Project
Manager's Corner: Exploring TMT in Chile
Gary
Sanders
I
have written several times in this column about our campaign
to evaluate and select the site for TMT. (Focus
On... Site Testing,
My Summer Vacation in
February, PM Corner, Looking
Up). I have
described visits to Hawaii and to Chile. These articles included
travelogues, meetings with officials, descriptions of scientific
tests of the quality of "seeing", and discussions of
the ceremonial importance to local communities of some of the mountains
contemplated by TMT.
Read
more...
Science
Nugget—Finding Habitable Earth-like Worlds Around
Nearby Stars
Steve
Vogt, UCO/Lick Observatory
Over
200 planets have now been detected around nearby stars by using
meter/second precision radial velocity observations from optical
spectroscopy to sense the tugging of the planet on its host star.
Any star hosting a planet wobbles in velocity, alternately being
pulled first towards and then away from us by the orbiting planet,
in strict Keplerian periodicity. The period and size of that
wobble reveals the unseen planets' mass and as well as the size
and shape of its orbit. The orbit size and brightness and temperature
of the star are then easily combined to yield the equilibrium
temperature of that planet.
Read
more...
Technology
Nugget—Collaboration, Competition, or "Collabortition"?
Mark
Sirota, TMT Telescope Controls Group Leader
Astronomy
is purely an observational science and as a result places high
value on first discovery. Although peer confirmation is essential
to all scientific discoveries; the thrill, recognition, and opportunity
that a new discovery brings inevitably goes to those who are
first. On the other hand astronomy is an academic pursuit placing
great value on collaboration and the sharing of knowledge. So
what is the manifestation of an environment where competition
to be first and collaboration and sharing of knowledge are both
the norm? Maybe we should call it a "collabortition".
Read
more...
Project
News
On
11 May 2007, Dr. Stephen Strom, one of the founding
pioneers in the TMT partnership, retired officially
from AURA/NOAO.
From the beginning of TMT, Steve played several key
roles including acting Observatory Scientist, Science
Advisory Committee (SAC) member for AURA, SAC chairperson
and wise advisor in a broad range of issues. We wish
Steve all the best during his "retirement" and
look forward to hearing from him for many years to
come.
Q & A
with Mark Sirota
Download
Mark Sirota Interview
[12:43 min. 11.6 MB MP3]
Mark
Sirota is the Telescope Controls Group Leader for the TMT project;
he joined the project in March of 2005. Mark has almost 20 years
of ground based astronomy experience; prior to TMT he served
in engineering and senior management positions with the W. M.
Keck observatory and the Magdalena Ridge Observatory Interferometer.
Mark brings a unique perspective to the TMT team having both
project and operations experience.
Mark
was recently interviewed by Warren Skidmore, the TMT Site Testing
Scientist.
Focus
On—Time Allocation
David
Silva, TMT Observatory Scientist
The
Universe is a big place with lots of exciting neighborhoods.
For every night at the TMT, there will be 5 or more
teams who want to explore those neighborhoods. Deciding
which teams get to use TMT is called time allocation
and scheduling.
For
TMT, we expect this process to begin within each of the partner
communities. The amount of time available to each partner will
be roughly proportional to their financial contribution to the
TMT construction and operations budgets. Each community is likely
to have different scientific priorities and models for scientific
exploration. It is possible that one partner may wish to allocate
all their time to one big project, spanning tens or hundreds
of nights. Such a large project may involve the participation
of tens of astronomers. A different partner may decide to award
one night each to many different projects. Each project may involve
a few astronomers or many astronomers. Given these differences,
each partner is likely to have a slightly different process to
request, received, and collect observing proposals – descriptions
of science ideas and desired observations.
Read
more...
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