The future of CFHT: Some Issues and Comments
The following remarks were prepared in mid-October as a contribution to the
discussion on the future development of OIR astronomy in Canada
that took place on Oct 18 at the DAO.
The fate of CFHT as an on-going facility and as a site cannot be entirely
divorced from a consideration of what comes next in OIR for Canada.
Site redevelopment
This is a very complex issue because, at its essence, it involves matters
related to Hawaiian Sovereignty and control of "ceded lands" (land which
formerly belonged to the Kingdom of Hawaii that passed to the Territory and
then to the State of Hawaii). BC residents, in particular, will be familiar
with the fundamental problem as it is similar to that arising from the
land claims of the non-treaty Indian Nations in BC.
The University of Hawaii (UH) has prepared a new
Master Plan for the summit
of Mauna Kea.
This plan has been submitted to the Board of Regents of the UH and will be
considered for approval
in January. The elements of this plan that pertain to the Astronomy
facilities may be considered to define the maximum extent of permitted
development in the future.
The key elements for our consideration are the following:
- no new site development will be permitted on the summit ridge
- existing sites (like the CFHT, UH 88",
IRTF, UKIRT) will be permitted
to redevelop within certain design guidelines. Basically, the
re-development will be limited to buildings which do not exceed the height
of the current CFHT dome (130 feet). In the Master Plan, CFHT is identified
as a redevelopment site for a 4m-12m+ telescope.
- the area for new telescope development is severely curtailed on the plateau
just below the summit ridge. Sites for two new O/IR Telescopes of moderate
aperture are identified, as is a site for an optical interferometer. ( One
of the contentious issues is how to "count" an interferometer...). There is
also a single site identified for a VLOT of 25m+ aperture.
There are several implications on this plan:
- The value of our site on the summit has been enhanced considerably. It may
already be considered the best site on the ridge. The key-hole shape and
large size of our site are important assets that should be used in the best
possible way.
- Even with the height restriction, it should be possible to
replace CFHT with a "near VLOT" (15m-class) using a non-dome enclosure.
Other "visibility from below" guidelines may be imposed but the fact that
our site is already disturbed obviates much of the environmental concern.
Clever design could minimize the apparent footprint on the summit ridge.
- Taking a long term view, it is virtually certain that the CFHT site will
be redeveloped. Should we give the site up, it may be extremely difficult
to get back on Mauna Kea. (Of course, our Gemini share is an additional
presence on Mauna Kea.)
- We should bear in mind that other countries are interested in establishing
a presence on Mauna Kea.The demand for opportunities to participate
in front-line Astronomy is likely to grow from many countries as
their economic prosperity improves.
- There is no compelling argument that I can see as to why there is only one
site for a VLOT in the Master Plan. The thinking was that only one
such instrument would ever be built in the Northern Hemisphere. It appears
that CELT (the CalTech-UC Extremely Large Telescope) is close to
being funded and that work on a segmented-mirror design of
30m aperture is proceeding, along with a well funded adaptive-optics
initiative, at Lick.
Using the Keck operation as a guide, it is very unlikely that
such a facility would be "open".
The site for CELT remains open as far as I know and Chile is certainly
being considered. On the other hand, the Keck facility on Hawaii could
easily be expanded to accommodate a new facility from the existing
partnership. Should CELT occupy the VLOT site in the MK Master Plan,
it would preclude the development of another similar facility,
unless the Plan were amended. In the present political climate,
one should not count on that happening.
The implication here is that we know that a Mauna Kea facility can be
serviced on a daily basis (if necessary), whereas a facility on
the Alto Plano should probably be designed for unattended operations
over extended time periods. This
could be a significant cost driver and design constraint.
CFHT configuration
- the current scenario for CFHT envisions operations centered
around "Wide Field Imaging", with MegaCam as the primary instrument,
up to about about 2006-7; perhaps
longer depending on the science drivers for optical
imaging and whether we can implement a wide-field IR (JHK)
imaging capability (WIRCAM and so on).
- Successful deployment of the NGST (2008?) will mark a
watershed for ground-based
astronomy and quickly force a resolution of the roles to be played by all
current facilities. The role of a 4m on a site as precious as ours
is certain to be questioned as that era dawns.
- Advantages of moving CFHT more aggressively toward a WF-IR capability
include the fact
that there is still considerable room for the development of
IR arrays and mosaic-cameras. Hence the deployment of WF-IR Imagers
could prolong the useful scientific life of CFHT (cf. the UK
VISTA project). In addition, the IR Imagers can be operated in
both bright
and dark time (MegaCam is fundamentally a dark-time instrument
although some thought is being directed toward possible bright time use).
- A scenario for CFHT-operations beyond about 2006 is very difficult to
develop for the above reasons. With a truly wide-field IR camera,
the scientific life of CFHT as an independent, front-line research
facility could be extended beyond the end of the next decade.
- The "natural" image quality delivered by CFHT could be
improved by refiguring the primary mirror and also by
improving air-flow through our dome.
The mirror improvements would likely require an extended
shut-down (1 year or so) whereas the dome ventilation could be
done over time with completion during a
"normal" maintenance shutdown. Hence the mirror refiguring project should be
considered only if the scientific life of CFHT were to be extended
beyond 2009.
Other operational Issues
- Canada has a significant interest in three Mauna Kea facilities,
all of which are operated independently. There are irreducible costs
associated with running
large facilities on an off-shore site and we are paying
thrice for services that need not be triplicated. Some rationalization
is needed: new facilities should involve existing institutions
and partnerships as far as possible.
- There are two other 4m-class and a 2m-class telescope on the MK summit ridge
that face similar (but by no means identical) operational and redevelopment
issues as the CFHT. The IRTF is operated by the IFA (UH) under contract with
NASA and is being considered for an upgrade to a novel
6.5m aperture facility. UKIRT is operated by the JAC for
PPARC and is moving toward a
"wide-field" capability. The UH 2.2m is operated by the IFA and
functions as an in-house facility for the UH Astronomy faculty and students.
At some level, the fate of these telescopes also affects the
fate of CFHT. I will continue to explore the possibilities for
co-operation among these facilities.
- GEMINI has expressed an interest in ensuring the most effective deployment
of partner 4m facilities to support Gemini-based science.
So far, no concrete action has developed from this and it is
unclear what the implications for CFHT might be. (France is not a
Gemini partner.) It may well be in Canada's
interest to consider how closer operational and scientific ties
between CFHT and Gemini might be realized. This could be considered
within the context of a VLOT-project carried out under the aegis of
Gemini (or a Gemini derivative).
- As far as I know, the French position on CFHT remains that defined at their
prospective meeting in Arcachon last year. Basically, this envisioned
operating CFHT with MegaCam to the year 2007. Beyond that era,
they wished to
await the recommendations of the New Generation CFHT (NGC) committee.
I am unaware of any further activities flowing from the NGC report
that may be related to a VLOT.
- My understanding is that the French community (and funding agency) remains
interested in keeping a French presence on Mauna Kea. The financial level of
commitment would be similar to that in CFHT. Arcachon does envision
a replacement facility on the CFHT site in the 2010 era.
Community Access Issues
Community access is an issue that always bubbles in
the background when new, expensive facilities are being
contemplated. I am conscious of it because in my musings
on the need to maintain a "front-line" capability in
"competitive" areas of our science, there is often a
counter-argument: the CFHT is the only 4m that Canada funds
and therefore it should serve a broad spectrum of Canadian
interests. A similar argument comes from some quarters of
the French community. There are two elements to this:
- the need to offer a reasonably broad range of
instruments for bright and dark time use,
- the availability of nights to service those who work
in areas of Astronomy which are not the "science
drivers" for expensive new facilities.
Astronomy follows very much a band-wagon style of activity
which can be rationalized fairly easily and is not so
different from other sciences in that way.
What does distinguish much of Astronomy is the reliance on
common facilities - it would seem strange indeed
if all the biochemists in Canada were to use only
four labs, for example.
We get away with this because our Observatories
typically have many instruments and they change reasonably
regularly. We also have some range in Observatory
capabilities.
Hence a concern is that as we evolve along a path toward
ever larger, more complex and expensive instrumentation,
we risk losing the diversity that now exists - both in
terms of the type of science that is done and the people
who are involved. A miniscule share of a VLOT may involve
a large team but that is unlikely to have anything
approaching the diversity we now have within our community.
Our subject is evolving toward the particle physics model
and I believe some care is needed to avoid the unattractive
elements that are present in that model.
Maybe all I'm saying is that the number of nights
does matter.