Land On Titan With Huygens in Beautiful New Video

Published: 12 Jan , 2017
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On December 25, 2004, the piggybacking Huygens probe was released from the ‘mothership’ Cassini spacecraft and it arrived at Titan on January 14, 2005. The probe began transmitting data to Cassini four minutes into its descent through Titan’s murky atmosphere, snapping photos and taking data all the while. Then it touched down, the first time a probe had landed on an extraterrestrial world in the outer Solar System.

JPL has released a re-mix of the data and images gathered by Huygens 12 years ago in a beautiful new video. This is the last opportunity to celebrate the success of Huygens before Cassini ends its mission in September of 2017.

Watch as the incredible view of Titan’s surface comes into view, with mountains, a system of river channels and a possible lakebed.

After a two-and-a-half-hour descent, the metallic, saucer-shaped spacecraft came to rest with a thud on a dark floodplain covered in cobbles of water ice, in temperatures hundreds of degrees below freezing.

Huygens had to quickly collect and transmit all the images and data it could because shortly after landing, Cassini would drop below the local horizon, “cutting off its link to the home world and silencing its voice forever.”

How much of this video is actual images and data vs computer graphics?

Of course, the clips at the beginning and end of the video are obviously animations of the probe and orbiter. However, the slow descending 1st-person point-of-view video is made using actual images from Huygens. But Huygens did not take a continuous movie sequence, so a lot of work was done by the team that operated Huygens’ optical imager, the Descent Imager/Spectral Radiometer (DISR), to enhance, colorize, and re-project the images into a variety of formats.

The view of the cobblestones and the parachute shadow near the end of the video is also created from real landing data, but was made in a different way from the rest of the descent video, because Huygens’ cameras did not actually image the parachute shadow. However, the upward looking infrared spectrometer took a measurement of the sky every couple of seconds, recording a darkening and then brightening to the unobstructed sky. The DISR team calculated from this the accurate speed and direction of the parachute, and of its shadow to create a very realistic video based on the data.

If you’re a data geek, there are some great videos of Huygens’ data by the University of Arizona Lunar and Planetary Laboratory team, such as this one:

The movie shows the operation of the DISR camera during the descent onto Titan. The almost 4-hour long operation
of DISR is shown in less than five minutes in 40 times actual sped up to landing and 100 times actual speed thereafter.

Erich Karkoschka from the UA team explained what all the sounds in the video are. “All parts of DISR worked together as programmed, creating a harmony,” he said. Here’s the full explanation:

Sound was added to mark various events. The left speaker follows the motion of Huygens. The pitch of the tone indicates the rotational speed. Vibrato indicates vibration of the parachute. Little clicks indicate the clocking of the rotation counter. Noise corresponds to heating of the heat shield, to parachute deployments, to the heat shield release, to the jettison of the DISR cover, and to touch down.

The sound in the right speaker follows DISR data. The pitch of the continuous tone goes with the signal strength. The 13 different chime tones indicate activity of the 13 components of DISR. The counters at the top and bottom of the list get the high and low notes, respectively.

You can see more info and videos created from Huygens’ data here.

Read some reminiscences about Huygens from some of the Cassini team here.

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5 Responses

  1. Aqua4U says:

    Beautiful! WHO will be the first human to set foot on Titan? Alive today? Probably not.. but maybe?

  2. Pvt.Pantzov says:

    wow, I wasn’t expecting to feel such nostalgia while watching this. what a time!

  3. ProfMOZ says:

    Beautiful, but old footage… and secondly, a moon, about 5000 km in diameter has an atmosphere almost as thick as earth?
    Who can answer that?

    • G.Freeman says:

      Titan is close enough to the Sun to have nitrogen still not frozen, but far enough from strong solar wind rapidly blowing out the atmosphere.

      There’s no magnetic field to protect it, so it’s leaking. Thing is Titan is really huge compared to other moons of Saturn, during forming from protoplanetary disk it grabbed almost all volatiles, (just like Jupiter trapped most of hydrogen in early solar system) so it has a big reservoir of them, even if it’s constantly bleeding the atmosphere.

      At least that’s how I think it happened.

  4. paul w says:

    Am I the only one who is heartily sick and tired of having massive text splattered across videos?

    What thought process went on here?

    “Hey, we have a great video of a probe landing on another moon, let’s put huge text all over the images!”

    Please. Stop.

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