ESA Science News Release – SNR 3-2005


First measurement of Titan’s winds from Huygens

Using a global network of radio telescopes, scientists have measured the speed of the winds faced by Huygens during its descent through the atmosphere of Titan. This measurement could not be done from space because of a configuration problem with one of Cassini’s receivers. The winds are weak near the surface and increase slowly with altitude up to about 60 km, becoming much rougher higher up where significant vertical wind shear may be present.

Preliminary estimates of the wind variations with altitude on Titan have been obtained from measurements of the frequency of Huygens’ radio signals recorded during the probe’s descent on 14 January 2005. These "Doppler" measurements, obtained by a global network of radio telescopes, reflect the relative speed between the transmitter on Huygens and the receiver on the Earth. Winds in the atmosphere affected the speed of Huygens’ descent and produced a change in the frequency of the signal received on Earth, in a manner similar to the commonly heard change in a siren's pitch from a speeding police car.

Leading the list of large radio antennas involved in the programme were the NRAO Robert C. Byrd Green Bank Telescope (GBT) in WestVirginia, USA, and the CSIRO Parkes Radio Telescope in Australia. Special instrumentation designed for detection of weak signals was used to measure the "carrier" frequency of the Huygens radio signal during this unique opportunity. The initial detection, made with the "Radio Science Receivers" on loan from NASA’s Deep Space Network, provided the first unequivocal proof that Huygens had survived the entry phase and had begun its radio relay transmission to Cassini.

The very successful signal detection on Earth provided a surprising turnabout for the Cassini-Huygens Doppler Wind Experiment (DWE), whose data could not be recorded on the Cassini spacecraft due to a commanding error needed to properly configure the receiver. “Our team has now taken a significant first step to recovering the data needed to fulfil our original scientific goal, an accurate profile of Titan's winds along the descent trajectory of Huygens,” said DWE’s Principal Investigator Dr Michael Bird (University of Bonn, Germany). The ground-based Doppler measurements were carried out and processed jointly by scientists from the NASA Jet Propulsion Laboratory (JPL, USA) and the Joint Institute for VLBI in Europe (JIVE, The Netherlands) working within the DWE team.

Winds on Titan are found to be flowing in the direction of Titan's rotation (from west to east) at nearly all altitudes. The maximum speed of roughly 120 m/s (430 km/hour) was measured about ten minutes after the start of the descent, at an altitude of about 120 km. The winds are weak near the surface and increase slowly with altitude up to about 60 km. This pattern does not continue at altitudes above 60 km, where large variations in the Doppler measurements are observed. Scientists believe that these variations may arise from significant vertical wind shear. That Huygens had a rough ride in this region was already known from the science and engineering data recorded on board Huygens.

“Major mission events, such as the parachute exchange about 15 minutes into the atmospheric flight and impact on Titan at 13:45 CET, produced Doppler signatures that we can clearly identify in the data,” Bird said.


At present, there exists an approximately 20-minute interval with no data between the measurements at GBT and Parkes. This gap in Doppler coverage will eventually be closed by data from other radio telescopes which are presently being analysed. In addition, the entire global set of radio telescopes performed Very Long Baseline Interferometry (VLBI) recordings of Huygens’ signal to determine the probe’s precise position during the descent.

“This is a stupendous example of the effectiveness of truly global scientific cooperation,” said Jean-Pierre Lebreton, ESA Huygens Project Scientist. “By combining the Doppler and VLBI data we will eventually obtain an extremely accurate three-dimensional record of the motion of Huygens during its mission at Titan,” he concluded.

-end-


Note for editors


The radio astronomy support of the Huygens mission is coordinated by JIVE and JPL and involves the Netherlands Foundation for Research in Astronomy (ASTRON, The Netherlands), the University of Bonn (Germany), Helsinki University of Technology (Espoo, Finland), the MERLIN National Facility (Jodrell Bank, UK), the Onsala Space Observatory (Sweden), the NASA Jet Propulsion Laboratory (Pasadena, USA), the National Radio Astronomy Observatory (NRAO, Green Bank, USA, and Socorro, USA), the CSIRO Australia Telescope National Facility (ATNF, Sydney, Australia), the University of Tasmania (Hobart, Australia), the National Astronomical Observatories of China, the Shanghai Astronomical Observatory (Shanghai and Urumqi, China) and the National Institute of Information and Communications Technologies (Kashima Space Research Center, Japan).

The Joint Institute for VLBI in Europe is hosted by ASTRON and funded by the national research councils, national facilities and institutes of The Netherlands (NOW), the United Kingdom (PPARC), Italy (CNR), Sweden (Onsala Space Observatory, National Facility), Spain (IGN) and Germany (MPIfR). The National Radio Astronomy Observatory is operated by Associated Universities, Inc., under a cooperative agreement with the National Science Foundation. The Australia Telescope is funded by the Commonwealth of Australia for operation as a National Facility managed by CSIRO. The Jet Propulsion Laboratory is operated by the California Institute of Technology under contract to NASA.


More about Cassini-Huygens

The Cassini-Huygens mission is a cooperation between NASA, ESA and ASI, the Italian space agency. The Jet Propulsion Laboratory (JPL), a division of the California Institute of Technology in Pasadena, is managing the mission for NASA's Office of Space Science, Washington DC. JPL designed, developed and assembled the Cassini orbiter while ESA operated the Huygens atmospheric probe. For more information about Cassini-Huygens please see:


http://saturn.esa.int


For further information please contact:

Dr Jean-Pierre Lebreton

Huygens Project Scientist

European Space Agency

Noordwijk, The Netherlands

Tel: +31 71 565 3600

E-mail: jplebret @ rssd.esa.int


Dr Michael Bird

University of Bonn

Bonn, Germany

Tel: +49 228 733 651

E-mail: mbird @ astro.uni-bonn.de


Dr Leonid Gurvits

Joint Institute for VLBI in Europe

Dwingeloo, The Netherlands

Tel: +31 521 596 514

E-mail: lgurvits @ jive.nl


Dr Guido De Marchi

Science Communication Office

European Space Agency

Noodrwijk, the Netherlands

Tel: +31 71 565 8332

E-mail: gdemarchi @ rssd.esa.int


Media Relations Division

European Space Agency

Paris, France

Tel: +33 1 5369 7155

Fax: +33 1 5369 7690