Kepler Gets a Little Help From Its Friends

JPL press release

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.

KIC 4862625
An artist’s illustration of an exoplanet system. Credit: Haven Giguere/Yale
Enter 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.”

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Keck Week is Coming

W. M. Keck Observatory press release

This Spring, the W. M. Keck Observatory is throwing a weeklong party called Keck Week 2013, to celebrate the observatory’s first twenty years of high-impact, game-changing astronomical discoveries from the venerable twin-domes on the summit of Mauna Kea, Hawaii. The festivities will take place in several Kohala Coast resort venues as well as in the town of Kamuela and will mark a distinctive confluence of the brightest minds in astronomy alongside our country’s most significant scientific philanthropists. Early registration lasts until December 20th, offering a 30 percent discount off all events.

Keck 1 Laser
The Keck 1 Laser undergoing engineering tests, Subaru telescope in background
“We are very excited and honored to host Keck Week 2013,” said Taft Armandroff, Director of the W. M. Keck Observatory. “We look forward to showcasing the unprecedented discoveries made by our powerful telescopes and our ambitious community of dedicated scientists. With this event, we want to celebrate Keck’s first twenty years of achievements and unveil a vibrant course for our future.”

Keck Week 2013 will open March 14th at The Fairmont Orchid, with the Keck Observatory 20th Anniversary Science Meeting – a rare, two-day binge of astronomy discourse and finely honed presentations describing Keck’s legacy discoveries. On March 16th, Keck Week will peak with a Star Struck Fundraising Gala, a grand evening at the Four Seasons Resort Hualalai and feature a live auction of spectacular items, a gourmet dinner, live music and dancing, and remarks by special guests. Other events planned for Keck Week 2013 include:

  • “Astronomy Live! Tonight” – Enjoy a hosted reception under the stars with Keck’s most popular astronomers, star gazing, a live feed from the summit and much more;
  • “Welcome to Our Universe – Keck Observatory’s Open House” – Explore and discover the science and engineering of the Keck Observatory with exhibits and hands-on activities developed by the professional staff at Keck;
  • Keck Tennis Match – Watch Keck astronomers out-parallax their Friends of Keck competitors on the court;
  • Contact! – A free showing of the feature film on the big screen; and
  • Hawai’i Astronomy – Visit Hawai’i’s other astronomical centers.

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Working the Weather

One of the little side jobs I have gotten assigned at Keck is updating the weather station. This involves replacing all of the weather monitoring equipment that allows the operators to keep an eye on conditions around the telescopes. This gear is absolutely critical, giving the operators the data they need to protect our equipment, including the irreplaceable mirrors.

Keck Weather Mast
The weather mast atop the Keck observatory building
As a side job it has been fun. A simple job that can be completed with a minimum of complications and the usual folderol that surrounds larger engineering projects. Just come up with a plan, put some numbers on the plan, buy the gear and install it. As budget has allowed I have worked my way through the plan, replacing bits of gear one item at a time.

It has been fun to learn about measuring temperature, humidity, dew point and more. It seems so simple at first, but the complications of getting a good reading are subtle. Passive instrument shelters, active ventilation, instrument positioning, calibration and more. Issues that can make a good instrument give bad data.

Barometric Sensor
A barometric sensor installed in the Keck weather mast
Likewise the severity of the weather at the 13,600ft elevation of the observatory is a real challenge. How do you get a good reading in 70mph blowing snow? What do you do about 8 inches of ice that has formed over every vertical surface. That one was a challenge, the first shelter I put up for the temperature and humidity partially collapsed under the weight of the ice on the sensor cables.

Last week I installed a new barometric sensor. This was the last part of the existing weather instrument suite that needed to be replaced. I got lucky, it was a great day on the summit, sunny with just a modest breeze. Just the day to spend a couple hours hanging off the weather mast in a climbing harness rewiring a junction box for the new cables. A few holes to drill, a few bolts, a couple cables… done!

My next item is to install an anemometer. We have not had an operational anemometer in many years and our observing staff has made it abundantly clear that they want an anemometer. Not that this one will be easy, it is a bit of a challenge to get a decent wind reading anywhere near a 100ft diameter dome. This challenge will be a bit more involved, and involve some good engineering fun. Time to learn about measuring wind-speed and how to do it right. Looking forward to the next part of the plan!

Found: One Planet Orbiting Sun-like Star. Only Twelve Light Years Away

W. M. Keck Observatory press release

An international team of astronomers using the W. M. Keck Observatory and other telescopes, has discovered that Tau Ceti, one of the closest and most Sun-like stars, may host five planets – with one in the elusive ‘Goldilocks Zone’.

Tau Ceti
Artists impression of the Tau Ceti System. Credit: J. Pinfield for the RoPACS network
At a distance of twelve light years and visible with the naked eye in the December evening sky, Tau Ceti is the closest single star that has the same spectral classification as our Sun. Its five planets are estimated to have masses between two and six times the mass of the Earth – making it the lowest-mass planetary system yet detected. One of the planets lies in the star’s habitable zone – the so-called Goldilocks Zone with it’s ‘just right’ temperatures for supporting liquid water – and has a mass around five times that of Earth, making it the smallest planet found to be orbiting in the habitable zone of any Sun-like star.

The international team of astronomers, from the UK, Chile, the USA, and Australia, combined more than 6,000 observations from three different instruments, including HIRES on the Keck I telescope. Using new techniques, the team has found a method to detect signals half the size previously thought possible. This greatly improves the sensitivity of searches for small planets and suggests that Tau Ceti is not a lone star but has a planetary system.

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Astronomers Go Infrared to Map Brightest Galaxies in Universe

W. M. Keck Observatory press release

A group of astronomers from the University of Hawaii at Manoa, the U.S. Mainland, Canada, and Europe recently used the twin telescopes of the W. M. Keck Observatory on Mauna Kea, Hawaii, to conduct a census of the brightest, but until now unseen, galaxies in the distant Universe, bringing astronomers one step closer to understanding how galaxies form and evolve.

Looking Back
A 3D projection of almost 300 galaxies in the census in the same part of the sky.
These galaxies glow so brightly at infrared wavelengths that they would outshine our own Milky Way by hundreds, maybe thousands, of times. They are forming stars so quickly that between 100 and 500 new stars are born in each galaxy every year, and have been coined “starbursts” by astronomers.

While it’s not clear what gives these galaxies their intense luminosity, it could be the result of a collision between two spiral-type galaxies, similar to the Milky Way and Andromeda Galaxies. Or they could be in a particularly gas-rich region of space, where galaxies form stars quickly due to constant bombardment from gas and dust.

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Keck Lecture Reminder

Günther Hasinger
University of Hawai’i
Black Holes and the Fate of the Universe

The character and distribution of stellar and supermassive black holes is a fascinating and rapidly changing area of astronomy research. Recently, the W. M. Keck Observatory has confirmed supermassive black holes are in the centers of most nearby galaxies, including our own Milky Way. A tight relationship exists between black hole mass and the properties of their host galaxies. New instrument capabilities, like those planned at Keck, will reveal even more about the nature of black holes and how they play a role in the ongoing evolution of the universe and everything in it.

Keck 2
Looking into the optics of the Keck 2 telescope
Tuesday, November 20, 2012
7:00 PM
Gates Performing Arts Center Auditorium
Hawaii Preparatory Academy
65-1692 Kohala Mtn. Rd., Waimea

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

Lowell Astronomer Prints Roadmap for Planet Hunters

W. M. Keck Observatory press release

Lowell astronomer Evgenya Shkolnik and her collaborators have published a set of directions for searching out exoplanets, using W. M. Keck Observatory spectroscopy.

Their paper, recently published in The Astrophysical Journal, examined new and existing data from stars and brown dwarfs that are less than 300 million years old, as determined from strong X-ray emission readings. In all, the authors identified 144 young targets for exoplanet searches, with 20 very strong candidates, according to Dr. Shkolnik. This candidate list is being searched for planets with Gemini’s NICI Planet-Finding Campaign and the Planets Around Low-Mass Stars survey, led by astronomer Michael Liu and graduate student Brendan Bowler, respectively, both at the Institute for Astronomy, University of Hawai‘i.

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Keck Astronomy Lecture

Günther Hasinger
University of Hawai’i
Black Holes and the Fate of the Universe

The character and distribution of stellar and supermassive black holes is a fascinating and rapidly changing area of astronomy research. Recently, the W. M. Keck Observatory has confirmed supermassive black holes are in the centers of most nearby galaxies, including our own Milky Way. A tight relationship exists between black hole mass and the properties of their host galaxies. New instrument capabilities, like those planned at Keck, will reveal even more about the nature of black holes and how they play a role in the ongoing evolution of the universe and everything in it.

Keck 2
Looking into the optics of the Keck 2 telescope
Tuesday, November 20, 2012
7:00 PM
Gates Performing Arts Center Auditorium
Hawaii Preparatory Academy
65-1692 Kohala Mtn. Rd., Waimea

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