Quick Update: On the evening of April 25, The Moon and Saturn had a close encounter. Sometimes called a “romancing affair.” They were about 5 degrees away from each other when I saw them from here in the desert at about 8 pm California time. By 4:20 am the next morning they were even closer but unfortunately both the Moon and Saturn had already set in the West. At 6:30 am (13:30 UT) that morning Saturn passed behind the Moon. It pulled away from the Moon leaving the Moon to the East. I guess the show is over but it was sort of fun to watch. Now on to Saturn and Jupiter…
Recently, when the weather was calmer here ( not so much high wind) I got a chance to look at two of my favorite planets, Jupiter and Saturn. While Jupiter is my all-time favorite, I marvel at Saturn and its so perfect form and symmetry.
For my last viewing of Jupiter I had to get up before dawn. And it was not warm outside. But as for Saturn I had only to be outside a hour or so after night fall. With my spotting scope on low power I centered-in on this beautiful astronomical sight. Then I moved up to the scope’s highest power, 60x. The ringed planet at that time was nicely lit by the Sun and showed that familiar Saturn- look we see in photos and depictions of the planet. (See my quick sketches in the Astronomy Album.) To the right of Saturn was the tiny little dot off from the rings. That’s Titan, Saturn’s largest moon. I’ve seen Titan many times before while viewing Saturn.
I remember the first time I saw Saturn through a telescope. I was about 16 years-old and living at home. Somehow I had heard that to see Saturn you had to get up at about 2:30 in the morning. So one early morning I took a small refractor telescope on loan from a friend at school and went out in to our backyard to look for Saturn. My father, a light sleeper, heard the noises and looked out to see what was going on. He was satisified to see it was his son with a telescope out in the backyard and he went back to bed.
I aimed the telescope at a yellowish-white object in the south eastern sky. I was shocked to find that with this small telescope I was actually seeing Saturn! There it was. It was real…and with rings, too! I remember I was shaking with excitement. That was my first viewing of Saturn and there would be many more.
Saturn has many moons, as many a hundred have been found. And the numbers seem to just keep growing as new “moons” are discovered. These outer moons are probably captured “moons”, not those which formed along with Saturn some four and half billion years ago. These satellites are most likely asteroids or other small rock-like bodies that wondered by Saturn and got caught in its massive gravitational pull.
Saturn is fairly close now, about 837 million miles (1.347 billion km) from the Earth. It is closer to us than it is to the Sun, 855.6 million miles (1.377 billion km). The orbits of Saturn and the Earth allow for this proximity in their ever changing relationship between each other.
Saturn’s rings were first sighted back in 1610 by Italian astronomer Galileo Galilei through what would now be seen as just a simple telescope. At that time he didn’t know what to think of them. He thought they were arms or handles connected to the planet. It wasn’t until 1659 that Christian Huygens, looking through a better telescope, determined that they were rings.
The rings of Saturn are 175,000 miles (282,00o km) across. But what is amazing they are only 3200 feet (1 km) in thickness. That’s hardly more than the length of eight football fields put together! Yet these rings can be easily seen from a more than billion miles (1.6 billion+ km) away. Some of the pieces of the rings are only the size of sugar grains, while others are as a big as a house.
There is a division in rings of Saturn that was found in 1675 by astronomer Jean-Dominique Cassini. He saw a break in the rings about 3000 miles (4800 km) wide. Recently this division has been determined to be caused by the gravitational pull of Saturn’s moon, Mimas. So to honor this division in the rings which Cassini found, the ring is named Cassini’s Division or simply, Cassini’s Ring.
The moon Mimas has an effect on the debris in the rings of Saturn like our moon has a pull on the oceans here on Earth, creating tides. But what if Mimas wasn’t there? It never existed. Then Cassini’s ring might not be there either. And further, suppose Mimas just decided to take off and leave Saturn, heading off into space ((highly unlikely due to Saturn’s colossal gravity)… or maybe Mimas became perturbed and fell out of its orbit and plunged into Saturn. Would the rings close back up as if they had never been separated at all? Or perhaps they would seal up again but after some long epoch of time? In any case, it might well be said: Mimas here, Cassini famous. Mimas not here, Cassini not famous.
But what dismays and disappoints me is that with a much more advanced telescope than Cassini ever had I can’t find that division! In fact, some local astronomers who have huge backyard telescopes and seem to be able to find anything in the Universe- well, they too can’t show me that division in Saturn’s rings. So how could Cassini, more than 330 years ago, find that division using an optical devise hardly better than a toy store telescope? The best that I can think of, and I hope to test this soon, is that maybe Cassini’s telescope let through a lot less light and so the brightness of Saturn was much dimmer. I may try using a darkening filter to significantly reduce the brightness of the rings thereby stopping excessive light from smearing the image over Cassini’s division.
And now Jupiter… the gigantic planet, also called the jovial planet- “jovial” well, because sometimes it does look happy and even clumsy. The expression jovial is a derivative of Jupiter. Jupiter is the largest and plainly most prominent planet in our solar system. It would take eleven of our Earths, wedged together to span the distance of Jupiter’s equator. And to fill Jupiter up inside with planet Earth’s? A thousands of those.
Jupiter sits only part way from our Sun in the solar system. It is currently 418 million miles (674 million kilometers) from Earth. And like Saturn, it is presently further from the Sun than from us at 495 million miles (797 million kilometers) .
Jupiter is one of the four gas giants circling our Sun. The others are Saturn, Uranus and Neptune. They are essentially globes of very cold gasses under tremendous pressures unknown here on earth. Their cores are liquid metals, mostly hydrogen. It is believed that there is liquid metallic hydrogen down at Jupiter’s center. Is is thought too that because of colder temeperatures on the more distant gas giants the hydrogen at their cores is solid metal.
Some astronomers call Jupiter a brown-star, a planet almost big enough to burst into a star. But there is just not enough matter and substance in Jupiter to fuel a nuclear fussion reaction for Jupiter to become a star.
Jupiter has nearly sixty moons which have been discovered so far. And like Saturn, probably some of those moons are captured moons. The four most prominent moons closest to the planet are Io, Europa, Ganymede and Calisto. These are the Galilean moons because they were first discovered by astronomer Galileo Galilei in 1610 along with the planet Saturn as mentioned above. They most probably formed along with Jupiter as it coalesced more than four billion years ago. These are the moons I see every time I look at Jupiter. Sometimes there are just two or three of these moons visible. But that is because one or more of these notable moons are either in front of the planet or behind it at the time. Often though I have seen all four moons neatly spread out on either sides of Jupiter. Yet I have never seen just one of those moons by itself. But that would the situation if three of the Galilean moons were in front or behind the planet.
One of the largest and the inner most Galilean moons is Io. This moon is actually volcanically active and spews out molten sulfur which colorfully paints that moon. These volcanoes on Io are of special interest to me. They are sending out molten sulfur at temperatures at least at the melting point of the sulfur, 275°F (135°C). But I would guess that the sulfur disgorging out of Io is hotter than that.
Obviously the Sun is not heating up Io because it just too far away. These energies in this Jovian moon are probably result of the rotational friction of Io and the gravitational interplay Io has with Jupiter. It is the closet large moon to Jupiter and is therefore subject to Jupiter’s tremendous gravity. The hot magma, sulfur in this case, probably has existed since the formation of our solar system and it is still there- but by now Io’s insides have undoubtedly cooled down considerably. But heat is still there, enough to fuel numerous volcanoes.
Because I do not know of any other moon of Jupiter where we see volcanoes it would not be known if there is any heat or magna in any of the other moons. Maybe they have solidified many ions ago and are their innards are cold and still. But once again, because of Io’s closeness to the massive gravitational forces of Jupiter it has life inside because those forces cause disruption and motion within the moon.
Further, the great pull of Jupiter may be triggering those volcanoes. Jupiter’s massive gravity may be literally pulling the molten sulfur out of Io and setting off volcanoes at every weak point on the moon’s surface. And because Io makes one full rotation in less than every two days (43 hours), all sides of the moon face Jupiter consistently causing volcanoes to burst out evenly on Io- much like a chicken on a rotisserie barbecues uniformly on all sides.
So in closing, Saturn and upiter are two wonderful astronomical sights, are free for all to see. You too can view them with just a simple telescope- and by using a power not much more than 40x. I do recommend a stronger power. Galileo saw them with a 20 power scope. Their planetary positions in the sky are usually published in newspapers, astronomy magazines and through the help of your local astronomy club.
All of the images in the Astronomy Album, with the exception of my two sketches, are courtesy of NASA. The photo taken close to Saturn’s rings shows two moons, Telhyse and Dione, just to the left of the planet. The shadow of Telhyse can be seen on the lower right of Saturn’s immense surface. There is also a shot of the orange-tinted moon Titan and Jupiter’s sulfur covered moon, Io. To see the best picture results it is necessary to click on a photo and after it loads click again for the best display.