Showing posts with label gigantic. Show all posts
Showing posts with label gigantic. Show all posts

Wednesday, October 1, 2014

NASA Cassini: Titan's Gigantic polar clouds of hydrogen cyanide

Titan's hazy orange globe hangs before the Cassini spacecraft. 

Image credit NASA/JPL/Space Science Institute.

Gigantic polar clouds of hydrogen cyanide roughly four times the area of the UK are part of the impressive atmospheric diversity of Titan, the largest moon of Saturn, a new study led by Leiden Observatory, the Netherlands Institute for Space Research and the University of Bristol has found.

The research is published today in Nature.

Titan is unique in our solar system because of its dense nitrogen-methane atmosphere, which is very similar to Earth's in some ways, but very different in others.

For example, air temperatures are around 200 degrees colder and, in contrast to the warm salt water seas of Earth, frigid hydrocarbon lakes populate Titan's surface.

Titan has seasons just like Earth, only each season lasts over seven years instead of three months due to its ponderous orbit around the Sun.

After equinox in 2009, Titan's south pole entered the perpetual darkness of polar winter. Soon after, instruments on NASA's Cassini spacecraft observed the development of a gigantic polar cloud covering over one million square kilometres, roughly four times the area of the UK.

Bristol researcher and co-author Dr Nick Teanby said: "The cloud was first seen in images from Cassini's cameras taken in 2012."

"It started off quite small but soon grew to cover the entire south polar region. This was totally unexpected and set us puzzling over what the cloud could be made of."

"Unfortunately, while the images showed that the cloud was very high up, at over 250km above the surface, they did not allow us to figure out what the cloud was actually made of or why it was there."

For the next two years Cassini gathered more data including infrared spectra of the cloudy region.

Lead author Remco de Kok said: "When we looked at the spectra, we saw two large peaks that weren't present in spectra of other places on Titan."

"These peaks coincided exactly with the peaks you'd expect from ice particles of hydrogen cyanide, or 'blauwzuur' (blue acid) as it's known in the Netherlands, which is highly toxic."

"This was very surprising to us, since we did not expect HCN ice to be able to form so high in Titan's atmosphere."

This new research suggests that Titan's south pole must be extremely cold to allow hydrogen cyanide to condense.

In fact, the upper atmosphere must have cooled by over 50 degrees in less than a year to reach a blisteringly cold -150C.

Remco de Kok concluded: "This is a very rapid change given Titan's long annual cycle and is much colder than previously thought possible."

"It suggests that once the pole is in shadow the upper atmosphere acts as a very efficient radiator of heat, perhaps due to the high abundance of exotic hydrocarbon and nitrogen based compounds, which emit strongly in the infrared."

"Cassini is set to continue observing Titan until it takes a dive into Saturn at the end of its mission in 2017. It will be fascinating to see how the cloud will develop."

More information: HCN ice in Titan's high-altitude southern polar cloud, Nature, dx.doi.org/10.1038/nature13789

Friday, September 5, 2014

Dreadnoughtus: A gigantic, exceptionally complete sauropod dinosaur

Kenneth Lacovara, PhD, with the 30-foot tail of Dreadnoughtus schrani, stretching along the length of the wall and around the corner in his lab. 

Beside Lacovara's hand is a set of chevron bones. 

Pairs of these chevrons run beneath each of the tail vertebrae and were found for each vertebra in the tail of Dreadnoughtus. 

In this animal the chevrons are noteworthy for the wide area for muscle attachment on the lower portion of the Y-shaped chevron. 

In Dreadnoughtus this attachment area is broad and spatula-shaped, allowing for extremely large tail muscles, giving this animal an extraordinarily powerful, 'weaponized' tail in Lacovara's description. 

Credit: Drexel University

Scientists have discovered and described a new supermassive dinosaur species with the most complete skeleton ever found of its type.

At 85 feet (26 m) long and weighing about 65 tons (59,300 kg) in life, Dreadnoughtus schrani is the largest land animal for which a body mass can be accurately calculated.

Its skeleton is exceptionally complete, with over 70 percent of the bones, excluding the head, represented. Because all previously discovered supermassive dinosaurs are known only from relatively fragmentary remains,

Dreadnoughtus offers an unprecedented window into the anatomy and biomechanics of the largest animals to ever walk the Earth.


"Dreadnoughtus schrani was astoundingly huge," said Kenneth Lacovara, PhD, an associate professor in Drexel University's College of Arts and Sciences, who discovered the Dreadnoughtus fossil skeleton in southern Patagonia in Argentina and led the excavation and analysis.

"It weighed as much as a dozen African elephants or more than seven T. rex. Shockingly, skeletal evidence shows that when this 65-ton specimen died, it was not yet full grown. It is by far the best example we have of any of the most giant creatures to ever walk the planet."

Lacovara and colleagues published the detailed description of their discovery, defining the genus and species Dreadnoughtus schrani, in the journal Scientific Reports from the Nature Publishing Group today.

The new dinosaur belongs to a group of large plant eaters known as titanosaurs. The fossil was unearthed over four field seasons from 2005 through 2009 by Lacovara and his team..

Over 100 elements of the Dreadnoughtus skeleton are represented from the type specimen, including most of the vertebrae from the 30-foot-long tail, a neck vertebra with a diameter of over a yard, scapula, numerous ribs, toes, a claw, a small section of jaw and a single tooth, and, most notably for calculating the animal's mass, nearly all the bones from both forelimbs and hindlimbs including a femur over 6 feet tall and a humerus.

A smaller individual with a less-complete skeleton was also unearthed at the site.

The 'gold standard' for calculating the mass of quadrupeds (four-legged animals) is based on measurements taken from the femur (thigh bone) and humerus (upper arm bone).

Because the Dreadnoughtus type specimen includes both these bones, its weight can be estimated with confidence.

Prior to the description of the 65-ton Dreadnoughtus schrani specimen, another Patagonian giant, Elaltitan, held the title of dinosaur with the greatest calculable weight at 47 tons, based on a recent study.

Overall, the Dreadnoughtus schrani type specimen's bones represent approximately 45.3 percent of the dinosaur's total skeleton, or up to 70.4 percent of the types of bones in its body, excluding the skull bones. This is far more complete than all previously discovered giant titanosaurian dinosaurs.

"Titanosaurs are a remarkable group of dinosaurs, with species ranging from the weight of a cow to the weight of a sperm whale or more. But the biggest titanosaurs have remained a mystery, because, in almost all cases, their fossils are very incomplete," said Matthew Lamanna.

A US-Argentinian team led by Drexel University's Kenneth Lacovara, PhD, excavated the skeleton of Dreadnoughtus schrani from southern Patagonia over four field seasons from 2005 through 2009. 

The completeness and articulated nature of the two skeletons they found are evidence that these individuals were buried in sediments rapidly before their bodies fully decomposed. 

Credit: Kenneth Lacovara

For example, Argentinosaurus was of a comparable and perhaps greater mass than Dreadnoughtus, but is known from only a half dozen vertebrae in its mid-back, a shinbone and a few other fragmentary pieces; because the specimen lacks upper limb bones, there is no reliable method to calculate a definitive mass of Argentinosaurus.

Futalognkosaurus was the most complete extremely massive titanosaur known prior to Dreadnoughtus, but that specimen lacks most limb bones, a tail and any part of its skull.

To better visualize the skeletal structure of Dreadnoughtus, Lacovara's team digitally scanned all of the bones from both dinosaur specimens.

They have made a "virtual mount" of the skeleton that is now publicly available for download from the paper's open-access online supplement as a three-dimensional digital reconstruction.

"This has the advantage that it doesn't take physical space," Lacovara said. "These images can be ported around the world to other scientists and museums. The fidelity is perfect. It doesn't decay over time like bones do in a collection."

"Digital modeling is the wave of the future. It's only going to become more common in paleontology, especially for studies of giant dinosaurs such as Dreadnoughtus, where a single bone can weigh hundreds of pounds," said Lamanna.

The 3D laser scans of Dreadnoughtus show the deep, exquisitely preserved muscle attachment scars that can provide a wealth of information about the function and force of muscles that the animal had and where they attached to the skeleton, information that is lacking in many sauropods.

Efforts to understand this dinosaur's body structure, growth rate, and biomechanics are ongoing areas of research within Lacovara's lab.

Of the 142 types of bones not including the skull, 100 types of bones, or 70.4 percent, are represented in the Dreadnoughtus skeleton. Skull bones from any titanosaur are extremely rarely recovered. Credit: Lacovara Lab, Drexel University

More information: Scientific Reports, dx.doi.org/10.1038/srep06196

Saturday, May 31, 2014

NASA's IRIS: Observing a gigantic CME eruption of solar material

A coronal mass ejection, or CME, surged off the side of the sun on May 9, 2014, and NASA's newest solar observatory caught it in extraordinary detail. 

This was the first CME observed by the Interface Region Imaging Spectrograph (IRIS), which launched in June 2013 to peer into the lowest levels of the sun's atmosphere with better resolution than ever before. 

IRIS must commit to pointing at certain areas of the sun at least a day in advance, so catching a CME in the act involves some educated guesses and a little bit of luck.

"We focus in on active regions to try to see a flare or a CME," said Bart De Pontieu, the IRIS science lead at Lockheed Martin Solar & Astrophysics Laboratory in Palo Alto, California. "And then we wait and hope that we'll catch something. This is the first clear CME for IRIS so the team is very excited."

The IRIS imagery focuses in on material of 30,000 kelvins at the base, or foot points, of the CME.

The line moving across the middle of the movie is the entrance slit for IRIS's spectrograph, an instrument that can split light into its many wavelengths, a technique that ultimately allows scientists to measure temperature, velocity and density of the solar material behind the slit.

The field of view for this imagery is about five Earths wide and about seven-and-a-half Earths tall.


Watch the movie to see how a curtain of solar material erupts outward at speeds of 1.5 million miles per hour.

A coronal mass ejection burst off the side of the sun on May 9, 2014. The giant sheet of solar material erupting was the first CME seen by NASA's Interface Region Imaging Spectrograph (IRIS). 

The field of view seen here is about five Earths wide and about seven-and-a-half Earths tall. Credit: NASA/LMSAL/IRIS/SDO/Goddard


Wednesday, February 12, 2014

NASA Chandra: Gigantic Black Hole Jets Shines - Video



A powerful jet shooting from a supermassive black hole at the center of a distant galaxy shines in a newly released image and video tour.

NASA's Chandra X-ray Observatory gathered data that was used to create the new photo of the galaxy Centaurus A — which is located about 12 million light-years from Earth.

The space-based observatory collected the data from 1999 to 2012, but the space agency released the photo on Feb. 6. You also can take a full video tour of the Centarus A photo.

While the black hole jet is a prominent feature, the picture also shows what scientists think to be the leftovers of a collision between Centaurus A (Cen A for short) and a smaller galaxy millions of years ago.

The "dust lane" that wraps around the middle of Cen A could be the remains of the incorporated galaxy, NASA officials said in the video.

The galaxy Centaurus A shines in a photo taken by the Chandra X-ray Observatory. 

Image uploaded Feb. 10, 2014. Credit: NASA/CXC/U.Birmingham/M.Burke et al.

"In this image, the lowest-energy X-rays Chandra detects are in red, while the medium-energy X-rays are green, and the highest-energy ones are blue," a NASA official said in the video explanation.

The Chandra X-ray Observatory has been observing Cen A since 1999, just after the space telescope came online. Scientists have found that point-like X-ray sources in Cen A fall into two groups.

The X-ray sources come from a system where either a black hole or neutron star is siphoning gas from a companion star, NASA officials said.

"These compact objects form by the collapse of massive stars, with black holes resulting from heavier stars than neutron stars," NASA officials said.

"The results suggested that nearly all of the compact objects [neutron stars or black holes] had masses that fell into two categories: either less than twice that of the sun, or more than five times as massive as the sun. These two groups correspond to neutron stars and black hole."

The Chandra observations are the first that show that the gap could occur in distant galaxies, space agency representatives said.

"If it turns out to be ubiquitous, it may mean that a special, rapid type of stellar collapse is required in some supernova explosions," NASA officials said.

Saturday, September 1, 2012

NASA SDO Image: Gigantic Solar filament eruption

NASA SDO observed today's gigantic solar filament eruption.

Credit: NASA SDO