Below are the "Herschel News" archive covering the period 2000-2008. The most recent information about the progresses of the Herschel Mission and the status of the Science Instruments can be found on the "Latest News".
System Operational Validation Test (SOVT-1) executed.
The first System Operational Validation Test (SOVT-1) has been executed on 6-10 September 2008.
For the first time, the whole Science Ground Segment (SGS) has been
connected together and operating with the Mission Operations Centre (MOC)
and the spacecraft in a complete end-to-end test simulating four days of
routine science operations.
The whole system has been exercised from the
generation of observation requests and schedules, the uplinking of command
timelines, through actual execution by the spacecraft, downlinking of the
generated telemetry, ingestion of the data by the Herschel Science Centre (HSC)
and performing pipeline data processing and product archiving and retrieval,
data propagation to the Instrument control Centres (ICCs), and responding
to Helpdesk questions and Targets of Opportunity. Pictures from left to right:
Sarah Leeks (SPIRE) monitoring the recycling of the He-3 cooler, Göran
Pilbratt explaining what is going on to Saku Tsuneta and Clare Bingham,
the MOC running the show, and the HSC videoconferencing with the rest of the SGS. [September 2008]
Herschel vibration testing completed.
After the acoustics campaign and associated post-testing the Herschel
spacecraft was transferred to another part of the ESTEC Test Centre
for the vibration runs. The actual testing on the shaker was performed
in the period 20 June - 3 July 2008. In each of the three spacecraft axes,
longitudinal (x) and transverse (z and y), four test runs were conducted,
at low, intermediate, and acceptance levels, followed by another low level
run. The four pictures above show Herschel on 26 June, positioned for z-axis
vibration. For some additional pictures and a video on the x-axis shaking
see also the SciTech webpage.
[July 2008]
Herschel acoustic testing performed.
Based on the availability of test facilities it was decided to perform
acoustics testing before vibration rather than, as initially foreseen,
the other way round. In the pictures above Herschel is seen during the
final test preparations in the Large European Acoustic Facility (LEAF)
in the ESTEC Test Centre. The left picture also provides a nice view
of the local oscillator unit (LOU) radiator. The telescope cover has
been removed which indicates that the start of testing is imminent.
The 'rings' which can be seen (in visible light!) on the telescope
primary mirror is a purely cosmetic effect. The acoustics testing runs
were performed on 5-6 June 2008.
[June 2008]
Herschel mechanical testing underway.
After completing the EMC campaign mechanical testing of Herschel is now
underway. The initial activities concerned PACS chopper and grating tuning
which was performed with the spacecraft inclined at an angle of 20°
(left two pictures). Then exceptionally Herschel was tilted 90°
to perform SPIRE SMEC testing, and the telescope cover was removed to perform
an M1-M2 distance confirmation measurement (right two pictures) which will be
repeated after the upcoming vibration and acoustics tests at spacecraft level
have been performed; see also the SciTech webpage.
[May 2008]
Herschel in Maxwell EMC chamber.
The Herschel spacecraft has been tested in the Maxwell EMC chamber. The pictures above were taken on 13 May 2008 as the final preparations for moving the spacecraft out of the chamber were being performed. The third picture from the left shows members of the industry and ESA Herschel teams while the image on the extreme right shows the Planck (with crossed arms) and Herschel Project Scientists posing in front of the spacecraft.
[May 2008]
Herschel spacecraft mechanical completion.
The Herschel spacecraft is nearing mechanical completion. These pictures
taken one week after telescope integration from inside the cleanroom
show three views of the spacecraft under completion. The major still to
be integrated items are the the LOU radiator and the thermal shield
between the SVM and the cryostat. Spacecraft alignment activities are
underway in late April, in May EMC and mechanical qualification
activities are due to commence.
[April 2008]
Herschel telescope mated to spacecraft.
During a long day on 16 Apr 2008 the Herschel telescope was mechanically
integrated onto the interface structure on the cryostat. The actual
lifting and placing of the telescope took place in the course of a
few hours in the afternoon. From left to right: telescope attached to
crane and ready to be hoisted (note the cover secured not touching the
telescope); telescope in transit; and telescope in place on the cryostat.
These pictures were taken from the viewing gallery outside the cleanroom
(through a window). The telescope integration was preceeded by solar
array/sunshade integration, for pictures from inside the cleanroom on both
of these events see the SciTech webpage.
[April 2008]
Herschel telescope ready for integration.
The Herschel telescope is now ready for integration onto the spacecraft! Personnel from the Astrium, Toulouse have completed the installation of accelerometers for the upcoming mechanical and acoustic tests at spacecraft level. These were the last steps needed on the telescope prior to its integration onto the cryostat telescope mounting structure. The integration of the Herschel solar array/sunshade will be performed before that of the telescope.
[April 2008]
Cryostat cooldown and System Validation Test.
After the conclusion of the the cryostat bake-out and the subsequent warm functional tests of the science instruments, the preparations for cooldown commenced. The cryostat was enclosed by scaffolding (left) and the cooldown to 'normal' helium (He-I) conditions commenced on 13 Feb 2008. A full main helium tank (nominally 2367 litres) was achieved on 1 March 2008, having used almost 10,000 litres of helium in the process (middle), see also the Herschel SciTech website.
Post cooldown additional functional testing of the spacecraft and its payload continued in order to conduct the second System Validation Test (SVT-1; the first was called SVT-0). The purpose of SVT-1 was to test and validate the external interfaces from the Missions Operations Centre (MOC, in ESOC) to the satellite (in ESTEC), in closed loop, and to validate the satellite telemetry and telecommand database definition, making use of satellite nominal and contingency flight operations procedures. The SVT-1 was performed in the period 11-20 March 2008, its successful conclusion was celebrated by the testing team (right).
[March 2008]
Herschel Key Programme time allocation completed.
The Key Programme (KP) time allocation process has been completed for both guaranteed time (GT) and open time (OT) observations. In addition to the 21 KP GT programmes by coincidence also precisely 21 KP OT programmes have been awarded observing time. In the left picture above the sky distribution of the targets is shown, while in the right picture the use shares of the instruments are depicted. These programmes are described under Key Programmes.
[February 2008]
Herschel solar array flashertests. The Herschel solar array has been subjected to a "flashertest". Here the performance of the solar array is measured by means of subjecting it to flashes with a near solarlike spectrum and measuring its output. A calibrated reference solar cell is also subjected to these flashes, and by comparison of the measured outputs the performance of the Herschel solar array can be verified. Meanwhile the Herschel cryostat cooldown is underway.
[February 2008]
Herschel telescope unpacked, inspected, cleaned, and tested. The Herschel telescope has been unpacked and the incoming inspection has been performed. A small amount of loose dust was removed by a non-touching method on 29 January 2008, this can be seen in the left picture above, in the middle picture the floor in the clean room and the people in front of the telescope can be seen in reflection in the telescope; see also the Herschel SciTech website. Telescope level M1-M2 distance confirmation measurements were successfully performed on 4-5 February, as can be seen in the right picture; see also the Herschel SciTech website. There is also a Corporate website telescope news story. [January-February 2008]
The Herschel flight telescope has arrived in ESTEC. The Herschel flight telescope has arrived safely in ESTEC by road from Astrium, Friedrichshafen, and was unloaded on 18 January 2008. After acclimatisation and preparation of ground support equipment it was moved out of its transport container on 24 January 2008. [January 2008].
The Herschel flight spacecraft has arrived in ESTEC.
The Herschel flight spacecraft has arrived in ESTEC in the early hours of Saturday 5 January 2008 by road from Astrium, Friedrichshafen. On 7 January 2008 Herschel was removed from its transport container. It currently consists of the (warm) cryostat and service module, with the flight science instruments integrated. After functional testing and bake-out, the cooling down will commence. During cooldown the telescope and sunshade/solar array will be integrated. Additional text and pictures can be found on the Herschel SciTech website [January 2008].
The HIFI FM FPU has joined SPIRE and PACS on the optical bench. After leaving SRON, Groningen on 9 July 2007 and arriving in Astrium, Friedrichshafen the following day, the HIFI FM FPU was integrated onto the Herschel optical bench. By joining the SPIRE and PACS FPUs already there all Herschel science instruments have been integrated. In the pictures above from left to right: HIFI with PACS to the left, HIFI with SPIRE to the right, HIFI under the instrument shield. Images courtesy of Astrium. [July 2007]
PACS FM FPU also mounted on the Herschel optical bench. The PACS flight model (FM) instrument has been delivered from the Max-Planck-Institut für extraterrestrisch Physik (MPE), Garching, to the Astrium premises in Friedrichshafen, Germany. The warm electronics were delivered on 3 July, the focal place unit (FPU) on 6 July, and in the pictures above the FPU can be seen being hoisted and mounted onto the Herschel flight cryostat optical bench next to SPIRE on 9 July 2007. [July 2007]
Herschel Open Time Key Programme proposals now welcome! The Herschel GT KP observations have now been established and the AO package has been updated as appropriate for the OT KP phase. The entire AO documentation with the associated AO tools are now available, as is a GT KP programme description. It is mandatory to use the HerschelFORM PDFLaTeX package provided to produce the scientific justification, and the HSpot observation planning tool to produce AORs and generate the required observing times. Start by reading the AO how-to 'step-by-step webpage. The deadline for proposal submission is 25 October 2007. [July 2007]
SPIRE FM FPU mounted on the Herschel optical bench.
The SPIRE flight model (FM) instrument has been delivered! The SPIRE focal place unit (FPU) and associated warm electronics have been shipped from the Rutherford Appleton Laboratory in Didcot, United Kingdom, to the Astrium premises in Friedrichshafen, Germany. In the pictures above the SPIRE FM FPU can be seen being hoisted and mounted onto the Herschel flight cryostat optical bench. Here SPIRE will soon be joined by the PACS and HIFI FPUs.
[April 2007]
Herschel Open Time Key Programme workshop. The Herschel OT KP workshop was held in ESTEC on 20-21 February 2007. The interest was so massive that due to fire regulations the registration had to be prematurely closed and a waiting list established. In the end about 250 people attended the meeting, some of whom can be seen in the pictures above.
[February 2007]
First Herschel AO released!
The initial Herschel Announcement of Opportunity (AO) for observing proposals was released by the Herschel Science Centre on 1 February 2007. This the first AO concerned guaranteed time (GT) Key Programmes (KPs) only. The deadline for responding to the AO by submitting proposals was 4 April 2007. In total 21 proposals were received.
[February 2007]
2006 - qualification tests
PACS FM instrument first light!
PACS photometer first light was achieved on 15 November 2006 (left picture). This momentous event was witnessed among others by (middle picture, left to right) Marc Sauvage, Koryo Okumura, and Roland Vavrek (standing). The photometer first light video is available
here (avi,
11Mb). The PACS spectrometer first light was achieved only two days
later on 17 November 2006 (right picture). This was a spectrometer
grating scan looking at a 30K optical ground support wquipment black
body source. In the picture 25 simultaneous spectra can be seen
(confirming all 25 modules working!) and in the inset the time
evolution of the signal in a single pixel.
[November 2006]
Herschel FM telescope at Flight Qualification Review
(FQR).
The telescope being inspected in the Astrium, Toulouse facilities as
part of the FQR on 9 November 2006. In left picture from left to right:
Dominic Doyle, Dominique Pierot, Jacqueline Fischer, Göran Pilbratt, Yves
Toulemont, Gerald Crone, Pierre Olivier, and Jean-Luc Varin. In middle
picture M2 and its supporting structure is inspected, in right
picture the 'scatter cone' can be seen.
[November 2006]
Herschel satellite undergoing environmental qualification
The Herschel satellite is undergoing environmental qualification in
the ESTEC Test Centre. Herschel is in STM configuration, but the
cryostat, 6 of 8 side and both top and bottom service module panels,
and the thermal shield between the SVM and cryostat, as well as
the upper half of the sunshade, are all flight hardware.
In the left and middle pictures Herschel is placed on the HYDRA
shaker, while on the right Herschel is on the multi-shaker during a
visit by the Herschel Science Team meeting on 1 Feb 2006.
In the picture from left to right: Thijs de Graauw, Matt Griffin,
Thomas Passvogel (Herschel PM), Matthias von Alberti (EADS Astrium),
Paul Goldsmith (JPL), Göran Pilbratt, Laurent Vigroux, Pierre
Encrenaz, Rüdiger Hohn (EADS Astrium), Christoffel Waelkens,
Martin Harwit, Göran Sandell (SOFIA/Ames), Jacqueline Fischer,
Timo Prusti (HSC), Paul Harvey, Albrecht Poglitsch, Fleming Pedersen
(Herschel AIV), Peter Barthel.
After the mechanical vibration Herschel will undergo acoustic tests,
alignment checks, and shock tests.
[February 2006]
2005 - integration and verification
Merry Christmas and Happy New Year!
The Herschel Science Centre wishes everyone a Merry Christmas and
Happy New Year! On the left the ESTEC people at the boulevard in
Noordwijk on a typical Dutch December day
(left to right: Hassan Siddiqui, Andrew Bonfield, Tilmann Zaeschke,
Nigel Dean, Tim Locke, Jon Brumfitt, Ana Heras, Craig Porrett,
Nicola de Candussio, Göran Pilbratt, Jean-Jacques Mathieu, Timo
Prusti, Rob Zondag, Kevin Galloway, Johannes Riedinger; missing
Stephan Ott), on the right the ESAC people onsite
(left to right: Miguel Sanchez-Portal, Ivan Valtchanov, David
Teyssier, Sarah Leeks, Anthony Marston, Pedro Garcia-Lario, Larry
O'Rourke, Bruno Altieri, Roland Vavrek).
[December 2005]
Spacecraft - STM preparations.
The Herschel satellite under reconfiguration to structural
thermal qualification model (STM) configuration in preparation
for mechanical qualification in Jan 2006.
The mating of the payload module (PLM)
with the service module (SVM) took place on 23 Nov 2005.
More pictures can be found on the Herschel
SciTech website.
The Herschel Ground Segment System Engineers meeting
(left to right: Sunil Sidher, Micha Schmidt, Luis Aloy,
Gottlob Ginger, Kevin Galloway, Gianpero Di Girolamo,
Larry O'Rourke, Ed Chester, Rik Huygens, Pjotr Roelfsema,
and Ana Heras) took the opportunity on 7 Dec 2005, being watched
by the sunshade which at the time was still waiting to be integrated.
Sunshade integration pictures can be found on the Herschel
SciTech website.
[November/December 2005]
EQM campaign - EMC testing.
The EQM campaign has now proceeded to EMC testing.
These pictures were taken in the morning of 18 Nov 2005, just before
commencing the final HIFI conductance susceptibility test. Tony Marston
(middle picture) from the Herschel Science Centre is watching an
intrepid SRON employee working from chair attached to a crane in the
EADS Astrium Ottobrunn facility.
[November 2005]
Spacecraft - PLM TB/TV.
The Herschel flight payload module (PLM) thermal balance/thermal
vacuum ( TB/TV) campaign in the Large Space Simulator (LSS).
In the middle the flight PLM with "thermal interface hardware"
simulating the thermal interfaces with different parts of the
satellite in test configuration inside the LSS in the ESTEC Test Centre.
On the left the test execution is monitored, on the right the EADS
Astrium team.
[October 2005]
Spacecraft - PLM.
The Herschel PLM was moved from its place next to the visitor's
gallery to the Large Space Simulator (LSS) on 19 Sep 2005.
In the pictures from left to right:
The bay next to the visitor's gallery (visible in the background)
had been 'home' for the PLM since its arrival in ESTEC,
now it had to navigate the dark corridors in the Test Centre,
finally to be lifted by a massive crane into the LSS,
where it was finally installed after a journey lasting most of the
day. The PLM assembly will remain in the LSS
for several weeks undergoing preparations
and then the actual thermal balance/thermal vacuum tests.
More pictures can be found on the Herschel
SciTech website.
[September 2005]
Telescope - qualification.
The completed Herschel telescope preparing for its last night
at 'home'. From left to right: Dominique Pierot, Jean-Luc Varin,
Yves Toulemont, Göran Pilbratt, and Dominic Doyle posing
in front of the completed telescope, close-up of the subreflector
assembly, and view of the backside being equipped with accelerators;
EADS Astrium, Toulouse, on 30 August 2005.
The following day the telescope was moved to Intespace, Toulouse, picture on extreme right, for mechanical qualification which was successfully performed in the first half of September. In connection with the qualification activities there was an ESA news story and a EuroNews feature with a video. [September 2005]
EQM facility - IMT campaign.
The integrated module tests (IMT) are now underway. The IMTs are using
the instrument cryogenic qualification model (CQM) focal plane units
(FPUs) integrated in the Herschel engineering qualification model (EQM).
The EQM facility is a "Herschel focal bench simulator" built using
refurbished hardware from the ISO programme, in order to provide an
FPU environment representative of in-orbit conditions.
Left: The FPUs integrated on the focal bench
in early 2005. Centre: The EQM facility in EADS Astrium, Ottobrunn.
Right: The EQM facility tilted for instrument internal cryo-cooler
recycling.
[September 2005]
SPIRE - FM 'first light'.
The SPIRE flight instrument has now achieved first light for both
photometer and spectrometer.
Left: First light on the full SPIRE flight
photometer was achieved on 8 September 2005 during the SPIRE PFM2
campaign with the detectors at a temperature of approx 290 mK.
Centre: The team who did it on the day; from left to right
Asier Aramburu, Sunil Sidher, Tim Waskett, Tanya Lim, and Bruce
Swinyard.
Right: First light for the spectrometer. These interferograms
were obtained already on 8 March 2005 during the PFM1 campaign.
[September 2005]
Telescope - alignment.
The Herschel telescope in the process of undergoing
warm alignment in the facilities of EADS Astrium
in Toulouse. After alignment and measurements under room temperature
conditions, the telescope will undergo warm (it is launched
warm) vibration tests, later to be followed by cryogenic
measurements to verify optical performance under operational
conditions.
[August 2005]
Spacecraft - PLM PFM.
The Herschel payload module (PLM) arrived in ESTEC on 16 August 2005.
The PLM was transported from EADS Astrium in
Friedrichshafen by lorry inside its container which can be seen being
gently lowered to the ground (left),
with the Herschel/Planck Project Team members and EADS Astrium
employes posing in front of it (centre),
and finally the PLM itself can be seen inside the Test Centre (right).
The PLM cryostat itself is flight hardware, currently containing science payload
focal plane unit (FPU) mass and thermal dummies. The PLM will undergo a series
of environmental qualification tests in the months to come.
More pictures can be found on the Herschel
SciTech website.
[August 2005]
Spacecraft - SVM STM.
In May 2005 the Herschel service module (SVM) structural thermal
model (STM) was installed in the Large Space Simulator (LSS) in the
ESTEC Test Centre
for testing which took place in the second half of the month.
In the pictures from left to right the SVM is being mounted in the LSS,
the Herschel Project Scientist Göran Pilbratt and the Planck
Project Scientist Jan Tauber with Isabelle Luthold from the
Herschel/Planck Project Team in front of the LSS chamber, followed by
two views of the SVM in the LSS ready for action.
[May 2005]
Spacecraft - SVM STM.
The first part of the Herschel spacecraft has arrived in ESTEC!
During Herschel Science Team
meeting#22 on 27 April 2005 the meeting
went to see the Herschel service module (SVM) structural thermal
model (STM) in the ESTEC Test Centre where it had arrived just a few days
before. The SVM STM will undergo testing, and will subsequently be
mated with the payload module (PLM) STM for environmental
testing.
In the picture, from left to right: Tom Phillips, Hal Yorke, Pierre
Encrenaz, Paul Harvey, Martin Harwit, Matt Griffin, Göran
Pilbratt, Christoffel Waelkens, Pepe Cernicharo, Albrecht Poglitsch,
Jackie Fischer, Peter Barthel, and Thijs de Graauw.
[April 2005]
Telescope - M1.
The Herschel telescope primary mirror under acceptance in the
facilities of Opteon in Turku, for subsequent transport by air to
EADS Astrium, Toulouse to be prepared for the coating campaign.
In the middle picture from left to right the Opteon team:
Aimo Sillanpää, Timo Lappalainen, Dominique Pierot
(EADS Astrium), Tapio Korhonen, Mikko Pasanen, and Perttu
Keinänen.
[April 2005]
Telescope. The flight primary mirror silicon
carbide (SiC) blank for the Herschel telescope has been successfully
manufactured! It consists of twelve segments which have been brazed
together to form a monolithic blank (view from above
and from below).
This blank will now be ground, polished, and coated to become
the primary mirror for the flight
telescope. The prime contractor for the Herschel telescope is
EADS Astrium SAS, Toulouse, with the SiC work performed by Boostec,
Tarbes. See further here.
[December 2003]
Toledo proceedings. These proceedings are now available
online!
[16 April 2002]
Toledo proceedings. The proceedings titled `The Promise
of the Herschel Space Observatory' from `The Promise of FIRST' symposium held in Toledo 12-15 December 2000 have now been published as ESA SP-460 (ISBN 92-9092-681-3), and are currently being distributed to all participants. The book (550 pages, full colour, price 50 Euro) is also available for purchase from the Spacebooks Online Shop. [3 October 2001]
Telescope. After evaluation of the received proposal,
and followed by successful negotiations, ESA has selected Astrium
SAS of Toulouse, France, to design, manufacture, and deliver the
Herschel telescope. The contract was signed by Astrium on 6 September,
and by ESA on 13 September. The Herschel telescope will be a Cassegrain
design, with a 3.5 m diameter primary mirror and optimised for
low emissivity and straylight. It will be made primarily of silicon
carbide, and must have an overall wavefront error in operations
of no more than 6 micron. [18 September 2001]
Telescope. In its meeting on 11 May 2001 the ESA Industrial
Policy Committee (IPC) gave its approval for ESA to issue an Invitation
To Tender (ITT) for direct negotiations with Astrium Toulouse
for the provision of the Herschel telescope. [May 2001]
Spacecraft. Herschel has now formally entered Phase B.
The contract with the selected prime contractor, Alcatel, was
signed by Alcatel on 27 April 2001, and by ESA on 2 May 2001.
The phase B activities formally started on 2 April 2001, 2 months
ahead of schedule. [May 2001]
AO. An Announcement of Opportunity for a Herschel Optical
Systems Scientist
has been issued on 2 April 2001. [2 April
2001]