Employment Opportunity at Keck – Senior Mechanical Engineer

W. M. Keck Position Announcement

The W. M. Keck Observatory seeks a Senior Mechanical Engineer to work under the direction of the TSD Senior Engineer to provide mechanical engineering and project management support, to develop new observatory capabilities and to upgrade existing observatory systems. This position is responsible for design, analysis, specification, and construction of high technology mechanical and opto-mechanical systems for precision telescope operations.

Segment Crane
the segment crane being lowered into place to remove a segment from a primary mirror
Qualifications for this position are:

  • B. S. Mechanical Engineering or equivalent.
  • >8 years of Mechanical Engineering experience, some experience with opto-mechanical devices, 3 years of which are in project/subcontract management and reporting.
  • Track record of precision designs of small and large scale mechanical components.
  • Competence with 3D computer aided design, finite element analysis, design for assembly and maintainability, product life cycle management, and reliability engineering.
  • Engineering process and configuration management experience.
  • Experienced use of modern manufacturing techniques.

To learn more and to apply please go to: http://keckobservatory.iapplicants.com/ViewJob-359943.html

Galaxies: some assembly required

Swinburne Observatory press release

New research using the world’s largest telescope at the Keck Observatory in Hawaii has revealed two distinct populations of star clusters surrounding galaxies that have radically different chemical compositions.

NGC6656
M22 or NGC6656 in Sagittarius, a classic globular cluster
An international team, led by Swinburne astronomers Christopher Usher and Professor Duncan Forbes, has measured the chemical composition of more than 900 star clusters in a dozen galaxies.

“This is ten times the number of star clusters previously examined, allowing us to confirm the existence of two chemically-distinct star clusters,” Mr Usher said.

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Large Binocular Telescope

A friend of mine, Dean Ketelsen is visiting the island with his wonderful wife, Melinda and a few family members. Dean grinds big glass for a living, as in 8.4m telescope mirrors for Steward Observatory. You can read about his various adventures at his personal blog.

Posted below is Dean’s latest time-lapse video of the LBT opening for a night of observing. I suspect he will be posting something similar of Keck in the near future. We toured the telescopes today and he had a chance to setup the camera while the guys swung the ‘scope around a bit.

I have visited the LBT, many years ago before it was completed. Even without the dual 8.4 meter primary mirrors it was an impressive facility.

Mercury at Maximum Elongation

Today Mercury reaches maximum elongation, the furthest point it will reach from the Sun in the sky and the highest it will be above the sunset this apparition. The planet is easily visible as a bright, starlike object about 15° above the setting Sun as the sky grows dark. Over the next couple weeks Mercury will slide back into the sunset, heading for inferior conjunction on November 17th.

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Reminder Keck Lecture Tonight

Keck Astronomy Lecture

Dr. Ben Zuckerman
University of California at Los Angeles
Violent Events in Rocky Planetary Systems: Implications for the fate of technological civilizations

Keck 2
Looking into the optics of the Keck 2 telescope
Thursday, October 25, 2012
7:00 PM
Gates Performing Arts Center Auditorium
Hawaii Preparatory Academy
65-1692 Kohala Mtn. Rd., Waimea

This evening, Dr. Ben Zuckerman of UCLA, will take us on a journey describing Earth’s formation 4.6 billion years ago to its possible demise 4-5 billion years from now. Along the way, we will consider a few tumultuous eras suffered by Earth’s biosphere, including the present. Such eras, from origins to final resting places, can be explored by understanding astronomical studies of other planetary systems. These systems also provide clues for the long-term fate of our technological civilization and the likelihood, or lack thereof, of civilizations beyond our own.

Seating is limited to first come, first served.
Doors Open at 6:30 PM
Free and Open to the Public

Postcard from Hawaii – Alaskan Halibut

One of the dividends of an Alaskan cruise is the fish we brought back. Processed, vacuum packed and frozen while on the boat, the fish was packed into a cooler and checked for the flight back to Hawai’i. It is a bit nerve-wracking, waiting for the cooler to appear on the baggage carousel in Kona. Appear it did, all of the contents still frozen solid as we loaded it into the freezer at home.

Thirty five pounds of coho salmon, halibut and picked dungeness crab. Light on the salmon, I gave much of it to my brother. Heavy on the halibut, on orders from my wife. We did well on crab, I pulled up full traps several times and we picked crab for hours on the back deck as we cruised along. Pick half a crab… eat a leg! It was a tasty way to go.

Last week I noted the market had frozen wild-caught dungeness crab, at $26 a pound. Halibut was a bit more expensive at Costco. Figure there was about $900 worth of seafood in that cooler. We will be eating well…

Pan Seared Halibut
Pan seared halibut in garlic, onion and pepper, over brown rice.

Amateur Astronomers Find Planet in Four-Star System

W. M. Keck Observatory press release

A joint effort of citizen scientists and professional astronomers at W.M. Keck Observatory in Hawaii has led to the first reported case of a Tatooine-like planet orbiting twin suns that in turn is orbited by a second distant pair of stars.

Aided by volunteers using the Planethunters.org website, a Yale-led international team of astronomers using Keck’s 10-meter telescope identified and confirmed discovery of the phenomenon, called a circumbinary planet in a four-star system.

Only six planets are known to orbit two stars, according to researchers, and none of these are orbited by distant stellar companions.

“Circumbinary planets are the extremes of planet formation,” said Meg Schwamb of Yale, lead author of a paper about the system presented Oct. 15 at the annual meeting of the Division for Planetary Sciences of the American Astronomical Society in Reno, Nevada. “The discovery of these systems is forcing us to go back to the drawing board to understand how such planets can assemble and evolve in these dynamically challenging environments.”

KIC 4862625
An artist’s illustration of PH1, a planet discovered by volunteers from the Planet Hunters citizen science project. PH1, shown in the foreground, is a circumbinary planet and orbits two suns. Credit: Haven Giguere/Yale

Dubbed PH1, the planet was first identified by citizen scientists participating in Planet Hunters, a Yale-led program that enlists the public to review astronomical data from NASA’s Kepler spacecraft for signs of planets. It is the project’s first confirmed planet.

The volunteers, Kian Jek of San Francisco and Robert Gagliano of Cottonwood, Arizona, spotted faint dips in light caused by the planet as it passed in front of its parent stars, a common method of finding extrasolar planets. Schwamb, a Yale postdoctoral researcher, led the team of professional astronomers that confirmed the discovery and characterized the planet, following observations from the Keck telescopes on Mauna Kea, Hawaii. PH1 is a gas giant with a radius about 6.2 times that of Earth, making it a bit bigger than Neptune.

“Planet Hunters is a symbiotic project, pairing the discovery power of the people with follow-up by a team of astronomers,” said Debra Fischer, a professor of astronomy at Yale and planet expert who helped launch Planet Hunters in 2010. “This unique system might have been entirely missed if not for the sharp eyes of the public.”

PH1 orbits outside the 20-day orbit of a pair of eclipsing stars that are 1.5 and 0.41 times the mass of the Sun. It revolves around its host stars roughly every 138 days. Beyond the planet’s orbit at about 1000 AU (roughly 1000 times the distance between Earth and the Sun) is a second pair of stars orbiting the planetary system.

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