Monday, December 31, 2012


Amazing People Compilation - Amazing skill and Talent in HD 2012



Compilation of some amazing people and their talents and skills!






Sunday, December 30, 2012


What is a Higgs Boson?



Fermilab scientist Don Lincoln describes the nature of the Higgs boson. Several large experimental groups are hot on the trail of this elusive subatomic particle which is thought to explain the origins of particle mass


The Origin of Mass





The mass is supposed to be the cause of the interaction of any particle with the Higgs Field, the field produced by the Higgs Bosons. This phenomenon by which the particle acquire mass by interacting with the Higgs Field id known as the Higgs Mechanism.

The Universe - Created Out Of Nothing?




Want to know why we don't have to worry about our sun burning out? It's because long before that happens, the sun will expand so enormously that Earth will be cooked to a cinder. Take a tour through the solar system, learn about the event horizon of black holes and when our galaxy began. 

1. Faster Than The Speed Of Light (1/2): The Universe - Created Out Of Nothing?
http://www.youtube.com/watch?v=fxNbXjBbzEo&fmt=18
2. Faster Than The Speed Of Light (2/2): The Expanding Universe
http://www.youtube.com/watch?v=MoTNGmlOO2g&fmt=18

EINSTEIN'S RELATIVITY:

Everything in the universe is traveling through space-time at the speed of light - the maximum speed possible. If you are sitting still in space, then you are traveling through time at the maximum speed. But if you begin traveling through space, then your progress through time slows down. Time Dilation and other relativistic phenomena await you in this interesting series, so hurry up and slow down!

1. Basics And Impact In Our Everyday Life
http://www.youtube.com/watch?v=j72bPmXsyvk&fmt=18
2. Time Dilation - Slowing Down Clocks
http://www.youtube.com/watch?v=HHRK6ojWdtU&fmt=18
3. The Famous Equation E=mc2
http://www.youtube.com/watch?v=7h7tyQlpda4&fmt=18
4. Gravity And Acceleration
http://www.youtube.com/watch?v=LHPqhTY6dh0&fmt=18
5. Black Holes, Event Horizon & Gravitational Waves
http://www.youtube.com/watch?v=iA53l7AG7Pg&fmt=18

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The Cassiopeia Project - making science simple!

The Cassiopeia Project is an effort to make high quality science videos available to everyone. If you can visualize it, then understanding is not far behind.

Cosmic Journeys The Riddle of AntiMatter



In high-res 1080p. Explores one of the deepest mysteries about the origin of our universe. According to standard theory, the early moments of the universe were marked by the explosive contact between subatomic particles of opposite charge. Featuring short interviews with Masaki Hori, Tokyo University and Jeffrey Hangst, Aarhus University.

Scientists are now focusing their most powerful technologies on an effort to figure out exactly what happened. Our understanding of cosmic history hangs on the question: how did matter as we know it survive? And what happened to its birth twin, its opposite, a mysterious substance known as antimatter? 

A crew of astronauts is making its way to a launch pad at the Kennedy Space Center in Florida. Little noticed in the publicity surrounding the close of this storied program is the cargo bolted into Endeavor's hold. It's a science instrument that some hope will become one of the most important scientific contributions of human space flight.

It's a kind of telescope, though it will not return dazzling images of cosmic realms long hidden from view, the distant corners of the universe, or the hidden structure of black holes and exploding stars.

Unlike the great observatories that were launched aboard the shuttle, it was not named for a famous astronomer, like Hubble, or the Chandra X-ray observatory.

The instrument, called the Alpha Magnetic Spectrometer, or AMS. The promise surrounding this device is that it will enable scientists to look at the universe in a completely new way. 

Most telescopes are designed to capture photons, so-called neutral particles reflected or emitted by objects such as stars or galaxies. AMS will capture something different: exotic particles and atoms that are endowed with an electrical charge. The instrument is tuned to capture "cosmic rays" at high energy hurled out by supernova explosions or the turbulent regions surrounding black holes. And there are high hopes that it will capture particles of antimatter from a very early time that remains shrouded in mystery.

The chain of events that gave rise to the universe is described by what's known as the Standard model. It's a theory in the scientific sense, in that it combines a body of observations, experimental evidence, and mathematical models into a consistent overall picture. But this picture is not necessarily complete.

The universe began hot. After about a billionth of a second, it had cooled down enough for fundamental particles to emerge in pairs of opposite charge, known as quarks and antiquarks. After that came leptons and antileptons, such as electrons and positrons. These pairs began annihilating each other.

Most quark pairs were gone by the time the universe was a second old, with most leptons gone a few seconds later. When the dust settled, so to speak, a tiny amount of matter, about one particle in a billion, managed to survive the mass annihilation. 

That tiny amount went on to form the universe we can know - all the light emitting gas, dust, stars, galaxies, and planets. To be sure, antimatter does exist in our universe today. The Fermi Gamma Ray Space Telescope spotted a giant plume of antimatter extending out from the center of our galaxy, most likely created by the acceleration of particles around a supermassive black hole. 

The same telescope picked up signs of antimatter created by lightning strikes in giant thunderstorms in Earth's atmosphere. Scientists have long known how to create antimatter artificially in physics labs - in the superhot environments created by crashing atoms together at nearly the speed of light.

Here is one of the biggest and most enduring mysteries in science: why do we live in a matter-dominated universe? What process caused matter to survive and antimatter to all but disappear? One possibility: that large amounts of antimatter have survived down the eons alongside matter.

In 1928, a young physicist, Paul Dirac, wrote equations that predicted the existence of antimatter. Dirac showed that every type of particle has a twin, exactly identical but of opposite charge. As Dirac saw it, the electron and the positron are mirror images of each other. With all the same properties, they would behave in exactly the same way whether in realms of matter or antimatter. It became clear, though, that ours is a matter universe. The Apollo astronauts went to the moon and back, never once getting annihilated. Solar cosmic rays proved to be matter, not antimatter.

It stands to reason that when the universe was more tightly packed, that it would have experienced an "annihilation catastrophe" that cleared the universe of large chunks of the stuff. Unless antimatter somehow became separated from its twin at birth and exists beyond our field of view, scientists are left to wonder: why do we live in a matter-dominated universe?

Area.51.America's.Book.Of.Secrets.



Saturday, December 29, 2012


Universe 2013 Journey Through the Milky Way 



2012 Awakening "Change is on the Horizon" - COMPLETE



Change is on the Horizon is the epic story of how the world lost its soul and how it will gain it back. Directed and narrated by James Rink.

Part 1 Dawn of the Golden Age - Discuses how Saint Germain helped bring about the beginnings of a enlightened era which soon fell into darkness under the helms of the Illuminati and a corrupted masonic order.


Part 2 - The American Federal Empire. America was always meant to be always a shinning beacon of freedom and prosperity to the world. But the machinations of British bankers and the Rothschild's soon destroyed all that was once good in this great land.


Part 3 - The Farmer Claim Program - Discuses how a class action lawsuit brought about in the early 1990's lead to the creation of NESARA, the National Economic Security and Reformation Act which will ultimately tear apart the New World Order and bankers plans right out from under their feet.


Japan Launching Ambitious Asteroid-Sampling Mission in 2014

Artist's concept of Japan's proposed Hayabusa 2 spacecraft, which would grab samples off the asteroid 1999 JU3 .




Artist's concept of Japan’s proposed 
Hayabusa 2 spacecraft, which would 
reconnoiter asteroid 1999 JU3 in mid-2018. Hayabusa 2 would hurl an impactor into
 the asteroid, sample the resulting crater
 and send pieces back to Earth for study.
CREDIT: JAXA/Akihiro Ikeshita




Japan's space agency is readying a new asteroid probe for launch, an ambitious mission that aims to build on the victory of the country's first round-trip asteroid mission that sent the Hayabusa spacecraft to retrieve samples of the space rock Itokowa.
The new Japanese asteroid mission, called Hayabusa2, is scheduled for launch in 2014 and aimed at the asteroid 1999 JU3, a large space rock about 3,018 feet (920 meters) in length. It is due to arrive at the asteroid in mid-2018, loiter at the space rock and carry out a slew of challenging firsts before departing the scene at the end of 2019.
If all goes well, the Hayabusa2 spacecraft will return to Earth with samples of asteroid 1999 JU3 at the end of 2020. The probe's name is Japanese for "Falcon2.
Building on success
Officials with the Japanese Aerospace Exploration Agency (JAXA) said Hayabusa2, like its Hayabusa predecessor, will also involve a significant level of international cooperation. 
The initial Hayabusa mission launched in May 2003 and returned samples of Itokawa — the first asteroid samples ever collected in space — in June 2010. [Japan Returns 1st Asteroid Samples to Earth (Photos)]
Japan unveils the Hayabusa2 asteroid probe on Dec. 26, 2012, during an event at JAXA's  Sagamihara Campus. The spacecraft will launch in 2014 to collect samples of the asteroid 1999 JU3.
Japan unveils the Hayabusa2 asteroid probe on Dec. 26, 2012, during an event at JAXA's Sagamihara Campus. The spacecraft will launch in 2014 to collect samples of the asteroid 1999 JU3.
CREDIT: JAXA
Like that first flight, the Hayabusa2 mission will rely on NASA’s Deep Space Network of ground stations to help track the spacecraft. The spacecraft's return capsule will also land in Australia, another similarity to the first flight.
Hayabusa2 is expected to stay with asteroid 1999 JU3 for more than a year, 18 months in all, thereby allowing ample time for observation and careful sample collection, according to the mission's project manager Makoto Yoshikawa of Japan's the Institute of Space and Astronautical Science (ISAS).
Asteroid 1999 JU3 is of particular interest to researchers because it consists of 4.5-billion-year-old material that has been altered very little. Measurements taken from Earth suggest that the asteroid’s rock may have come into contact with water.
The C-type asteroid is expected to contain organic and hydrated minerals, making it different from Itokawa, which was a rocky S-type asteroid. Asteroid 1999 JU3 is also larger than Itokawa, which was 1,771 (540 m) long.
An artist's illustration of Japan's Hayabusa2 probe crashing an impactor into the asteroid 1999 JU3 ahead of sampling the space rock in 2018.
CREDIT: JAXA/Akihiro Ikeshita
New and novel hardware
While the configuration of Hayabusa2 is similar to that of the first Hayabusa, the second probe will carry new and novel asteroid-studying hardware.
For example, the antenna for Hayabusa was a single parabolic dish, but Hayabusa2 will sport two flat high-gain antennas to support faster communication speeds than its predecessor. Also, Hayabusa2 is to will fly through space with more propulsion power from its ion engines. [How Japan's 1st Asteroid Probe Worked (Infographic)]
Another addition is a 4-pound (2 kilograms) "collision device" that will be used to create an artificial crater on asteroid 1999 JU3 during the mission. This human-caused dent is expected to be a small one, a few meters in diameter. But it will allow Hayabusa2 to acquire samples of the asteroid that are exposed by the smashing event, fresh specimens that are less weathered by the brutal space environment on the asteroid's surface.
Yoshikawa noted that during the first Hayabusa mission, the probe's MIcro/Nano Experimental Robot Vehicle for Asteroid (MINERVA) failed to reach the surface of Itokawa. "So for Hayabusa2 we have even greater motivation to succeed with our new version of the robot, MINERVA2."
German MASCOT lander to ride Japan's Hayabusa2 spacecraft to the asteroid 1999 JU3.
Integration of Germany’s Mobile Asteroid Surface Scout (MASCOT) asteroid lander, being readied to fly on Japan’s Hayabusa2 mission. To land on the asteroid 1999 JU3 in 2018.
CREDIT: German Aerospace Center (DLR)

Hayabusa2's MASCOT hitchhiker
For its part, the German Aerospace Center’s (DLR) Institute of Space Systems in Bremen is contributing the Mobile Asteroid Surface Scout asteroid lander, or Mascot, to the JAXA mission. Mascot is being developed by DLR in collaboration with the French space agency and JAXA.
After Hayabusa2 arrives at asteroid 1999 JU3 in 2018, Mascot will be released from the main spacecraft. A spring-loaded mechanism will push the 22-pound (10 kilograms) lander clear of from Hayabusa2.
Mascot is a "hopping" lander packed with four separate instruments and is designed to move across thesurface of an asteroid. Doing so will enable it to take measurements at different sites. As Mascot performs the near-asteroid maneuvers, a radiometer will measure the temperature of the asteroid and a camera will image the fine structure of the surface of 1999 JU3.
The lander will be controlled from DLR's Microgravity User Support Center in Cologne.
Free-falling on an asteroid
"Mascot will free-fall to the asteroid from an altitude of around 100 meters [328 feet]," said Tra-Mi Ho, DLR's project leader for the device, in a statement. Sensors will then ensure that Mascot knows which way is up and down, so it can orient itself and, if necessary, correct its attitude.
Once on the asteroid, Mascot is expected to automatically adjust itself and "hop" from one measurement site to the next.
"Mascot is due to take measurements of the regolith itself, which will provide reference data about the surface and enable the samples subsequently brought back by Hayabusa2 to be interpreted in the correct context," said Ralf Jaumann, a DLR planetary researcher and scientific spokesman for the experiments on the lander.
Mascot will work on the asteroid for a total of 16 hours, the equivalent of two days on asteroid 1999 JU3.
Named 25143 Itokawa, this asteroid is some 540 meters by 270 meters by 210 meters. Japan's robotic Hayabusa spacecraft rendezvoused with asteroid Itokawa in mid-September 2005 and studied the space rock's shape, spin, topography, color, composition, densi
CREDIT: JAXA
Up close with an asteroid
"We anticipate obtaining close-up photographs of the asteroid surface up to the order of centimeter-level resolution, something that Hayabusa1 was unable to capture,” said Masanao Abe, Hayabusa2 project scientist at ISAS.
The experience gained from that first Hayabusa mission, in terms of asteroid sample collection and analysis technologies, is proving highly useful, Abe said.
"Japan is at the forefront of sample-return technology and execution," Abe added "and we are constantly thinking about how we can maintain our position and steadily working on things that will keep us at the leading edge."
Asteroid Basics: A Space Rock Quiz
Asteroids are fascinating for lots of reasons. They contain a variety of valuable resources and slam into our planet on a regular basis, occasionally snuffing out most of Earth's lifeforms. How much do you know about space rocks?
Start the Quiz
Earth Causes Asteroid-Quakes
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New discoveries ahead
Akio Fujimura, an advisor in JAXA's Lunar and Planetary Exploration Program Group, said that in Hayabusa2's snagging of carbonaceous asteroid material, there is a high probability of gaining samples that contain organic matter — the fundamental building blocks of life.
"So, first, I expect Hayabusa2 to be a success. Then after that, I'd like us to proceed with an inquiry concerning where we came from and how life came about," Fujimura said. "It would be great to uncover the origins of the solar system, Earth, the other planets, and life itself by getting information that we can't obtain here on Earth. I'd like us to open up new lines of scientific inquiry that seek to discover these origins."
JAXA and the ISAS has learned a great deal from the first Hayabusa mission, said Michael Zolensky, a Hayabusa team member in sample analysis at the NASA Johnson Space Center in Houston, Texas.
"Although the second spacecraft is based on the first one, they have made significant upgrades and expanded the capabilities of the spacecraft for Hayabusa2," Zolensky told SPACE.com. "It should be a fantastic mission. No fooling."
Leonard David has been reporting on the space industry for more than five decades. He is the 2011 winner of the National Space Club Press Award and a past editor-in-chief of the National Space Society's Ad Astra and Space World magazines. He has written for SPACE.com since 1999.

The 500 Phases of Matter: New System Successfully Classifies Symmetry-Protected Phases



Dec. 21, 2012 — Forget solid, liquid, and gas: there are in fact more than 500 phases of matter. In a major paper in a recent issue of Science, Perimeter Faculty member Xiao-Gang Wen reveals a modern reclassification of all of them.


Condensed matter physics -- the branch of physics responsible for discovering and describing most of these phases -- has traditionally classified phases by the way their fundamental building blocks -- usually atoms -- are arranged. The key is something called symmetry.
To understand symmetry, imagine flying through liquid water in an impossibly tiny ship: the atoms would swirl randomly around you and every direction -- whether up, down, or sideways -- would be the same. The technical term for this is "symmetry" -- and liquids are highly symmetric. Crystal ice, another phase of water, is less symmetric. If you flew through ice in the same way, you would see the straight rows of crystalline structures passing as regularly as the girders of an unfinished skyscraper. Certain angles would give you different views. Certain paths would be blocked, others wide open. Ice has many symmetries -- every "floor" and every "room" would look the same, for instance -- but physicists would say that the high symmetry of liquid water is broken.
Classifying the phases of matter by describing their symmetries and where and how those symmetries break is known as the Landau paradigm. More than simply a way of arranging the phases of matter into a chart, Landau's theory is a powerful tool which both guides scientists in discovering new phases of matter and helps them grapple with the behaviours of the known phases. Physicists were so pleased with Landau's theory that for a long time they believed that all phases of matter could be described by symmetries. That's why it was such an eye-opening experience when they discovered a handful of phases that Landau couldn't describe.
Beginning in the 1980s, condensed matter researchers, including Xiao-Gang Wen -- now a faculty member at Perimeter Institute -- investigated new quantum systems where numerous ground states existed with the same symmetry. Wen pointed out that those new states contain a new kind of order: topological order. Topological order is a quantum mechanical phenomenon: it is not related to the symmetry of the ground state, but instead to the global properties of the ground state's wave function. Therefore, it transcends the Landau paradigm, which is based on classical physics concepts.
Topological order is a more general understanding of quantum phases and the transitions between them. In the new framework, the phases of matter were described not by the patterns of symmetry in the ground state, but by the patterns of a decidedly quantum property -- entanglement. When two particles are entangled, certain measurements performed on one of them immediately affect the other, no matter how far apart the particles are. The patterns of such quantum effects, unlike the patterns of the atomic positions, could not be described by their symmetries. If you were to describe a city as a topologically ordered state from the cockpit of your impossibly tiny ship, you'd no longer be describing the girders and buildings of the crystals you passed, but rather invisible connections between them -- rather like describing a city based on the information flow in its telephone system.
This more general description of matter developed by Wen and collaborators was powerful -- but there were still a few phases that didn't fit. Specifically, there were a set of short-range entangled phases that did not break the symmetry, the so-called symmetry-protected topological phases. Examples of symmetry-protected phases include some topological superconductors and topological insulators, which are of widespread immediate interest because they show promise for use in the coming first generation of quantum electronics.
In the paper featured in Science, Wen and collaborators reveal a new system which can, at last, successfully classify these symmetry-protected phases.
Using modern mathematics -- specifically group cohomology theory and group super-cohomology theory -- the researchers have constructed and classified the symmetry-protected phases in any number of dimensions and for any symmetries. Their new classification system will provide insight about these quantum phases of matter, which may in turn increase our ability to design states of matter for use in superconductors or quantum computers.
This paper is a revealing look at the intricate and fascinating world of quantum entanglement, and an important step toward a modern reclassification of all phases of matter.

Friday, December 28, 2012


Decoding The Past - The Other Nostradamus





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Could the future already be written? This mammoth series spans human experience to illuminate this question. Common wisdom has it we prepare for our future by understanding our past. But did the ancient prophets already know the future? Are we living in the world they predicted? In this enlightening and often unsettling series, the viewer revisits the prophecies and divinations of the Ancients and traces them to the modern events they may have been predicting. Beyond great leaders and pivotal battles, our history contains a trove of information and insight, tradition and warning. From the Tibetan Book of the Dead to a 20th Century Nostradamus, from the secrets of the Templars to the real fiend behind the Frankenstein story, these programs address some of these persistent curiosities from the Ages.

National Geographic: Hubbles Amazing Universe



National Geographic: Hubbles Amazing Universe

Responsible for unlocking many mysteries of the final frontier, the most renowned telescope in the world is in danger of being lost forever. The Hubble Space Telescope has explored the creation of stars and planets, the glory of supernovas and the formation of super massive black holes, charted dark matter and changed forever our understanding of reality itself. Now, it's spiraling toward the Earth, and astronauts are embarking on a dangerous mission to fix it.

In Hubble's Amazing Universe, glimpse the far ends of the universe as seen through the amazing Hubble Space Telescope, and meet one of the astronauts risking everything to save it

Thursday, December 27, 2012


The Universe - Strangest Things In The Universe (Full Documentary)





Johannes Kepler Biography




When Johannes Kepler was born in the late sixteenth century, scientists believed that planets in the solar system traveled in circular orbits around the Earth. The occasional problem was solved by the addition of miniature circles test — epicycles — to planetary paths. But Kepler not only adamantly defended the idea that planets orbit the sun, he also revealed that their paths were not perfect circles. His descriptions of planetary motions became known as Kepler’s laws. [See also our overview of Famous Astronomers and great scientists from many fields who have contributed to the rich history of discoveries in astronomy.]
Here is a brief biography of Kepler:
German astronomer Johannes Kepler used mathematics to calculate the path of the planets,
finding that they traveled not in circles, as long expected, but in ellipses.iew full size image






















Johannes Kepler Facts
Born in December of 1571, young Kepler was a sickly child of poor parents. He was awarded scholarship to the University of Tübingen, where he studied to become a Lutheran minister. While there, he studied the work of Nicolaus Copernicus, who taught that the planets orbited the sun rather than the Earth, though he had no observational evidence to offer as proof.
In 1596, Kepler wrote the first public defense of the Copernican system. This was a dangerous stance, given that in 1539, Martin Luther, founder of the Lutheran church, derided the theory when he first heard it, while the Catholic church deemed such a position heretical in 1615 (they later subjected astronomer Galileo Galilei to house arrest for his publication on the subject).
In search of the most detailed notes about the paths of the planets, Kepler contacted astronomer Tycho Brahe. A wealthy Danish nobleman, Brahe built an observatory in Prague where he tracked the motions of the planets and maintained the most accurate observations of the solar system at the time. In 1600, Brahe invited Kepler to come work with him.
Brahe, however, proved to be suspicious and unwilling to share his detailed notes with his assistant. Instead, he assigned Kepler to solve the mystery of Mars, one of the most puzzling problems in astronomy at the time. Ironically, the detailed records of the challenging planet were the tools Kepler needed to understand how the solar system functioned.
When Brahe died in 1601, Kepler managed to acquire Brahe's observations before his family could use them to their financial benefit.
Kepler's laws
The Martian problem, which Kepler said he would solve in eight days, took nearly eight years. Astronomers had long struggled to figure out why Mars appeared to walk backwards across the night sky. No model of the solar system — not even Copernicus' — could account for the retrograde motion.
Using Brahe's detailed observations, Kepler realized that the planets traveled in "stretched out" circles known as ellipses. The sun didn't sit exactly at the center of their orbit, but instead lay off to the side, at one of the two points known as the focus. Some planets, such as Earth, had an orbit that was very close to a circle, but the orbit of Mars was one of the most eccentric, or widely stretched. The fact that planets travel on elliptical paths is known as Kepler's First Law.
Mars appeared to move backward when Earth, on an inner orbit, came from behind the red planet, then caught up and passed it. Copernicus had suggested that observations made from a moving Earth (rather than a centrally located one) could be a cause of the retrograde motion, but the perfect circular orbits he posited still required epicycles to account for the paths of the planets. Kepler realized that two planets, traveling on ellipses, would create the appearance of the red planet's backward motion in the night sky.
Kepler also struggled with changes in the velocities of the planets. He realized that a planet moved slower when it was farther away from the sun than it did when nearby. Once he understood that planets traveled in ellipses, he determined that an invisible line connecting the sun to a planet covered an equal amount of area over the same amount of time. He posited this, his Second Law, along with his first, which he published in 1609.
Kepler's Third Law was published a decade later, and recognized that the relationship between the period of two planets — the time they take to orbit the sun — is connected to their distance from the sun. Specifically, the square of the ratio of the period of two plants is equal to the cube of the ratio of their radius. While his first two laws focus on the specifics of a single planet's movement, his third is a comparison between the orbit of two planets.
Other notable discoveries
Though Kepler is best known for his defining laws regarding planetary motion, he made several other notable contributions to science. He was the first to determine that refraction drives vision in the eye, and that using two eyes enables depth perception. He created eyeglasses for both near and farsightedness, and explained how a telescope worked. He described images and magnification, and understood the properties of reflection.
Kepler claimed that gravity was caused by two bodies, rather than one, and as such, the moon was the cause of the motion of tides on the Earth. He suggested that the sun rotates, and created the word 'satellite'. He tried to use his knowledge of the distance Earth travels to measure the distance to the stars. Kepler also calculated the birth year of Christ.
In recognition of his contribution to his our understanding of the motion of the planets, NASA named theirplanet-finding telescope after the German astronomer.
Other references:
Johannes Kepler, by Michael Fowler of the University of Virginia