In the previous article of this series on leviathans, we looked at how we think black holes have formed. Now, let's look first at how we can find these black holes, and second at how old we think they are.
Dr Ravinder Bhatia, TMT Associate Project Manager, interviews with Annapurni Subramaniam, Professor of Astronomy at the Indian Institute of Astrophysics in Bangalore. She is the Indian project manager for the TMT observatory Software development.
A couple of weeks ago I was in Mumbai, to give a talk on TMT at "Vigyan Samagam—Pushing the Frontiers of Science”. The event was organized by the Indian government, to showcase India’s contributions to large international collaborations in fundamental science and research.
“Wax on, wax off,” said Mr. Miyagi to "The Karate Kid" (1984), to help the kid develop efficiency of movement, attention to detail, and grace—while also polishing Mr. Miyagi’s classic car. What could this possibly have to do with TMT?
As I’ve explained elsewhere in this blog, segment support assemblies are what hold in place each of TMT’s primary mirror segments. They also let each segment be positioned in real time to provide the best possible imaging capability. Staff at the TMT Project Lab in Monrovia, California, are building six segment support assemblies to determine whether the design can be manufactured in a repeatable, problem-free manner.
It’s been some time since my last blog entry because TMT has been keeping me rather busy. I’ll talk about some of the latest happenings in upcoming entries as soon as time permits. However, before letting any more time go by, I’d like to take a moment to highlight TMT’s WFOS system.
As I write this, the final design for TMT’s enclosure—a huge, moveable dome that will house the telescope—is nearing completion. A substantial portion of the final design has already been done, allowing for work to begin on the production readiness phase. The last of the design reviews, for the enclosure’s electrical and controls aspects, is planned for the coming months, with the hope that a contract for the fabrication phase and making all...
One of the highlights for me starting to working on TMT four years ago was my first visit to our laboratory, and the opportunity to see and touch the hardware prototypes for TMT’s mirror support and control systems.
In the Himalayan foothills near Naintal, India, stands the largest single-mirror optical telescope in Asia: India’s new Devasthal Telescope, designed and built under the joint leadership of the Aryabhatta Research Institute of Observational Sciences (ARIES), the Indian Institute for Astrophysics, and the Tata Institute for Fundamental Research.
The Thirty Meter Telescope is being designed and built by an international partnership of institutes and countries representing almost half the world’s total population.