Kepler finds first earth-size planets beyond our solar system



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Kepler finds first earth-size planets beyond

our solar system

20 December 2011

  

 

  



This chart compares the first Earth-size planets found

around a sun-like star to planets in our own solar

system, Earth and Venus. NASA's Kepler mission

discovered the new found planets, called Kepler-20e and

Kepler-20f. Kepler-20e is slightly smaller than Venus

with a radius .87 times that of Earth. Kepler-20f is a bit

larger than Earth at 1.03 times the radius of Earth.

Venus is very similar in size to Earth, with a radius of .95

times that our planet. Prior to this discovery, the smallest

known planet orbiting a sun-like star was Kepler-10b

with a radius of 1.42 that of Earth, which translates to 2.9

times the volume. Both Kepler-20e and Kepler-20f circle

in close to their star, called Kepler-20, with orbital

periods of 6.1 and 19.6 days, respectively. Astronomers

say the two little planets are rocky like Earth but with

scorching temperatures. There are three other larger,

likely gaseous planets also know to circle the same star,

known as Kepler-20b, Kepler-20c and Kepler-20d.

Image credit: NASA/Ames/JPL-Caltech

(PhysOrg.com) -- NASA's Kepler mission has

discovered the first Earth-size planets orbiting a

sun-like star outside our solar system. The planets,

called Kepler-20e and Kepler-20f, are too close to

their star to be in the so-called habitable zone

where liquid water could exist on a planet's

surface, but they are the smallest exoplanets ever

confirmed around a star like our sun. 

The discovery marks the next important milestone in

the ultimate search for planets like Earth. The 

new


planets

 are thought to be rocky. Kepler-20e is

slightly smaller than Venus, measuring 0.87 times

the radius of Earth. Kepler-20f is slightly larger than

Earth, measuring 1.03 times its radius. Both planets

reside in a five-planet system called Kepler-20,

approximately 1,000 light-years away in the

constellation Lyra. 

Kepler-20e orbits its 

parent star

 every 6.1 days and

Kepler-20f every 19.6 days. These short orbital

periods mean very hot, inhospitable worlds.

Kepler-20f, at 800 degrees Fahrenheit, is similar to

an average day on the 

planet Mercury

. The surface

temperature of Kepler-20e, at more than 1,400

degrees Fahrenheit, would melt glass. 

This artist's animation flies through the Kepler-20

star system, where NASA's Kepler mission

discovered the first Earth-size planets around a star

beyond our own. Animation credit:

NASA/Ames/JPL-Caltech

"The primary goal of the 

Kepler mission

 is to find

Earth-sized planets in the 

habitable zone

," said

Francois Fressin of the Harvard-Smithsonian



Center for Astrophysics in Cambridge, Mass., lead

author of a new study published in the journal

Nature. "This discovery demonstrates for the first

time that Earth-size planets exist around other 

stars

, and that we are able to detect them." 



The Kepler-20 system includes three other planets

that are larger than Earth but smaller than Neptune.

Kepler-20b, the closest planet, Kepler-20c, the third

planet, and Kepler-20d, the fifth planet, orbit their

star every 3.7, 10.9 and 77.6 days. All five planets

have orbits lying roughly within Mercury's orbit in

our solar system. The host star belongs to the

same G-type class as our sun, although it is slightly

smaller and cooler. 

The system has an unexpected arrangement. In

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our solar system, small, rocky worlds orbit close to

the sun and large, gaseous worlds orbit farther out.

In comparison, the planets of Kepler-20 are

organized in alternating size: large, small, large,

small and large. 

  

 

  



Kepler-20e is the smallest planet found to date orbiting a

Sun-like star. It circles its star every 6.1 days at a

distance of 4.7 million miles. At that distance, its

temperature is expected to be about 1,400 degrees F.

This is an artist's rendering. Credit: NASA/JPL-Caltech/T.

Pyle


"The Kepler data are showing us some planetary

systems have arrangements of planets very

different from that seen in our 

solar system

," said

Jack Lissauer, planetary scientist and Kepler



science team member at NASA's Ames Research

Center in Moffett Field, Calif. "The analysis of

Kepler data continue to reveal new insights about

the diversity of planets and planetary systems

within our galaxy." 

Scientists are not certain how the system evolved

but they do not think the planets formed in their

existing locations. They theorize the planets formed

farther from their star and then migrated inward,

likely through interactions with the disk of material

from which they originated. This allowed the worlds

to maintain their regular spacing despite alternating

sizes. 

The Kepler space telescope detects planets and



planet candidates by measuring dips in the

brightness of more than 150,000 stars to search for

planets crossing in front, or transiting, their stars.

The Kepler science team requires at least three

transits to verify a signal as a planet. 

The Kepler science team uses ground-based

telescopes and the Spitzer Space Telescope to

review observations on planet candidates the

spacecraft finds. The star field Kepler observes in

the constellations Cygnus and Lyra can be seen

only from ground-based observatories in spring

through early fall. The data from these other

observations help determine which candidates can

be validated as planets. 

  

 

  



Kepler-20f orbits its star every 19.6 days at a distance of

10.3 million miles. Although its average temperature

could be as high as 800 degrees F, it might have been

able to retain a water atmosphere as it migrated closer to

the star after it formed. This is an artist's rendering.

Credit: NASA/JPL-Caltech/T. Pyle

To validate Kepler-20e and Kepler-20f,

astronomers used a computer program called

Blender, which runs simulations to help rule out

other astrophysical phenomena masquerading as a

planet. 

On Dec. 5 the team announced the discovery of

Kepler-22b in the habitable zone of its parent star.

It is likely to be too large to have a rocky surface.

While Kepler-20e and Kepler-20f are Earth-size,

they are too close to their parent star to have 

liquid

water


 on the surface. 

"In the cosmic game of hide and seek, finding 

                               2 / 3



 

planets


 with just the right size and just the right

temperature seems only a matter of time," said

Natalie Batalha, Kepler deputy science team lead

and professor of astronomy and physics at San

Jose State University. "We are on the edge of our

seats knowing that Kepler's most anticipated

discoveries are still to come." 

  Provided by JPL/NASA

APA citation: Kepler finds first earth-size planets beyond our solar system (2011, December 20)

retrieved 1 January 2018 from 

https://phys.org/news/2011-12-kepler-earth-size-planets-solar.html

This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no

part may be reproduced without the written permission. The content is provided for information purposes only.

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