is a national committee that I serve on trying to arrange a good experience with the eclipse for as many people as possible. Wish us luck! Dennis and i are also working with science teachers, libraries, and science and nature museums to become centers of eclipse information for their communities.

I'll say more about preparations for the eclipse on this page as the year goes on. But for now, you may want to note the date and if you have friends or relatives in the total eclipse zone, be extra nice to them starting now.

And thanks to Prof. Tyler Nordgren of the University of the Redlands for permission to use his cool poster.

Map of the 2017 Total Eclipse Path

For those of you who are teachers, or who know a teacher, we will be doing a webinar on how to prepare yourself and your students for the eclipse.  For more see:

http://bit.ly/2bbAwfo

A Sparkling Cluster of Stars from the Hubble

Here is a beautiful new image from the Hubble Space Telescope, showing a young cluster of stars called Trumpler 14.

Located about 8,000 light years away in the constellation of Carina, this grouping of hot bright stars formed only recently from a great cloud of cosmic raw material, called the Carina Nebula. It is one of the great ideas that we now know about how stars live that the more massive a star, the brighter it shines, and the shorter its life-span will be before it "burns out." Superstars die first, is the general rule.

Because Trumpler 14 formed only about 500,000 years ago (which is a very short time on the cosmic scale), this group still includes a lot of bright superstars, which dominate our image.

Robert Trumpler (1886-1956) was a Berkeley astronomer, who compiled a very useful list of star clusters (places where dozens to thousands of stars are born together.) An annual award at the Astronomical Society of the Pacific, honoring the best PhD thesis in astronomy in North America, is named in his honor.

In our picture, you can see a jewel-like display of bright stars in front of the glowing gas and dust of the nebula. The stars in this cluster are one ten thousandth the age of our Sun. Mere babies, really!

Click on the photo to enlarge it and see it even better.