Kepler Discovers First Earth Sized Planets inside Habitable Zone

by Ken Kremer on February 2, 2011

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Keplers 1200 Planet candidates by size and location
on the Photometer array of 42 CCD elements. Credit: NASA/Wendy Stenzel
As the number of Pale Blue Dots increase, so do the chances for finding life on a Second Earth
Updated with more Videos and photos below

With the startling new finding of dozens of Earth-sized extrasolar planets, NASA’s Kepler planet hunting space telescope has just revolutionized our understanding of Earths place in the Universe and the search for Extraterrestrial Life. And the historic science discovery is based on data collected in just the first few months of operation of the powerful telescope as it scans only a tiny portion of the sky.

The discovery of 1235 new extrasolar planet candidates was announced today (Feb.2) by NASA and Kepler scientists at a media briefing. 68 of these planet candidates are Earth-sized. Another 288 are Super-Earth-size, 662 are Neptune-size and 165 are Jupiter-size. Most of these candidates orbit stars like our sun.

Even more significant is that 54 of the planet candidates are located within the ‘habitable zone’ of their host stars and 5 of those are Earth-sized. Before today we knew of exactly ZERO Earth-sized planets within the habitable zone. Now there are 5.

Finding a ‘Pale Blue Dot’ or ‘Second Earth’ inside a habitable zone that harbors water and environmental conditions that can support life is the ‘Holy Grail’ of science.

Are We Alone ?

“We went from zero to 68 Earth-sized planet candidates and zero to 54 candidates in the habitable zone – a region where liquid water could exist on a planet’s surface. Some candidates could even have moons with liquid water,” said William Borucki of NASA’s Ames Research Center, Moffett Field, Calif.. Borucki is the science principal investigator for NASA’s Kepler mission.

“Five of the planetary candidates are both near Earth-size and orbit in the habitable zone of their parent stars.”

Earth-sized water worlds are the most conducive to the formation and evolution of alien life forms. Water is an essential prerequisite for life as we know it.

“Kepler’s blown the lid off everything we know about extrasolar planets,” said Debra Fischer, professor of Astronomy at Yale University, New Haven, Conn

Kepler's over 1200 planet candidates as of Feb. 1, 2011. Credit: NASA/Wendy Stenzel

Kepler is the first NASA mission capable of finding Earth-size planets in or near the habitable zones around their parent stars. The mission uses the transit method to detect the tell tale signatures of planets. The goal is to determine how common are planets the size of Earth orbiting inside the habitable zone of stars like our sun.

Kepler measures the miniscule decreases in the brightness of stars caused by planets crossing in front of them and blocking the starlight. Imagine calculating the difference in light transmission caused by a flea sitting on a cars headlight.

Follow up observations over a period of several years will be required to confirm these results, the scientists explained. Astronomers expect that over 80% of the candidate planets will be positively confirmed as real planets by utilizing ground based observatories and the Spitzer Space Telescope.

For an Earth-sized planet orbiting a sun-like star inside the habitable zone, transits occur about once per year. Since three transits are required to verify a planets status, it will therefore take about three years to reach a definitive conclusion.

These remarkable new planet discoveries are based on observations from only the first four months of Kepler’s telescopic operations – May 12, 2009 to Sept. 17, 2009. The space based observatory continuously monitors more than 156,000 stars using 42 CCD detectors with a field of view that covers only 1/400 of the sky.

“Kepler is making good progress towards its goals,” said Borucki

“We have found over twelve hundred candidate planets – that’s more than all the people have found so far in history.”

“Imagine if we could look wider. Kepler looks at one 400th of the sky. If we had 400 of these fields of view, we’d see 400 times that number of candidates. We would see 400,000 candidate planets.”

Keplers over 1200 Planet candidates sorted by size

“The fact that we’ve found so many planet candidates in such a tiny fraction of the sky suggests there are countless planets orbiting stars like our sun in our galaxy,” Borucki amplified. “Our results indicate there must be millions of planets orbiting the stars that surround our sun.”

“If we find that Earth’s are common in the habitable zones of stars, very likely that means life is common around these stars.”

“Kepler has shown that planetary systems like our own are common,” said Debra Fischer.

Planets in Keplers Field of View.
Before and after the discovery of over 1200 planet candidates by NASA’s Kepler Space Telescope.

“The search for planets is motivated by the search for life,” Fischer added.

“We have allowed the public to participate though the website,” she added. “And now we have over 16,000 dedicated users. The public is excited to be a part of research and history.”

“Thanks to Kepler for this treasure chest of data!” Fisher concluded.

Kepler is just the first step in finding Earth sized and Earth like planets. “We are building the foundation for future generations of explorers,” said Borucki.

“Future missions will be developed to study the composition of planetary atmospheres to determine if they are compatible with the presence of life. The design for these missions depends on Kepler finding whether Earth-size planets in the habitable zone are common or rare.”

The first planets beyond our solar system were discovered in 1995. Up to today there were just over 500 known extrasolar planets.

Kepler now has 15 confirmed extrasolar planet discoveries and over 1200 possible candidates.

In January 2011, Kepler confirmed the discovery of its first rocky planet, named Kepler-10b. The molten world measures just 1.4 times the size of Earth and is the smallest planet ever discovered outside our solar system.

NASA’s Kepler spacecraft was launched on March 6, 2009 from Launch Complex 17-B atop a Delta II rocket at Cape Canaveral Air Force Station in Florida. See spacecraft and launch photos below

Kepler’s science operations are currently funded for three and one half years of operations until November 2012. The mission’s lifetime – and its goal of discovering multitudes of new planets as small as Earth – can be extended if NASA funding is approved by Congress and the President.

William Borucki – Explains Keplers Discovery of Earth Sized Planets
Science principal investigator for NASA’s Kepler mission, NASA’s Ames Research Center

Video Caption: NASA’s Kepler mission has discovered its first Earth-size planet candidates and its first candidates in the habitable zone, a region where liquid water could exist on a planet’s surface. Five of the potential planets are near Earth-size and orbit in the habitable zone of smaller, cooler stars than our sun.

Kepler also found six confirmed planets orbiting a sun-like star, Kepler-11. This is the largest group of transiting planets orbiting a single star yet discovered outside our solar system. Located approximately 2,000 light years from Earth, Kepler-11 is the most tightly packed planetary system yet discovered. All six of its confirmed planets have orbits smaller than Venus, and five of the six have orbits smaller than Mercury’s.

What is an Earth like planet ? Explantion here

David Charbonneau, an exoplanet researcher at Harvard University, explains what scientists mean when they say “earthlike planet” and “super Earth.” This interview was recorded at NASA’s Goddard Space Flight Center on December 10, 2010, by NASA science writer Daniel Pendick.

Kepler Mission Star Field
An image by Carter Roberts of the Eastbay Astronomical Society in Oakland, CA, showing the Milky Way region of the sky where the Kepler spacecraft/photometer will be pointing. Each rectangle indicates the specific region of the sky covered by each CCD element of the Kepler photometer. There are a total of 42 CCD elements in pairs, each pair comprising a square.
Credit: Carter Roberts / Eastbay Astronomical Society.

Kepler's target region in the Milky Way. Credit: Jon Lomberg

Kepler being prepared in the clean room at Astrotech
prior to launch on March 6, 2009. Credit:

More Kepler photos courtesy of here

Delta 2 rocket streaks to the heavens.
Launch of NASA’s Kepler planet hunting space telescope from Cape Canaveral Air Force Station, FL, Complex 17, on March 6, 2009 at 10:49 p.m. Credit: Ben Cooper

Ben Cooper Featured on Astronomy Picture of the Day (APOD); March 9, 2009

Launch Pad 17 B and a Delta II rocket
from my perch on the 8th floor of Launch Pad 17 A as rocket is encased in launch tower. Credit: Ken Kremer

View of Launch Complex 17 B and cryogenic storage tanks by Ken Kremer

NASA’s Kepler Media Briefing on Feb. 2, 2011


Dr. Ken Kremer is a speaker, scientist, freelance science journalist (Princeton, NJ) and photographer whose articles, space exploration images and Mars mosaics have appeared in magazines, books, websites and calanders including Astronomy Picture of the Day, NBC, BBC,, Spaceflight Now and the covers of Aviation Week & Space Technology, Spaceflight and the Explorers Club magazines. Ken has presented at numerous educational institutions, civic & religious organizations, museums and astronomy clubs. Ken has reported first hand from the Kennedy Space Center, Cape Canaveral and NASA Wallops on over 40 launches including 8 shuttle launches. He lectures on both Human and Robotic spaceflight -

G-Man May 22, 2011 at 8:08 AM

I’ve been involved in the subject of exo-planets since around 1984. I won’t be surprised to discover that there is an ideal “Earth” world out there somewhere. It is bound to happen, let’s face it, it is already becoming obvious that planet formation is a rule, not an exception. Gravity is the universal force of attraction between all matter. Where loose matter exists in sufficient volumes, things are going to happen. Stars are an obvious consequence of massive amounts of matter collapsing under gravitational forces to eventually compress atomic nuclei into thermonuclear chain reactions.

As stars collapse toward primary ignition, as with planets and lesser bodies, things start to rotate. Clouds of debris from which solar systems evolve rotate. Planets condense and orbit the core body that is to become their parent star and eventually orbits are born. The dark body at the center becomes a star. Solar systems are a natural occurrence. Gravity’s nature is to bring “spin” to things that collapse inward.

Who knows, perhaps Robert Jastrow was correct in his book “Red Giants And White Dwarfs” that our solar system is the result of a super nova explosion? It may explain things as to the abundance of heavy metals in our sun and planets. Why wouldn’t that same possible mechanism be at play every where in our universe. I can’t visualize a solar system evolving out of hydrogen and helium. It makes no sense in quantum mechanics.There is apparently a large volume of heavy materials distributed in space and it suggests to me that stellar explosions are the key behind all of it. Those solar systems came about because heavy atoms evolved in the hearts of stars and that final gasp of life as a star detonates is what gave birth to those heavy materials that brought solar systems and “life” into existence.

It’s an evolutionary process………think about it!

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