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Stealth Alien Planet Discovered by New Technique

For the first time, scientists have definitively discovered an “invisible” alien planet by noticing how its gravity affects the orbit of a neighboring world, a new study reports.

NASA’s Kepler space telescope detected both alien planets, which are known as Kepler-19b and Kepler-19c. Kepler spotted 19b as it passed in front of, or transited, its host star. Researchers then inferred the existence of 19c after observing that 19b’s transits periodically came a little later or earlier than expected. The gravity of 19c tugs on 19b, changing its orbit.

The discovery of Kepler-19c marks the first time this method — known as transit timing variation, or TTV — has robustly found an exoplanet, researchers said. But it almost certainly won’t be the last.

“My expectation is that this method will be applied dozens of times, if not more, for other candidates in the Kepler mission,” said study lead author Sarah Ballard, of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass.

Finding Two New Planets

The Kepler spacecraft launched in March 2009. It typically hunts for alien worlds by measuring the telltale dips in a star’s brightness caused when a planet crosses the star’s face from the telescope’s perspective, blocking some of its light.

Kepler has been incredibly successful using this so-called transit method, spotting 1,235 candidate alien planets in its first four months of operation. That’s the way it detected Kepler-19b, a world 650 light-years away from Earth in the constellation Lyra.

jtotheizzoe:

The Carl Sagan-inspired surrealist GIFs of Ignacio Torres, featuring humans as star stuff.

(images by Ignacio Torres, full gallery at The Morning News)

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The Cosmos - Cosmology: The Study of the Universe

Cosmology is the scientific study of the large scale properties of the Universe as a whole. It endeavors to use the scientific method to understand the origin, evolution and ultimate fate of the entire Universe. Like any field of science, cosmology involves the formation of theories or hypotheses about the universe which make specific predictions for phenomena that can be tested with observations. Depending on the outcome of the observations, the theories will need to be abandoned, revised or extended to accommodate the data. The prevailing theory about the origin and evolution of our Universe is the so-called Big Bang theory.

Big Bang Cosmology

The Big Bang Model is a broadly accepted theory for the origin and evolution of our universe. It postulates that 12 to 14 billion years ago, the portion of the universe we can see today was only a few millimeters across. It has since expanded from this hot dense state into the vast and much cooler cosmos we currently inhabit. We can see remnants of this hot dense matter as the now very cold cosmic microwave background radiation which still pervades the universe and is visible to microwave detectors as a uniform glow across the entire sky.

Foundations of The Big Bang Model

The Big Bang Model rests on two theoretical pillars:

General Relativity

The first key idea dates to 1916 when Einstein developed his General Theory of Relativity which he proposed as a new theory of gravity. His theory generalizes Isaac Newton’s original theory of gravity, c. 1680, in that it is supposed to be valid for bodies in motion as well as bodies at rest. Newton’s gravity is only valid for bodies at rest or moving very slowly compared to the speed of light (usually not too restrictive an assumption!). A key concept of General Relativity is that gravity is no longer described by a gravitational “field” but rather it is supposed to be a distortion of space and time itself. Physicist John Wheeler put it well when he said “Matter tells space how to curve, and space tells matter how to move.” Originally, the theory was able to account for peculiarities in the orbit of Mercury and the bending of light by the Sun, both unexplained in Isaac Newton’s theory of gravity. In recent years, the theory has passed a series of rigorous tests.

The Cosmological Principle

After the introduction of General Relativity a number of scientists, including Einstein, tried to apply the new gravitational dynamics to the universe as a whole. At the time this required an assumption about how the matter in the universe was distributed. The simplest assumption to make is that if you viewed the contents of the universe with sufficiently poor vision, it would appear roughly the same everywhere and in every direction. That is, the matter in the universe is homogeneous and isotropic when averaged over very large scales. This is called the Cosmological Principle. This assumption is being tested continuously as we actually observe the distribution of galaxies on ever larger scales. The accompanying picture shows how uniform the distribution of measured galaxies is over a 70° swath of the sky. In addition the cosmic microwave background radiation, the remnant heat from the Big Bang, has a temperature which is highly uniform over the entire sky. This fact strongly supports the notion that the gas which emitted this radiation long ago was very uniformly distributed.

Read the rest of NASA’s .PDF on Cosmology basics here.