Forum for Science, Industry and Business

Sponsored by:     3M 
Search our Site:

 

Second space Christmas for ESA: Huygens to begin its final journey to Titan

07.12.2004


One year after Mars Express’ arrival at Mars, the mighty rules of celestial mechanics have again set Christmas as the date for a major ESA event in deep space.



At 1.25 billion km from Earth, after a 7-year journey through the Solar system, ESA’s Huygens probe is about to separate from the Cassini orbiter to enter a ballistic trajectory toward Titan, the largest and most mysterious moon of Saturn, in order to dive into its atmosphere on 14 January. This will be the first man-made object to explore in-situ this unique environment, whose chemistry is assumed to be very similar to that of the early Earth just before life began, 3.8 billion years ago.

The Cassini-Huygens pair, a joint mission conducted by NASA, ESA and the Italian space agency (ASI), was launched into space on 15 October 1997. With the help of several gravity assist manoeuvres during flybys of Venus, Earth and Jupiter, it took almost 7 years for the spacecraft to reach Saturn.


The Cassini orbiter, carrying Huygens on its flank, entered an orbit around Saturn on 1 July 2004, and began to investigate the ringed planet and its moons for a mission that will last at least four years.

The first distant flyby of Titan took place on 2-3 July 2004. It provided data on Titan’s atmosphere which were confirmed by the data obtained during the first close flyby on 26 October 2004 at an altitude of 1174 km. These data were used to validate the entry conditions of the Huygens probe. A second close flyby of Titan by Cassini-Huygens at an altitude of 1200 km is scheduled on 13 December and will provide additional data to further validate the entry conditions of the Huygens probe.

On 17 December the orbiter will be placed on a controlled collision course with Titan in order to release Huygens on the proper trajectory, and on 21 December (some dates and times are subject to minor adjustment for operational reasons, except the entry time on 14 January which is know to within an accuracy of under 2 minutes) all systems will be set up for separation and the Huygens timers will be set to wake the probe a few hours before its arrival at Titan.

The Huygens probe is due to separate on the morning of 25 December at about 05:08 CET. Since the Cassini orbiter will have to achieve precise pointing for the release, there will be no real-time telemetry available until it turns back its main antenna toward Earth and beams the recorded data of the release. It will take over an hour (67 min) for the signals to reach us on Earth. The final data confirming the separation will be available later on Christmas Day.

After release, Huygens will move away from Cassini at a speed of about 35 cm per second and, to keep on track, will spin on its axis, making about 7 revolutions a minute. Huygens will not communicate with Cassini for the whole period until after deployment of the main parachute following entry into Titan’s atmosphere. On 28 December Cassini will then manoeuvre off collision course to resume its mission and prepare itself to receive Huygens data, which it will record for later playback to Earth.

Huygens will remain dormant until a few hours before its arrival at Titan on 14 January. The entry into the atmosphere is set for 11:15 CET. Huygens is planned to complete its descent in about two hours and 15 minutes, beaming back its science data to the Cassini orbiter for replay to Earth later in the afternoon. If Huygens, which is designed as an atmospheric probe rather than a lander, survives touchdown on the surface, it could deliver up to 2 hours of bonus data before the link with Cassini is lost.

Direct radio signals from Huygens will reach Earth after 67 minutes of interplanetary travel at the speed of light. An experiment has been set up by radio scientists that will use an array of radio telescopes around the Pacific to attempt to detect a faint tone from Huygens. If successful, early detection is not expected before around 11:30 CET.

The European Space Agency owns and manages the Huygens probe and is in charge of operations of the probe from its control centre in Darmstadt, Germany. NASA’s Jet Propulsion Laboratory in Pasadena, California, designed, developed and assembled the Cassini orbiter. NASA’s Deep Space Network, also managed by JPL, will be providing communications support via the Cassini orbiter and relaying it to ESA’s control centre in Darmstadt for processing. The Italian Space Agency provided the high-gain antenna on the Cassini orbiter, much of the radio system and elements of several of Cassini’s science instruments. The Huygens payload has been provided by teams including from CNES, DLR, ASI and PPARC, and outside Europe, from NASA.

Practical arrangements for the Media wishing to cover the event

These dramatic events marking the first attempt ever to unveil the mysteries of Titan in-situ, a distant world bigger than Mercury and Pluto which may hold clues to the early days of our own planet, will be marked by several media activities not to be missed. Pencil them into your diary.

Saturday 25 December

Spacecraft operations will be run at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California.

The ESA Media Relations Office in Paris will be operational from 04:00 hrs to 12:00 CET. ESA specialists can be reached for interviews and comments via the ESA News Desk on +33(0)1.53.69.71.55.

Contacts: Franco Bonacina, Anne-Marie Rémondin, Roberto Lo Verde.

Interviews from JPL can also be arranged by calling the JPL media relations office at + 1. 818-354-5011.

ESA specialists at JPL: Jean-Pierre Lebreton, Claudio Sollazzo.

05:08 CET - Expected separation of the Huygens probe from the Cassini orbiter

~07:00 CET - Status report upon successful separation from NASA/JPL

10:00 CET at the latest : ESA press release assessing the separation of the Huygens probe

~10:00 CET - ESA TV Video News Release produced at JPL during separation (contact for TVs: Claus Habfast: + 31(0)6.51.18.14.96, claus.habfast@esa.int)

Transmission details will be on http://television.esa.int

12:00 CET - Replay of ESA TV Video News Release on separation

Thursday 13 January

ESA’s ESOC establishment in Darmstadt, Germany, will act as the main European press centre. The Huygens Principal Investigators, the ESA Huygens Mission Manager and Project Scientist will be at ESA/ESOC and available for interviews. If you wish to attend the media activities at ESOC, please return the accreditation form (link on the right).

Press Contacts:

Jocelyne Landeau-Constantin
jocelyne.landeau-constantin@esa.int (+49(0)6151.90.2696)

Bernhard von Weyhe
Bernhard.von.Weyhe@esa.int (+49(0)6151.90.2516).

17:00-17:30 CET - Press briefing at ESA/ESOC Control Centre. Televised on ESA TV - This event can also be followed remotely by phone : +49(0)69.4035.9681.

Friday 14 January

Media briefings originated at ESA/ESOC will also be retransmitted to several ESA establishments and across Europe: Cité des Sciences/ La Villette in Paris (F), (event hosted in coordination with ESA and CNES)
ESA/ESTEC in Noordwijk (NL)
ESA/ESRIN Frascati (I)
ESA/ESAC in Villafranca (E)
Central London (event hosted by PPARC).

ESA specialists will be on hand at the various locations for interviews.

If you wish to attend the briefings at one of these venues, please contact the local Communication services directly.

ESA for Cité des Sciences, Paris (F):
Anne-Marie Rémondin (Anne-Marie.Remondin@esa.int) + 33(0)1.5369.7155
Brigitte Kolmsee (Brigitte.Kolmsee@esa.int), + 33(0)1.5369.7299

ESA/ESTEC,Noorwijk Space Expo (NL): + 31(0)71.565.3006- Wil Spangenberg (Wil.Spangenberg@esa.int)

ESA/ESRIN, Frascati (I): + 39 06 9418 0951- Franca Morgia (Franca.Morgia@esa.int)

ESA/ESAC, Villafranca (E): + 34 91 813 11 00 - Monica Oerke (Monica.Oerke@esa.int)

PPARC, London (UK) : Peter Barratt + 44 (0)1793 44 20 25 (Peter.Barratt@pparc.ac.uk)

ESA TV Broadcast schedule for 14 January 2005

09:00-09:30 CET - ESA TV broadcast - Cassini turns to Huygens - Feeds from ESA/ESOC main Control Room

11:00-12:15 CET - ESA TV Broadcast - Probe activation to parachute deployment and status of tracking by radio-telescope

13:30-14:00 CET - Press briefing at ESA/ESOC: Huygens descent update (possible results from ground radio telescope observations – televised on ESA TV

14:30-15:00 CET - ESA TV broadcast: mission update

16:00-16:30 CET - ESA TV broadcast: mission update

As of 17:15 CET - Press briefing: arrival of first data – televised on ESA TV

23:00-24:00 CET - Press briefing: presentation of first image if available) - Televised on ESA TV

All events can also be followed (audio only) by calling + 49(0)69.4035.9681 and highlights of ESA TV can be watched on the Web at http://saturn.esa.int

Saturday 15 January

11:00-12:00 CET - Press conference at ESA/ESOC: presentation of the first image, sounds, etc. - not broadcast live on ESA TV. This event can also be followed (audio only) by calling + 49(0)69.4035.9681.

A video news release with the highlights will be available on ESA TV for broadcasters immediately at the end of the press conference.

Satellite details for ESA TV broadcast reception:

The ESA TV Service provides live broadcasts of ESA’s most important events on the Astra 2-C satellite, using a digital transponder that enables everyone in the satellite’s footprint, with a digital receiver and a parabolic pointing at 19.2 degrees East, to follow these events.

For more information and updates, please check the ESA TV Website: http://television.esa.int .

On the Web

You can follow all main Cassini/Huygens mission events on the ESA web at: http://saturn.esa.int Bookmark now! If you have not already done so, subscribe to the ESA portal news service at http://www.esa.int/esaCP/subscribers.html
to get the latest news on this fascinating mission directly into your mail box.

Here you will find information on Cassini-Huygens and its status, a rich selection of multimedia material, news on the separation of Huygens from the Cassini orbiter and the latest updates on January 13. There will be continuous coverage during the last exciting hours of the descent on 14 January, with the first image expected late on 14 January or on 15 January.

Messages from earthlings and pop music heading to Titan

Before the mission was launched, ESA offered Europeans a unique opportunity to send a message to the unknown. Over 80 000 people wanted to share the excitement of this mission and wrote or drew a message that was engraved on a CD-ROM put on board the Huygens probe. The messages can be seen on http://television.esa.int/Huygens/index.cfm

The same CD ROM carries four pop songs, composed by French musicians Julien Civange and Louis Haéri. More about this project at http://www.music2titan.com

Specific information for media representatives going to ESA/ESOC

Getting there:

The nearest airport is Frankfurt-am-Main and it takes about 20 minutes by taxi to get to ESA/ESOC. A shuttle bus is also available from the airport approximately every 30 minutes. There are also frequent trains (approx. every 40 minutes) from the airport to Darmstadt (one change).

http://www.heag.de/verkehr/02_02.html http://www.bahn.de/pv/view/index.shtml

Accommodation:

Darmstadt has many hotels, ranging in price from € 68 to € 230 (the closest to ESA/ESOC is a 4-star Maritim Konferenz Hotel, in walking distance from the Control Centre). For further information about Darmstadt hotels go to http://www.proregio-darmstadt.de/uebernachten/hotel.asp. If you need help with accommodation, do not hesitate to contact the ESA/ESOC travel office on +49(0)6151.902.885.

Laptops/ Internet/ Cell Phones:

Power supply rating: 220-240 volts (adaptor plug available in most hardware stores or at most international airport shops). Most North American cell phones will not work in Europe unless they are tri-band phones.

Internet via LAN: Standard network connector RJ45 required in laptop.

Internet via analogue modem: Standard RJ11 connector in laptop, special German Telekom TAE connection to the socket.

Internet via ISDN: PCMCIA Card inside Laptop, RJ45 in the wall.

The ESA/ESOC Press Rooms are equipped with ISDN and standard network with RJ45 cable. No wireless LAN is available for the media. Analog lines can be provided if needed.

For further information, please contact:

ESA/ESOC Media Relations:
Jocelyne Landeau-Constantin:
Tel : +49(0)6151.90.2696:
jocelyne.landeau-constantin@esa.int

ESA/HO Media Relations:

Franco Bonacina
Tel : + 33(0)1.5369.7155
Franco.Bonacina1@esa.int

JPL Media Relations:

Carolina Martinez
Tel: + 1 818-354-9382 or + 1 818-354-5011
Carolina.Martinez@jpl.nasa.gov

Franco Bonacina | EurekAlert!
Further information:
http://www.esa.int/esaCP/SEMUPZWDE2E_index_0.html
http://www.esa.int

More articles from Physics and Astronomy:

nachricht SwRI-led team discovers lull in Mars' giant impact history
26.04.2017 | Southwest Research Institute

nachricht New survey hints at exotic origin for the Cold Spot
26.04.2017 | Royal Astronomical Society

All articles from Physics and Astronomy >>>

The most recent press releases about innovation >>>

Die letzten 5 Focus-News des innovations-reports im Überblick:

Im Focus: Making lightweight construction suitable for series production

More and more automobile companies are focusing on body parts made of carbon fiber reinforced plastics (CFRP). However, manufacturing and repair costs must be further reduced in order to make CFRP more economical in use. Together with the Volkswagen AG and five other partners in the project HolQueSt 3D, the Laser Zentrum Hannover e.V. (LZH) has developed laser processes for the automatic trimming, drilling and repair of three-dimensional components.

Automated manufacturing processes are the basis for ultimately establishing the series production of CFRP components. In the project HolQueSt 3D, the LZH has...

Im Focus: Wonder material? Novel nanotube structure strengthens thin films for flexible electronics

Reflecting the structure of composites found in nature and the ancient world, researchers at the University of Illinois at Urbana-Champaign have synthesized thin carbon nanotube (CNT) textiles that exhibit both high electrical conductivity and a level of toughness that is about fifty times higher than copper films, currently used in electronics.

"The structural robustness of thin metal films has significant importance for the reliable operation of smart skin and flexible electronics including...

Im Focus: Deep inside Galaxy M87

The nearby, giant radio galaxy M87 hosts a supermassive black hole (BH) and is well-known for its bright jet dominating the spectrum over ten orders of magnitude in frequency. Due to its proximity, jet prominence, and the large black hole mass, M87 is the best laboratory for investigating the formation, acceleration, and collimation of relativistic jets. A research team led by Silke Britzen from the Max Planck Institute for Radio Astronomy in Bonn, Germany, has found strong indication for turbulent processes connecting the accretion disk and the jet of that galaxy providing insights into the longstanding problem of the origin of astrophysical jets.

Supermassive black holes form some of the most enigmatic phenomena in astrophysics. Their enormous energy output is supposed to be generated by the...

Im Focus: A Quantum Low Pass for Photons

Physicists in Garching observe novel quantum effect that limits the number of emitted photons.

The probability to find a certain number of photons inside a laser pulse usually corresponds to a classical distribution of independent events, the so-called...

Im Focus: Microprocessors based on a layer of just three atoms

Microprocessors based on atomically thin materials hold the promise of the evolution of traditional processors as well as new applications in the field of flexible electronics. Now, a TU Wien research team led by Thomas Müller has made a breakthrough in this field as part of an ongoing research project.

Two-dimensional materials, or 2D materials for short, are extremely versatile, although – or often more precisely because – they are made up of just one or a...

All Focus news of the innovation-report >>>

Anzeige

Anzeige

Event News

Expert meeting “Health Business Connect” will connect international medical technology companies

20.04.2017 | Event News

Wenn der Computer das Gehirn austrickst

18.04.2017 | Event News

7th International Conference on Crystalline Silicon Photovoltaics in Freiburg on April 3-5, 2017

03.04.2017 | Event News

 
Latest News

Scientist invents way to trigger artificial photosynthesis to clean air

26.04.2017 | Materials Sciences

Ammonium nitrogen input increases the synthesis of anticarcinogenic compounds in broccoli

26.04.2017 | Agricultural and Forestry Science

SwRI-led team discovers lull in Mars' giant impact history

26.04.2017 | Physics and Astronomy

VideoLinks
B2B-VideoLinks
More VideoLinks >>>