Fragments of the Sutter’s Mill meteorite fall collected by astronomer Dr. Peter Jennisken. (NASA)

Researchers have struck scientific gold at Sutter’s Mill, site of the famed California Gold Rush where the precious metal was first discovered in 1848.

In April of this year, the scientists recovered a rare meteorite which contains clues to the early history of the solar system.

Using Doppler radar, the same technology used by weather forecasters, the scientists detected a shower of meteors raining down over the communities of Coloma and Lotus, just after the asteroid broke up in the atmosphere.

That allowed scientists to, for the first time,  quickly find, recover and study a primitive meteorite that had little exposure to the elements.

It’s the most pristine look at the surface of ancient asteroids scientists have been able to study so far. Because of the rapid recovery of materials, scientists were able to detect compounds that quickly disappear once a meteorite hits Earth.

Reporting in Science, the researchers say their rare find was classified as a Carbonaceous-Mighei or CM-type carbonaceous chondrite meteorite, which is known to contain water and complex organic compounds, such as amino acids, molecules that help form life.

But, according to NASA’s Danny Glavin, he and the other scientists weren’t able to detect many of the amino acids in their find because it appeared the samples had been heated in space before arriving on Earth.

“The small three meter-sized asteroid that impacted over California’s Sierra Nevada came in at twice the speed of typical meteorite falls,” said lead author Peter Jenniskens, of the SETI Institute and NASA’s Ames Research Center, both located in California. “Clocked at 64,000 miles per hour, it was the biggest impact over land since the impact of the four meter-sized asteroid 2008 TC3, four years ago over Sudan.”

The scientists also say that, for the first time, they were able to identify the region of space where these types of meteorites come from.

After studying photographs and video of the asteroid, Jenniskens figured that it came in on an unusually low-angled orbit, more like a comet‘s orbit, passing closer to the sun than what has been learned from past recorded meteorite falls.

Scientists found the asteroid, as it was in orbit, was influenced by the gravity of both the Sun and Jupiter at times.

“It circled the sun three times during a single orbit of Jupiter, in resonance with that planet,” Jenniskens said.

A meteor flashes across the sky during the peak of the November 2009 Leonid Meteor Shower. (Photo: Ed Sweeney via Wikimedia Commons)

The asteroid that spawned the meteorite was estimated to be around 45359 kg.  Of that, less than 1kg was actually recovered on the ground in the form of 77 tiny meteorites. The biggest of those meteorites was 205 grams.

While the scientists didn’t find much actual gold in the Sutter’s Mill meteorite, about 150 parts per billion, it was still “scientific gold,” according to co-author and cosmochemist Qing-zhu Yin of the University of California at Davis.

“With 78 other elements measured, Sutter’s Mill provides one of the most complete records of elemental compositions documented for such primitive meteorites,” he said.

The moon (Photo: NASA)

The Earth and its moon started with a big bang, according to a new theory from NASA scientists, who believe both were born out of collisions between two massive developing planets.The new theory suggests the two giant planetary bodies, each about five times the size of Mars, collided with each other twice.

After the first collision, the planets smashed into each other again, leaving behind material which resulted in our early Earth. The fledgling planet was surrounded by a disk of left-over material, which later combined to form the moon.

This new theory challenges the widely-held “giant impact hypothesis,” which suggests the moon formed early in our solar system’s history after an enormous impact between Earth and a Mars-sized planet that was still being formed.  Some call that protoplanet Theia, after the mother of the goddess of the moon in Greek mythology.

However, skeptics say if the Theia theory were true, Earth and the moon would have different chemical compositions from each other, which they don’t.

Iconic photo of the Earth and moon as seen from the Apollo 8 spacecraft while in lunar orbit on 12/24/1968. (Photo: NASA)

According to the new NASA theory, the two collisions, along with the subsequent melding of left-over material, formed both the Earth and the moon, which is why they have similar chemical compositions. “Our understanding of the solar system is constantly being refined with each new discovery,” says NASA’s Greg Schmidt. “This research illustrates the importance of modeling planetary formation to enhance our scientific understanding of the moon and its place in the solar system.”

The model which demonstrates this new theory was developed at the Southwest Research Institute (SwRI), in San Antonio, Texas by Robin M. Canup.

Canup says her work was inspired by previous studies on the early history of the moon, which explain the similar chemical composition of the Earth and moon, while at the same time producing an appropriate mass for Earth and the moon.

“The ultimate likelihood of each impact scenario will need to be assessed by improved models of terrestrial planet formation,” Canup said.  Canup’s work is outlined in Science.

Video: A computer simulation of a low-velocity collision of two protoplanets that contain 45 and 55 percent of the Earth’s mass. Colors indicate particle temperature in kelvin, with blue-to-red indicating temperatures from 2,000 K to in excess of 6,440 K. After the first protoplanetary impact, they re-collide, merge and form a rapidly spinning Earth-mass planet that is surrounded by a disk of particles that would later form the Moon. (Video: Southwest Research Institute)

This small portion of a deep space image taken by the Canada-France-Hawaii Telscope Legacy Survey reveals thousands of galaxies yet to be explored. (Image: © CFHT/Coelum/Terapix/AstrOmatic)

Scientists have released the final version of the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS), data gathered over six years which probes deep recesses of the Universe, including galaxies as far as nine billion light-years away.

This treasure trove of information  will allow scientists to better study dark matter; energy;  new, developing and evolving galaxies; and any solar system bodies beyond the orbit of Neptune, in a region called the Kuiper Belt.

The unique and powerful multi-color collection of astronomical images and data put together by the international team,  was gathered from the Canada-France-Hawaii Telescope (CFHT) located atop the summit of Hawaii’s Mauna Kea volcano.

The project is led by French and Canadian astronomers who imaged and mapped an extremely large volume of the Universe using a ground-based, rather than space telescope, such as the Hubble.

The dome of the Canada-France-Hawaii Telescope (CFHT) is a world class 3.6-meter telescope that sits above the clouds atop Hawaii’s Mauna Kea, a dormant volcano. (Photo: © J.-C. Cuillandre (CFHT))

“The Legacy Survey has already generated a lot of results and is the most heavily cited work from CFHT,” says Raymond Carlberg of the University of Toronto, who helped with project planning and oversight.

The high-quality images  allowed them to produce a large data bank which includes dark matter maps on the largest scale  ever  observed, according to the researchers.

The data set also contains the first high-quality light measurements which show that dark energy closely resembles the cosmological constant,  which counteracts the gravitational pull of matter, something  Albert Einstein predicted in his General Theory of Relativity and  later thought might have been his greatest mistake.

Although dark matter and dark energy dominate the universe,  they can’t be seen or identified.  However, astronomers are able to measure the effect that dark energy has on the rate of the expansion of our universe.

To help scientists gain a better understanding of dark energy, the Legacy Survey team set out to precisely measure several hundred “Type Ia” supernovae, which they say are excellent standard light measurements for measuring galaxy distances.

At the heart of the Legacy Survey was a state-of-the-art, 340-Megapixel digital camera called MegaCam, that was coupled to the 3.6-meter Canada-France-Hawaii telescope in Hawaii.  More than 15,000 individual MegaCam images were used to produce the survey.

This is image filled with a number of galaxies and other cosmological objects was taken from just a very small fraction of the Canada-France-Hawaii Telescope Legacy Survey (Image: ©CFHT/Coelum)

Observations began in 2003 and ended in 2009.  The scientists then took three more years to precisely calibrate the huge volume of data gathered from the images.

In the course of their work, project members were able to image and map across a combined area of the heavens which is about 800 times the surface area of the full moon as seen in the sky.

The survey revealed some 38 million celestial objects, which were mostly  distant galaxies in various stages of evolution.

The search for new solar system bodies beyond Neptune’s orbit, in a region called the Kuiper Belt, also proved successful. That area of space contains numerous chunks of material left over from when the solar system formed.

The astronomers  were able to collect what they term “an exceptional sample” of minor bodies in that region.

A new initiative, the Canada-France Ecliptic Plane Survey, has taken over that area of study. With Legacy Survey data, as well from other telescopes, those scientists have so far been able to determine the orbits of nearly 200 Kuiper Belt objects with high-precision. Other astronomers studying the formation of our solar system are also using the Legacy Survey’s information to test various scientific models.

“The legacy  will not be limited to follow-ups of the survey,” says Yannick Mellier, who leads a group of scientists  contributing to the European Space Agency’s Euclid mission – a space telescope with cameras designed to accurately measure dark energy. “MegaCam and the CFHTLS truly paved the way for the Euclid space mission both from the scientific and technical aspects.”

As shown in the above video, the supernova reaches its peak very quickly (a few days) and then slowly fades out over weeks to months. At its peak, a supernova can shine brighter than all the other stars combined in the host galaxy. The animation spans about 4 months, from pre- to post-supernova status. Credit: SNLS