Subscribe free to our newsletters via your
. 24/7 Space News .




EXO WORLDS
Keck Teaming Up With Kepler To Find Other Earths
by Staff Writers
Kamuela HI (SPX) Mar 13, 2009


In the Kepler-Keck duo, once Kepler team members find an Earth candidate and determine as best they can that they're not looking at two stars orbiting each other, they will hand the object off to Marcy and his colleagues. The team will use Keck I telescope and its instrument HIRES, the High Resolution Spectrometer, to monitor how the light coming from the parent star changes as the planet candidate orbits.

For nearly a decade, Cal-Berkeley astronomer Geoff Marcy and his colleagues have been using the W. M. Keck telescopes to discover giant planets orbiting distant stars. Now, with the successful launch of NASA's Kepler mission, they will be using Keck I's ten-meter astronomical eye to discover distant Earths.

Kepler will pick out Earth-like candidates. Keck will then zero in on them and determine, with certainty, if they are at all similar to our home planet.

"Keck and NASA have a long-standing partnership to push astronomy research to its fullest potential. This Keck-Kepler collaboration gives that partnership a compelling new scientific focus," said Taft Armandroff, the Director of Keck Observatory headquartered in Kamuela, HI.

Kepler was launched from NASA's Kennedy Space Center last Friday. Aboard the spacecraft is an 84-megapixel camera that will focus on a single region of the sky and snap repeated images of 100,000 stars looking for those that dim periodically.

By studying the stars' episodic decreases in starlight, astronomers will be able to determine the diameter of the object that passes in front of the star, blocks its light and causes the dimming.

"Kepler does not tell astronomers with certainty if the object taking a bite out of the starlight is a planet or another star.That is where Keck plays a crucial role to the Kepler mission," said Marcy, a frequent Keck user and Kepler mission co-investigator.

He, along with a large international planet-hunting team, has discovered nearly half of the 300-plus known planets outside the Solar System.

Astronomers call the objects Kepler detects transits because from the telescope's perspective the planet candidate seems to eclipse its parent star's light.

The phenomenon is similar to the Moon eclipsing the Sun during a total solar eclipse. But a distant planet eclipsing its parent star will only block a small fraction, 1/10,000, of the star's light. The Moon, by contrast, blocks nearly all of the Sun's light in a total solar eclipse.

In the Kepler-Keck duo, once Kepler team members find an Earth candidate and determine as best they can that they're not looking at two stars orbiting each other, they will hand the object off to Marcy and his colleagues. The team will use Keck I telescope and its instrument HIRES, the High Resolution Spectrometer, to monitor how the light coming from the parent star changes as the planet candidate orbits.

HIRES is an instrument that spreads light collected from the telescope mirrors into its component wavelengths or colors. This is called a spectrum. When the planet candidate orbits around the back of the star, its gravity will ever so slightly pull on the star causing the star's spectrum to shift toward redder wavelengths.

When the planet comes around in its orbit to cross the face of the star, it will pull the star in the other direction, and the star's spectrum will shift toward bluer wavelengths. HIRES will detect these shifts and give astronomers the star's radial velocity, or the speed at which the star moves toward or away from Earth. Based on this speed, Marcy and his team will be able to calculate the mass of planet candidate.

"Keck's HIRES is the only game in town that can measure spectral shifts caused by an Earth-sized planet. No other telescope is big enough," Marcy said. "That is why NASA is really heavily dependent on the Keck telescopes right now."

Calculating the planet candidate's mass is important because it tells astronomers whether a planet or another star is eclipsing the parent star. If the object turns out to be a planet, Marcy and his team can then use the Keck-calculated mass and Kepler-calculated diameter to determine the planet's density.

"In a sense it's as if we are taking the planets and dunking them in a bathtub to see if they float. A rocky planet like Earth would sink," Marcy said. Earth has a density of about five grams per cubic centimeter. Gas giants, on the other hand, have a density close to water at about one gram per cubic centimeter.

"Studying the radial velocity of the planet candidates Kepler discovers is a key endeavor in understanding our place in the cosmos. It will help answer one of humanity 'biggest questions, "Are we alone?" Armandroff said.

Marcy and his colleagues plan to start studying Kepler's candidate Earths with Keck I and HIRES during the last three night of July 2009.

.


Related Links
W. M. Keck Observatory
Lands Beyond Beyond - extra solar planets - news and science
Life Beyond Earth






Comment on this article via your Facebook, Yahoo, AOL, Hotmail login.

Share this article via these popular social media networks
del.icio.usdel.icio.us DiggDigg RedditReddit GoogleGoogle








EXO WORLDS
Starlight, Star Bright
Moffett Field CA (SPX) Mar 13, 2009
"Our holy grail in exoplanet science is to find an Earth twin," says Sara Seager of MIT. An Earth twin would have three crucial characteristics: it would be a rocky planet the same size as Earth; it would orbit a sun-like star; and it would be located in its star's habitable zone, at the same distance from its star that the Earth is from the sun. Such a planet would be a prime candid ... read more


EXO WORLDS
China To Land Probe On Moon At Latest In 2013

Help To Define A Lunar Lander

What Is The Story Behind The Dark Side Of The Moon

Obama's First Budget Backs Core Lunar 2.0 Goals

EXO WORLDS
HiRISE Camera Captures Subtle Colors of Mars' Tiny Moon Deimos

Mars Odyssey Reboots Successfully

Mars, Then and Now: Google Mars Update

Spirit Makes Slight Progress on New Route - sol 1831-1837

EXO WORLDS
North Korea Joins Space Treaty And Convention

Copenhagen Suborbitals Tests Hybrid Atmospheric Transfer Vehicle (HATV)

Where Is The Coldest Point In The Universe

Kazakh Astronaut To Replace Tourist In Russian Spaceship

EXO WORLDS
China Able To Send Man To Moon Around 2020

China To Launch 15 To 16 Satellites In 2009

Macao Donates 14 Million Yuan To Mainland Space Program

Scholarships Established For Aerospace Research

EXO WORLDS
ISS Partners Rule Out Turning Life On Orbiter Into Reality Show

Station Spacewalkers Install Experiments And Probe

US, Russian spacemen take spacewalk: mission control

Space junk sparks crew scare on ISS

EXO WORLDS
45th Space Wing Set To Launch MilComms Satellite

ILS Announces Proton Launch ViaSat-1 Satellite In 2011

45th Space Wing Set To Launch MilComms Satellite

Ariane 5 Ready For Integration Of Dual Space Science Payload

EXO WORLDS
Starlight, Star Bright

Keck Teaming Up With Kepler To Find Other Earths

Kepler Mission Rockets To Space In Search Of Other Earths

Texas Astronomer To Aid Search For Earth-like Planets

EXO WORLDS
SES To Move ASTRA 2C Satellite To 31.5 Degrees East

Radar offer for US missile system still on: Russia

Engineers Crack Ceramics Production Obstacle

SSTL Delivers On Russian KANOPUS Missions




The content herein, unless otherwise known to be public domain, are Copyright 1995-2014 - Space Media Network. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA Portal Reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. Advertising does not imply endorsement,agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. Privacy Statement