Kepler Team Validates 41 New Exoplanets with Keck

W. M. Keck Observatory press release

The Kepler team today reports on four years of observations from the W. M. Keck Observatory targeting Kepler’s exoplanet systems, announcing results this week at the American Astronomical Society meeting in Washington. These observations, from Keck Observatory on the summit of Mauna Kea, confirm that numerous Kepler discoveries are indeed planets and yield mass measurements of these enigmatic worlds that vary between Earth and Neptune in size.

Kepler Planets
Chart of Kepler planet candidates as of January 2014., credit NASA Ames
More than three-quarters of the planet candidates discovered by NASA’s Kepler spacecraft have sizes ranging from that of Earth to that of Neptune, which is nearly four times as big as Earth. Such planets dominate the galactic census but are not represented in our own solar system. Astronomers don’t know how they form or if they are made of rock, water or gas.

Using one of the two world’s largest telescopes at Keck Observatory in Hawaii, scientists confirmed 41 of the exoplanets discovered by Kepler and determined the masses of 16. With the mass and diameter in-hand, scientists could immediately determine the density of the planets, characterizing them as rocky or gaseous, or mixtures of the two.

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Postcard from the Summit – A Very Cold Day

Getting to and from the vehicles was done as quickly as possible, running from door to door. Not only were the temperatures as low as anyone could remember, the wind was adding to the issue, blowing at a steady 35mph. The temperatures reached -8°C (17°F) at night and never rose above freezing during the day. The ice is slowly sublimating in the dry air, but there is still too much on the domes for safe observing.

Now if the wind would obey the posted speed limit…

A Very Cold Day
The remains of heavy ice sublimating in cold, dry air with steady 35mph winds

Kepler and Keck Provide Insights on Enigmatic Planets

JPL press release

More than three-quarters of the planet candidates discovered by NASA’s Kepler spacecraft have sizes ranging from that of Earth to that of Neptune, which is nearly four times as big as Earth. Such planets dominate the galactic census but are not represented in our own solar system. Astronomers don’t know how they form or if they are made of rock, water or gas.

Kepler
Artist’s rendition of the Kepler Spacecraft in orbit around the Sun peering at a distant solar system, press release image from the NASA Kepler website
The Kepler team today reports on four years of ground-based follow-up observations targeting Kepler’s exoplanet systems at the American Astronomical Society meeting in Washington. These observations confirm the numerous Kepler discoveries are indeed planets and yield mass measurements of these enigmatic worlds that vary between Earth and Neptune in size.

Included in the findings are five new rocky planets ranging in size from 10 to 80 percent larger than Earth. Two of the new rocky worlds, dubbed Kepler-99b and Kepler-406b, are both 40 percent larger in size than Earth and have a density similar to lead. The planets orbit their host stars in less than five and three days respectively, making these worlds too hot for life as we know it.

A major component of these follow-up observations was Doppler measurements of the planets’ host stars. The team measured the reflex wobble of the host star, caused by the gravitational tug on the star exerted by the orbiting planet. That measured wobble reveals the mass of the planet: the higher the mass of the planet, the greater the gravitational tug on the star and hence the greater the wobble.

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Jupiter at Opposition

Jupiter will pass through opposition at 09:49HST today.

Jove
Jupiter and the moons Europa, Ganymede and Callisto (left-right)
Jupiter orbits the Sun once every 11.86 years. As the giant planet continues on its way the Earth swings around much faster on our inside track. As a result we lap Jupiter once every 399 days, passing between the planet and the Sun. During opposition Jupiter will rise at sunset, transit at midnight, and set at dawn. This makes the planet available for observation for the entire night.

Look for a bright object rising in the eastern sky after sunset. It is difficult to mistake for anything else, shining at it’s brightest during opposition, a brilliant -2.7 magnitude. For the remainder of the winter and much of the spring, the planet will be quite prominent in the evening sky.

Juvenile Bigeye Emporer

Sometimes you see a fish that is not familiar, asking yourself “What is that?” After so many dives I probably have seen one before, but have not paid any attention to that particular fish in the swirl of color and fish on the reef.

Then comes the challenge of identifying the photo. A first run through the book provided no answers. A second run, checking any families with similar body plans… Nothing. Great, it is probably juvenile that looks nothing like the adult… The adult photo is in the book. More browsing, this time on the Stender’s website. The website often has multiple photos of the same species, including the color variations that come with differing sex and age.

Yup, a juvenile bigeye emperor, it looks absolutely nothing like the adult

Juvenile Bigeye Emperor
A juvenile bigeye emperor (Monotaxis grandoculis) at 30ft depth, Hoover’s Tower

Rainbow Wheel

As I have mentioned previously, Waimea has rainbows.  Not just a few rainbows either, but multiple rainbows through the day.  Add a few cloud bows, and moon-bows into the schedule and you get the idea of how common rainbows are in this town.  The last couple weeks have been above average, with rainbows even us jaded rainbow viewers have stopped and taken notice of.

I stopped for this rainbow as is looked like a good photo op,  I was just on my way home from work and had plenty of time to play with a camera.  To my surprise I noted that some cloud shadows were cutting the south end of the bow, creating a wheel, something I had never seen before.

Rainbow Wheel
A rainbow and cloud shadows produce a rainbow wheel