Cassini’s Grand Finale Begins

I don’t want to sound like one of those crazies standing in the public square holding a sign that says, “The End is Nigh”. However, in the case of the Cassini spacecraft, the end really is near. In fact, it’s five orbits away.

What Cassini mission scientists plan is a grand finale as the spacecraft makes its last orbits and plunges into the planet’s atmosphere.
The last of its trips around Saturn begins on Sunday (August 13), and these orbits will see it dip very close to the planet. Cassini’s final orbit will take it into the planet on September 15, 2017. Just before that, a quick gravity maneuver with Titan will slow the spacecraft down. That prepares it for the final dive into Saturn. On the way in, all its science instruments will be turned on. They’ll transmit data until it breaks up under the dense atmospheric pressure of the lower atmosphere. The idea is to get information about a region of Saturn hitherto unexplored and Cassini will be the first official probe of the planet’s atmosphere.

Leading Up to the Finale

Cassini grand finale
An artist’s concept of the Cassini mission as it begins its final five orbits of Saturn. Courtesy Cassini Mission/NASA.

In case you haven’t kept score on this long-running mission, the Cassini spacecraft left Earth on its one-way trip to Saturn twenty years ago, on October 14, 1997. I knew some of the folks on the team but was immersed in my own research into comets at the time. So, I followed it from afar for a while before getting hooked on its fantastic images a few years ago.

What a trip it’s been on! Cassini spent seven years getting to its target. It looped past Venus twice, and back by Earth before heading to Jupiter. Then, it slipped into orbit in the Saturnian system on July 1, 2004. By that time, it had already been imaging the planet and its moons and was ready to begin serious data-gathering.

Cassini’s Accomplishments In Review

pre grand finale aurorae sighted over southern pole
Aurorae over Saturn’s south pole. Courtesy NASA.

Over the years since then, the spacecraft has given us amazing looks at the moon Titan (both from orbit and via the Cassini-Huygens lander).  It also revealed incredible details about the moon Enceladus, including in-depth looks (and fly-throughs) of the jets of ice particles spewing from that moon. Of course, the rings and the planet’s atmosphere were major targets. Who would have thought that the rings had propellers? And kinks? And waves? And aurorae in the atmosphere? And that the atmosphere had such fascinating structures? The Hexagon alone is worth another spacecraft visit, in my opinion! For 13 years, the Cassini spacecraft has delivered the best solar system gift a planetary scientist could ask for: an in-depth look at a distant gas giant world. It will be a long time before humans can get out there and study it in person.

The Grand Finale Orbits

Now that it’s down to the last five orbits, what will Cassini be doing? As it gets closer to the planet, the spacecraft’s instruments will continue to measure Saturn’s immense gravitational field and its magnetic field. Such observations give valuable clues to the interior structure of the planet. It may actually reveal just how fast Saturn’s interior is rotating (which is where its magnetic field is generated).

Not surprisingly, with the spacecraft drawing ever-closer to the planet, the cameras are going to get a good look at the structure of the upper atmosphere as well as the rings. While it passes through ring-plane crossing, specialized instruments called “particle detectors” will study the tiny bits of ice that exist in the rings. In addition, Cassini scientists should get a very good feel for just how dense those rings really are. Finally, as the spacecraft plunges into the atmosphere, the mass spectrometer on board will sample the “air” and reveal more about the mix of gases that float high above the planet.

Why Send it Into Saturn?

It seems rather odd to be sending a working spacecraft into the planet at the end of its mission. In truth, the propellants are running low. In addition, Cassini’s instruments will eventually stop working. But, why not leave the spacecraft in a final orbit as a testament to the fantastic mission? The answer lies on the Saturn moons: pristine ice surfaces. Enceladus and Titan, in particular, could be targets if the spacecraft’s orbit should decay and cause it to stray through their orbits. That would bring Earth-based contaminants to these worlds. It’s not something anybody wants, particularly if there’s a chance of life existing on either of those moons. Or, what’s worse, if they’re home to compounds that could form life in the future. In either case, sending an Earth-based spacecraft their way would mess up the delicate balance that leads to or supports life. So, the safest thing is to send Cassini into the Saturnian atmosphere. There, it will burn up and any bio-contaminants would presumably be destroyed.

There’s a bit over a month left to enjoy the fruits of Cassini’s final orbits. Follow the news on the mission Web page and watch for announcements of new findings and images. It’s going to be a tremendous grand finale!

 

 

 

 

The Shadow of 2014 MU69 Tells a Tantalizing Tale

Is MU69 A Double-lobed World?

In just under a year and a half, the New Horizons spacecraft will pass by a distant Kuiper Belt Object called 2014 MU69.

No one was quite sure what shape this tiny world is, and the mission scientists needed to know. So, they put together an ingenious plan.
Earth-based observations gave the New Horizons scientists a tantalizing look by watching what’s called a “stellar occultation”. They watched as MU69 passed in front of a star on July 17, 2017,  watching a little eclipse-type event more accurately called an “occultation”. This was after a first occultation observation mission on June 3, 2017, was set up for observers in South Africa and Argentina, and a crew aboard the airborne Strategic Observatory for Infrared Astronomy (SOFIA) watched the event on July 10. The observations, plus high-resolution scans using Hubble Space Telescope (which looked for debris in the area right around MU69) gave clues to this little world’s shape.

Unlike eclipses, which can last for minutes, the MU69 occultations lasted only a few seconds. That was precious little time to gather information about the size and shape of the object. Scattering observers along pre-selected sites from where the event could be seen (and imaged) gave the New Horizons team much more data. That gave a better feel for what MU69’s shape must be.

What Does 2014 MU69 Look Like?

MU69
The Kuiper Belt object 2014 MU69 may be a double-lobed object or possibly a more spherical one with a chunk missing. The New Horizons spacecraft will fly by this object in January 2019. Courtesy JHU/APL/SWRI/Alex Parker

It turns out 2014 MU69 is pretty weird-looking, at least from our great distance from it. The measurements reveal what looks like a double-lobed object or maybe a tiny world with a big bite taken out of it. It’s not a perfectly round place. It’s also possible that 2014 MU69 could be two objects orbiting very close to (or even touching) one another — too close to be distinguished from each other. Right now, MU69 is more than 6.5 billion kilometers from Earth and its tiny size (about 30 km) makes it difficult to get a final answer about that oddball shape. Still, it’s a pretty amazing feat to use occultations and high-resolution measurements to get this far 17 months ahead of the flyby. It will be interesting to see how it all pans out as the spacecraft gets closer and returns better images. That won’t happen until later in 2018.

Threading the Needle at MU69

Not only is this information pretty cool to know for its own sake, but the observations made this summer also help the New Horizons mission planners do a more accurate job of targeting the flyby. That’s set for January 1, 2019. The closer they can get for a safe flyby, the better the science will be. However, it’s like threading an incredibly tiny needle. Obviously, it’s good to know if there’s a debris field orbiting along with 2014 MU69. We don’t want to see New Horizons whack into something that could be avoided.

Mission Science

The science to be gained at MU69 itself is incredibly important. However, the upcoming flyby will also tell us a lot about its environment. The Kuiper Belt, the third “regime” of the solar system, contains many objects that range in size from fairly small to some larger than Pluto. This one is among the smaller worldlets out there. The short-period comets also come from this region, and Pluto is among its more famous planetary bodies. MU69 lies on the way “out” of the solar system along the New Horizons trajectory from Pluto (which it explored on a quick flyby in July 2015). The mission is essentially sampling KBOs as it goes. From its data, we may see more than just this oddball world; if there’s debris, then that will also give clues to the population of objects in the neighborhood.

Questions about 2014 MU69

I can imagine all kinds of questions to be answered by the next flyby, all aimed at figuring out just how MU69 (and any companions) formed. Is nearby debris the result of an ancient collision? Or, could it be left over from MU69’s formation (which itself could be the result of a collision)? What’s it all made of? Are they mostly rocks? Mostly ice? A mix? If so, which ices are predominant out there? What do the surfaces look like? These are all questions to be answered with images and data from the flyby. New Horizons is our “forward scout”, exploring the territory ahead and giving ever-more-detailed answers about the outer frontiers of the solar system.

Addendum:  Check out the comments below, where artist Adolph Schaller shares his interpretation of the occultation data for MU69. He does a remarkable job of extrapolating the possible shape of this object.

Exploring Science and the Cosmos

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