This is a recoding of a Keck Observatory Astronomy Talk given by Dr. Günter Hasinger, Astronomer and Director of the University of Hawaii Institute for Astronomy. His talk, ‘Black Holes ad the Fate of the Universe’, was given on November 20, 2012 at the Gates Performing Arts Center at Hawaii Preparatory Academy, part of the W. M. Keck Observatory public lecture series.
It’s a little bit of the story of the Universe from beginning to end,” said Dr. Hasinger. “What role do black holes have on the fate of the universe, what are they, and how we can understand them better?”
A team of astronomers from the University of California, Berkeley and the University of Hawaii at Manoa has found that 17 percent of all sun-like stars have planets one to two times the diameter of Earth in close orbits. The finding, based on an analysis of the first three years of data from NASA’s Kepler mission and the W. W. Keck Observatory on the summit of Mauna Kea, Hawaii, was announced at the American Astronomical Society meeting in Long Beach, California this week.
While other studies had shown that planets around stars are common in our galaxy, until this study, it remained unclear if this is true for Earth-size planets.
The fraction of sun-like stars having planets of different sizes, orbiting within one-fourth of the Earth-sun distance (0.25 AU) of the host star. Image credit: Erik Petigura, Geoff Marcy, Andrew Howard,The team consists of UC Berkeley graduate student Erik Petigura, former UC Berkeley postdoctoral fellow Andrew Howard, now on the faculty of the UH Manoa Institute for Astronomy, and UC Berkeley professor Geoff Marcy.
To find planets, the Kepler space telescope repeatedly images 150,000 stars in a small region of the sky. It looks for a tiny dip in each star’s brightness that indicates a planet is passing in front of it, much like Venus passed between Earth and the sun last summer.
We took a census of the planets detected by the Kepler Space Telescope,” said Howard. “Erik Petigura wrote a new pipeline to detect the shallow dimmings of Earth-size planets in Kepler photometry. With his efficient and well-calibrated pipeline we could confidently report the size distribution of close-in planets down to Earth-size. The result is that Earth-size planets are just a common as planets twice Earth size. Remarkable.”
A very young moon over Waikoloa, this is only 26 hours after new, visible to the unaided eye as a sliver in the fading glow of sunsetNew Moon will occur today at 09:44HST.
The aircraft is rather unremarkable, a standard small jet sitting among many similar aircraft at the Kona airport. It is the NASA colors and the odd pod hanging underneath that belies that this jet is somewhat unusual. This aircraft does not shuttle passengers across the country, it is home to a unique instrument called UAVSAR.
NASA aircraft equipped with UAVSAR podAfter giving the JPL staff a tour of Keck, they reciprocated and offered a tour of their aircraft. An offer that we readily accepted! After three days of watching the jet fly overhead, an opportunity to to see this aircraft up close was not to be wasted.
During this deployment the aircraft has quartered the Big Island, mapping any changes in the landscape on this volcanically active land. The acronym UAVSAR stands for Uninhabited Aerial Vehicle Synthetic Aperture Radar. As the name implies the system is designed to operate from a UAV, but it is currently installed in a crewed Gulfstream III aircraft.
Color-enhanced UAVSAR interferogram images of Hawaii’s Kilauea volcano, image credit: NASA/JPL-CaltechThe system is capable of sub-centimeter accuracy, mapping the surface of our planet with a reconfigurable, polarimetric L-band synthetic aperture radar (SAR). This can reveal precise information about the shape of the land, moisture content of the soil, vegetation differences and more. Making multiple passes of the same area allows study of subtle changes in the terrain due to erosion or volcanic activity. Flying at 12,000 meters (40,000ft) the aircraft must navigate with exceptional accuracy to allow the radar to gather the data. A custom autopilot flies the aircraft through a 33 foot (10 meter) “tube” in the air between two GPS waypoints.
For this mission it is this volcanic island that is the target. As any islander knows we live on a rock that moves. The island settles into the sea, slides into the ocean, and swells where magma pushes its way into the volcano. Each year they return to Hawai’i to re-map the island, this is the fourth year they have returned to check the changes wrought by the volcanoes.
The JPL/NASA folks have completed their mission to the island for the year. Our tour was the morning they were due to depart, flying back to the Dryden Flight Research Center in California.
UAVSAR radar podThe aircraft is not as jammed with electronics as I envisioned. Boarding the plane one finds a few equipment racks and a number of comfortable seats available for the folks that have to tend the electronics through ten hour missions. It is an odd combination of custom electronics built to aerospace standards and off-the-shelf electronics fastened into the racks, including computers, monitors and ethernet routers. Much of the gear is used for simply monitoring the instrument, rather than needed for the radar. One can see how the system could be installed in a smaller UAV.
Hanging underneath the aircraft is the pod containing the radar itself. Bright white, the pod sports a flat antenna down the port side for the sideways looking beam. A trio of scoops on the front ram air through the pod to keep the electronics cool.
We chatted with the flight crew and the radar team learning about the instrument and aircraft. They travel all over the US and sometimes around the globe. They have mapped volcanoes in Alaska and Japan, glaciers in Iceland, measured oil spills, and scanned regions effected by major earthquakes. We noted that they had a fascinating job, while they said the same right back at us.
After the tour our hosts kicked us off the plane and began start-up for their hop back to the mainland. We got the data disks with the GPS data we needed for our tests and traded business cards and contact info. I will have to keep my eye out for the results of this year’s Big Island deployment.
Tomorrow morning will find a razor thin crescent Moon about 5° from a brilliant Venus just above the rising Sun. The Moon will rise about 05:50HST, with Venus already in the sky. With sunrise at 06:59HST the pair should rise about 13° above the sunrise. This is enough to allow the the Moon, only 1.9% illuminated to be spotted fairly easily given a clear eastern horizon.
The W. M. Keck Observatory operates the world’s two largest optical/infrared telescopes located on the summit of Mauna Kea on the Big Island of Hawaii. Both telescopes are equipped with AO systems which are routinely used in both Natural and Laser Guide Star (LGS) AO modes. These systems have been extremely productive scientifically. New, more capable, systems are currently in design and development including the implementation of a new laser, new laser launch telescope, near-infrared tip-tilt sensor and a facility to provide simultaneous AO-corrected point spread function estimates to support science data reduction.
Working on the Keck 1 AO benchThe AO Specialist will be expected to play a lead role in all phases of the development of new AO capabilities from the concept phase through the design and development, commissioning and handover to operations; as well as in the characterization, optimization and improvement of the existing AO systems. The Specialist will also be expected to help guide the development of the Observatory’s high angular resolution capabilities.
The AO Scientist will also participate in improvements to the existing AO facilities including performance optimization and characterization.
Minimum requirements for this position include: Ph.D. level degree in adaptive optics or high angular resolution astronomy or equivalent experience; three years of relevant experience in the development and/or use of AO for astronomical research; two years of work experience in instrumentation development or operations; a broad understanding of the multiple engineering disciplines needed to develop AO systems; and experience in data visualization and analysis. Desirable qualifications include: a proven track record in the development or optimization of AO systems for astronomy; demonstrated leadership skills; optical, mechanical and controls design and engineering expertise; expertise in the development of the high level software needed to operate and optimize AO systems; and previous Observatory experience.
The following skills are required: Excellent written and oral English communication skills, ability to work independently and as part of a team, strong project and time management skills; ability to set priorities and meet deadlines with flexibility.
Kepler’s follow-up observers confirm new discoveries
More than 2,300 exoplanet candidate discoveries have made it the most prolific planet hunter in history. But even NASA’s Kepler mission needs a little help from its friends.
An artist’s illustration of an exoplanet system. Credit: Haven Giguere/YaleEnter the Kepler follow-up observation program, a consortium of astronomers dedicated to getting in-depth with the mission’s findings and verifying them to an extremely high degree of confidence.
A single Kepler observation alone is often not enough to prove that the telescope has found an exoplanet, said Nick Gautier, the mission’s deputy project scientist at NASA’s Jet Propulsion Laboratory, Pasadena, Calif., who coordinated and continues to help run Kepler’s robust follow-up program.
Kepler finds exoplanets by watching for worlds that move directly between the telescope and their host stars. As they do this, they block a tiny fraction of the star’s light, an event astronomers call a “transit.”
