In the 1970s and 80s, before advanced computer graphics, artist Ken Hodges was hired by JPL to create paintings that depicted many different missions – some in the planning stages and some only imagined.
Bruce Murray became JPL's Director in 1976, and he advocated new missions (Purple Pigeons) that would have enough pizzazz to attract public and scientific support. Hodges painted many of the Purple Pigeon images, including this scene of a Saturn orbiter with a lander going to the surface of Saturn's largest moon Titan. This artwork was done almost 30 years before Cassini's Huygens Probe reached the surface of Titan. Cassini was launched in 1997 and spent seven years traveling to Saturn. The probe was released in December 2004, and landed on Titan on January 14, 2005.
For more information about the history of JPL, contact the JPL Archives for assistance. [Archival and other sources: P-numbered photo albums and indexes, Cassini and Huygens web pages.]
On Sunday evening, my eyes were glued to eight windows on my computer screen, watching data pop up every few seconds. NASA's Cassini spacecraft was making its lowest swing through the atmosphere of Saturn's moon Titan and I was on the edge of my seat. Trina Ray, a Titan orbiter science team co-chair, was keeping me company. Five other members of my team were also at JPL. Between us, we were keeping an eye on about 2,000 data channels.
One of the 34-meter antennas at the Deep Space Network's Goldstone complex, DSS-24, was pointed at Saturn and listening for the signal that was expected to be here in just a few minutes. The data would be arriving at my computer as quickly as they could be sent back to Earth, though there was an agonizing hour-and-18-minute delay because of the distance the data had to travel. (We call this flyby T70, but it is actually Cassini's 71st flyby of Titan.)
It was a nervous time for me -- the previous night we had been at JPL to send some other real-time commands to the spacecraft when an alarm came in indicating that the magnetometer, the prime instrument taking data for the T70 flyby, needed a reset. Fortunately, the controller on duty immediately called the magnetometer instrument operations team lead in England. Within 90 minutes, the commands were on their way to do a computer reset and clear the alarm. At 2 a.m. Pacific time on Sunday, we got the email indicating all was well and the magnetometer was ready for the Titan closest approach.
So here we were, past one hurdle, hoping nothing else would come up. We had run hundreds of simulations over the past three-and-a-half years, so I knew we had done everything we could think to do. We did more training for this event than anything else we had done since we dropped off the Huygens probe in January 2005 for a descent through the moon's hazy atmosphere.
Right on time, at 7:26 p.m., the Deep Space Network locked on the spacecraft downlink, a good start. I was focused on the data for spacecraft pointing. As long as we stayed within an eighth of a degree of the expected pointing, everything would be fine. At 7:45 p.m., we got the data from closest approach, a mere 880 kilometers (547 miles) in altitude. Over the vocabox, a cross between a telephone and walkie-talkie, the attitude control team reported that the thrusters were firing about twice as much as we expected. The Titan atmosphere appeared to be a little thicker than we expected, even though we had fed about 40 previous low Titan flybys by Cassini and the descent data from Huygens into our modeling.
But spacecraft control was right on the money, keeping the pointing within our predicted limits. Even with the extra thrusting, we stayed well within our safety margin.
At 7:53 p.m., the spacecraft turned away to go to the next observation. I let out a sigh of relief, happy that everything during closest approach had gone just as we planned. Five attitude control guys crowded into my office with smiles on their faces. Trina and I were marveling at what a wonderful spacecraft we have to work with. Another first for the Cassini mission!
Now, as Trina says, we have to finish the job by returning all the great science data. We have data playbacks today at two different Deep Space Network stations to make sure we have - as we say here - both belts and suspenders. Engineers will also go back to analyze the data with the scientists to see just how dense the Titan atmosphere turned out to be at our flyby altitude.
But last night, at least, my team and I went home happy!
This weekend, Cassini will embark on an exciting mission: trying to establish if Titan, Saturn's largest moon, possesses a magnetic field of its own. This is important for understanding the moon's interior and geochemical evolution.
For Titan scientists, this is one of the most anticipated flybys of the whole mission. We want to get as close to the surface with our magnetometer as possible for a one-of-a-kind scan of the moon. Magnetometer team scientists (including me) have a reputation for pushing the lower limits. In a world of infinite possibilities, we would have liked many flybys at 800 kilometers. But we went back and forth a lot with the engineers, who have to ensure the safety of the spacecraft and fuel reserves. We agreed on one flyby at 880 kilometers (547 miles) and both sides were happy.
Flying at this low altitude will mark the first time Cassini will be below the moon's ionosphere, a shell of electrons and other charged particles that make up the upper part of the atmosphere. As a result, the spacecraft will find itself in a region almost entirely shielded from Saturn's magnetic field and will be able to detect any magnetic signature originating from within Titan.
Titan orbits within the confines of the magnetic bubble around Saturn and is permanently exposed to the planet's magnetic disturbances. Previous measurements by NASA's Voyager spacecraft and Cassini at altitudes above 950 kilometers (590 miles) have shown that Titan does not possess an appreciable magnetic field capable of counterbalancing Saturn's. However, this does not imply that Titan's field is zero. We'd like to know what the internal field might be, no matter how small.
The internal structure of Titan can be probed remotely from its gravitational field or its magnetic properties. Planets with a magnetic field -- like Titan's parent Saturn or our Earth -- are believed to generate their global-scale magnetic fields from a mechanism called a dynamo. Dynamo magnetic fields are generated from currents in a molten core where charge-conducting materials such as metals are flowing around each other and also undergoing other stresses because of the planet's rotation.
We might not find a magnetic field at all. A positive detection of an internal magnetic field from Titan could imply one of the following:
a) Titan's interior still bears enough energy to sustain a dynamo.
b) Titan's interior is "cold" (and therefore has no dynamo), but its crust is magnetized in a similar way as Mars' crust. If this is the case, we should find out how this magnetization took place.
c) Something under the surface of Titan got charged temporarily by Saturn's magnetic field before this Cassini flyby. While I said earlier that the ionosphere shields the Titan atmosphere from Saturn's magnetic bubble, the ionosphere is only an active shield when the moon is exposed to sunlight. During part of its orbit around the planet, Titan is in the dark and magnetic field lines from Saturn can reach the Titan surface. A temporary magnetic field can be created if there is a conducting layer, like an ocean, on or below the moon's crust.
Once Cassini leaves Titan, the spacecraft will perform a series of rolls to fine-calibrate its magnetometer in order to assess T70 measurements with the highest precision. We're looking forward to poring through the data coming down, especially after all the negotiations we had to make for them!