According to a new study, Chelyabinsk-scale meteorite impacts happen more often than we have been aware.

According to a new study, Chelyabinsk-scale meteorite impacts happen more often than we have been aware.

The bright flare of the Russian meteor was hard to miss, and left 1,200 people injured in February 2013. What the human eye missed was two separate high-altitude explosions that occurred over Argentina and the North Atlantic Ocean just months later. That’s according to data from an infrasound network used to track nuke tests, released Tuesday by the B612 Foundation.

The data shows that there were 26 comparable events since 2000.

Red tape appears to be preventing the U.S. military from releasing meteorite data obtained by its nuclear test monitoring system.

Red tape appears to be preventing the U.S. military from releasing meteorite data obtained by its nuclear test monitoring system.

Details of atmospheric meteor explosions, as recorded by U.S. military spacecraft sensors, were posted on a publicly accessible NASA website run by the Jet Propulsion Laboratory (JPL) in Pasadena, Calif. In fact, the military-civil cooperation was spurred by the details of the February 2013 fireball explosion over Chelyabinsk, Russia — termed a “superbolide” event. The website postings are designed to assist the scientific community’s investigation of bolides, or exceptionally bright fireballs.

However, multiple scientists noted that the JPL website had not been updated recently. That presumably meant that there was some sort of delay, as some fairly big events were detected by infrasound in the last year. “Because of budget and personnel reductions on our military partner, they ran into workforce issues to accomplish this task,” said Lindley Johnson, NEO program executive within the Planetary Science Division of NASA’s Science Mission Directorate in Washington, D.C.

In other words, it looks like everyone in the military is saying “Ain’t my job, man!” so it doesn’t get done. They need to assign someone the job and be done with it.

A history of global warming “Tipping Points” where it was declared that doomsday was certain in only a few years if we didn’t act now

Crying wolf! A history of global warming “Tipping Points” where it was declared that doomsday was certain in only a few years if we didn’t act now.

The article is quite hilarious. Again and again and again and again the climate fear-mongers have announced with absolute certainty that, unless we pass draconian government regulations, the climate was going to go crazy and we were all going to die. Sometimes they declared we only had hours, sometimes months, sometimes years, sometimes even decades, but every time they were certain they knew what was going to happen and thus we had better obey them. And anyone who dared question their certainty was worse than a fool and should be imprisoned!

Of course, none of these predictions have proven true. The climate might yet warm and even go wild, but none of these doom-sayers have done any of us any good. If things do start going bad in future years, it is now going to be very difficult to convince anyone of this fact.

Posted from Tucson International Airport. I am on the way to Denver to tape two television interviews with George Noory of Coast to Coast for his television show, Beyond Belief. Should be fun.

The existence of a Kepler-found earth-sized planet in the habitable zone has been confirmed.

Worlds without end: The existence of a Kepler-found earth-sized planet in the habitable zone has been confirmed.

The newfound planet, called Kepler-186f, was first spotted by NASA’s Kepler space telescope and circles a dim red dwarf star about 490 light-years from Earth. While the host star is dimmer than Earth’s sun and the planet is slightly bigger than Earth, the positioning of the alien world coupled with its size suggests that Kepler-186f could have water on its surface, scientists say.

In this new work, the Keck and Gemini ground-based telescopes confirmed Kepler’s discovery.

New research suggests that, in general, Mars has always been too cold to harbor liquid water on its surface.

The uncertainty of science: New research suggests that, in general, Mars has always been too cold to harbor liquid water on its surface for long periods.

Mars’ atmosphere was probably never thick enough to keep temperatures on the planet’s surface above freezing for the long term, suggests research published today in Nature Geoscience1. Although the planet’s topography indicates that liquid water has flooded Mars in the distant past, evidence increasingly suggests that those episodes reflect occasional warm spells, not a consistently hospitable phase of the planet’s history.

The research does not say that liquid water never flowed on the Martian surface, only that such events were short-lived. They looked at craters and noted that the surface has impacts from meteorites that would not have survived to the surface had the atmosphere been thick enough for liquid water.

The research however did not address Mars’ relatively smooth northern hemisphere, where there are not a lot of craters and where some scientists think there might once have been a shallow ocean. If Mars never had liquid water for long periods, why does this area lack craters?

Forecasters at Colorado State University are predicting the 2014 hurricane season will be quieter than normal.

Uh-oh: Forecasters at Colorado State University are predicting the 2014 hurricane season will be quieter than normal.

This is the same team that last year predicted 2013 would be one of the worst hurricane seasons in history. Instead, last year was one of the weakest in history, and as a result they lost their funding. That these same guys are now saying 2014 will be weak makes me fear for the American Atlantic coast. It could be wiped out this time!

An award winning science teacher was suspended when an unnamed school employee thought two student science projects looked too much like weapons.

Idiocracy: An award winning science teacher was suspended when an unnamed school employee thought two student science projects looked too much like weapons.

Schiller got into trouble after two of his students turned in science projects designed to shoot little projectiles, reports the Los Angeles Times. One of the projects used compressed air (but was not actually connected to any air). The other one was coil gun: a tube surrounded by a coil and powered by a standard AA battery.

An unidentified school employee saw the air-pressure projectile device and got scared because, to her, it looked like a fearsome weapon. The amount of knowledge the employee has concerning science – if any – is unclear.

As a result of the unnamed employee’s fears, Schiller – who actually never got to see either the air-pressure project or the coil project except in photos – was dismissed from the classroom indefinitely. School officials impounded both projects as “evidence,” according to the mother of the kid who did the coil project.

Why am I reminded of this movie scene?
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“A lot of investment in green technology has been a giant scam, if well intentioned.”

“A lot of investment in green technology has been a giant scam, if well intentioned.”

The quote, and entire interview, are significant for two reasons. First, the interview is seeped with many skeptical opinions about human caused global warming, is very critical of that movement’s effort to politicize science, and the person being interviewed is James Lovelock, the founder of of the concept of Gaia, a former strong advocate of global warming but now a skeptic.

Most significant however is where the interview is published. It is in Nature, one of the most important and influential science journals, which previously has been aggressively pushing global warming politics for years. That they allowed these politically incorrect opinions within their walls and then broadcast them to their readers signals a major cultural shift within the science community. It is beginning to be acceptable to be a skeptic again!

Scientists have found that Saturn’s hexagon-shaped jet stream is deeply rooted and that its rotation might be revealing the planet’s rotation as well.

Scientists have found that Saturn’s hexagon-shaped jet stream is deeply rooted and that its rotation might be revealing the planet’s rotation as well.

Due to the tilt of approximately 27º of the planet Saturn, its polar atmosphere undergoes intense seasonable variations with long polar nights lasting over seven years, followed by a long period of 23 years of variable illumination. However, the seasonal variations do not affect the hexagon and its jet stream at all, so both are part of an extensive wave, deeply rooted in Saturn’s atmosphere. The UPV/EHU researchers suggest that the hexagon and its stream are the manifestation of a “Rossby wave” similar to those that form in the mid-latitudes of the earth. On our planet the jet stream meanders from west to east and brings, associated with it, the system of areas of low pressure and anticyclones which we have been seeing regularly on weather maps.

On Saturn, a hydrogen gas planet, ten times the size of the Earth, cold in its upper clouds, without a solid surface, and with an atmosphere as deep as that of an ocean, “the hexagonal wavy motion of the jet stream is expected to be propagated vertically and reveal to us aspects of the planet’s hidden atmosphere,” pointed out Agustín Sánchez-Lavega, Head of the Planetary Sciences research group. “The movement of the hexagon could therefore be linked to the depths of Saturn, and the rotation period of this structure, which, as we have been able to ascertain, is 10 hours, 39 minutes and 23 seconds, could be that of the planet itself,” he added. Saturn is the only planet in the Solar System whose rotation period is not yet known.

Geologists, using computer models, have reconstructed the size and impact velocity of a giant asteroid that hit the Earth approximately 3.26 billion years ago.

Geologists, using computer models, have reconstructed the size and impact velocity of a giant asteroid that hit the Earth approximately 3.26 billion years ago.

This is a fascinating result, but it is very important to recognize its very large uncertainties. The article for example says almost nothing about how these conclusions were reached, except for this one paragraph:

Lowe, who discovered telltale rock formations in the Barberton greenstone a decade ago, thought their structure smacked of an asteroid impact. The new research models for the first time how big the asteroid was and the effect it had on the planet, including the possible initiation of a more modern plate tectonic system that is seen in the region, according to Lowe. [emphasis mine]

I have highlighted that one word because it reveals a great deal. What they did was to create a computer model of the data they had, which was merely very unusual geology spread over a certain region called the Barberton Greenstone Belt. Note also that this region is not where the impact occurred. “The study’s co-authors think the asteroid hit the Earth thousands of kilometers away from the Barberton Greenstone Belt, although they can’t pinpoint the exact location.”

The Sun continues to hiccup

It’s sunspot time again! On Monday NOAA posted its monthly update of the solar cycle, showing the sunspot activity for the Sun in February. I am once again posting it here, below the fold, with annotations.

Like it did in January, the Sun’s second peak of the solar maximum continued to beat its first peak, an unprecedented event. Though activity dropped slightly, it still remained above prediction and was only slightly below the first peak’s maximum. Overall, the second peak has been much stronger than the first, something that scientists have never seen before. In the past, when the Sun had a double peaked solar maximum, the second peak was always weaker. Not this time!
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The oldest galaxy known might be a tiny dwarf galaxy orbiting the Milky Way.

The oldest galaxy known might be a tiny dwarf galaxy orbiting the Milky Way.

Segue 1 is very, very tiny. It appears to contain only a few hundred stars, compared with the few hundred billion stars in the Milky Way Galaxy. Researchers led by Anna Frebel of the Massachusetts Institute of Technology in Cambridge collected detailed information on the elemental composition of six of the brightest of Segue 1’s stars using the Las Campanas Observatory’s Magellan Telescopes in Chile and the Keck Observatory in Hawaii. The measurements, reported in a paper accepted for Astrophysical Journal and posted on the arXiv repository, revealed that these stars are made almost entirely of hydrogen and helium, and contain just trace amounts of heavier elements such as iron. No other galaxy studied holds so few heavy elements, making Segue 1 the “least chemically evolved galaxy known.”

Complex elements are forged inside the cores of stars by the nuclear fusion of more basic elements such as hydrogen and helium atoms. When stars explode in supernovae, even heavier atoms are created. elements spew into space to infuse the gas that births the next generation of stars, so that each successive generation contains more and more heavy elements, known as metals. “Segue 1 is so ridiculously metal-poor that we suspect at least a couple of the stars are direct descendants of the first stars ever to blow up in the universe,” says study co-author Evan Kirby of the University of California, Irvine.

As the NASA lunar probe LADEE nears its planned end — where it will crash onto the Moon — the scientists running it admit that they have as yet been unable to solve its primary scientific question about levitating lunar dust.

As the NASA lunar probe LADEE nears its planned end — where it will crash onto the Moon — the scientists running it admit that they have as yet been unable to solve its primary scientific question about levitating lunar dust.

A major goal of the mission was to understand a bizarre glow on the Moon’s horizon, spotted by Apollo astronauts just before sunrise. “So far we haven’t come up with an explanation for that,” project scientist Rick Elphic, of NASA’s Ames Research Center in Moffett Field, California, said at a media briefing on 3 April. One leading idea is that the Sun’s ultraviolet rays cause lunar dust particles to become electrically charged. That dust then lofts upwards, forming a cloud that caught the light and the astronauts’ eyes.

LADEE carries an instrument that measures the impact of individual dust particles, as well as the collective signal from smaller particles. Lunar scientists had expected a certain amount of tiny dust to explain what the Apollo astronauts saw. But LADEE didn’t find it. “We did measure a signal that indicates that the amount of lofted dust has to be at least two orders of magnitude below the expectations that were based on the Apollo reports,” says Mihály Horányi, the instrument’s principal investigator, who is at the University of Colorado. Perhaps the dust lofting happens only occasionally, he suggests, and the astronauts were in just the right place at the right time to see it.

This remains an important question. Knowing what caused that horizon glow and knowing how often it occurs is essential knowledge for any future lunar base or research station.

Because of a $10 million shortfall in its astrophysics budget, NASA is weighing the fate of nine operating space telescopes.

Because of a $10 million shortfall in its astrophysics budget, NASA is weighing the fate of nine operating space telescopes.

Six of the projects vying for extended funding are U.S.-based. Three are overseen by international space agencies and have U.S. partners.

The NASA missions are: the Fermi Gamma-ray Space Telescope; the Nuclear Spectroscopic Telescope Array X-ray observatory; the infrared Spitzer Space Telescope; the Swift Telescope, which tracks gamma-ray bursts; a proposed Kepler space telescope follow-on mission known as K2; and the Wide-field Infrared Survey Explorer, which was brought out of hibernation last year to help search for asteroids on a collision course with Earth.

Also in the running are two European Space Agency missions, XMM-Newton — an X-ray observatory — and Planck, which studied relic radiation from the Big Bang. Planck was decommissioned in October, but its data analysis program continues.

The final contender is Japan’s Suzaku X-ray telescope.

A skydiver’s helmet cam captures a meteorite zipping past him as it falls.

A skydiver’s helmet cam videotapes a meteorite zipping past him as it falls.

The incident happened back in the summer of 2012, when skydiver Anders Helstrup and other members of the Oslo Parachute Club took to the skies above Hedmark, Norway. Helstrup documented the jump with two cameras fixed to the front and back of his helmet. Helstrup tells NRK (the largest media outlet in Norway) that on the way down he felt “something” happen, but didn’t know what. It was only after landing and reviewing his camera footage that he discovered something shocking: a rock had fallen from the heavens and missed him by just a few yards.

Video below the fold. The news woman is annoying, but the footage is quite cool.
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A scientist whistleblower has found that publicly questioning bad science papers vs privately notifying the publisher significantly increases the chances of getting them retracted.

Surprise, surprise! A scientist whistleblower has found that publicly questioning bad science papers vs privately notifying the publisher significantly increases the chances of getting them retracted.

[Paul] Brookes ran the blog Science Fraud from July 2012 to January 2013, before closing it down in response to threats of legal action. For the PeerJ study, Brookes compared the outcomes of two sets of papers — 274 whose alleged data problems he chronicled on his blog, and 223 that he was e-mailed about but did not post before he shut the site down. Those private e-mails, he says, were also copied to the relevant journals, funding agencies and authors’ research institutions, so authorities would also have had the opportunity to review the allegations.

Of the 274 papers Brookes blogged about, 16 were retracted and 47 corrected by December 2013, he reports, meaning that action was taken in 23% of the cases. But of the 223 unpublicized papers, only two were retracted and five corrected — a rate of 3%.

As always, the more freedom and openness we have, the better. The only people who suffer in such a situation are the incompetent and dishonest ones.

A new analysis of data from Messenger suggests that violent explosive volcanism occurred throughout much of Mercury’s history.

A new analysis of data from Messenger suggests that violent explosive volcanism occurred throughout much of Mercury’s history.

What is interesting about this result is that previously it was believed that explosive volcanism didn’t happen at all on Mercury.

On Earth, volcanic explosions like the one that tore the lid off Mount St. Helens happen because our planet’s interior is rich in volatiles — water, carbon dioxide and other compounds with relatively low boiling points. As lava rises from the depths toward the surface, volatiles dissolved within it change phase from liquid to gas, expanding in the process. The pressure of that expansion can cause the crust above to burst like an overinflated balloon.

Mercury, however, was long thought to be bone dry when it comes to volatiles, and without volatiles there can’t be explosive volcanism. But that view started to change in 2008, after NASA’s MESSENGER spacecraft made its first flybys of Mercury. Those glimpses of the surface revealed deposits of pyroclastic ash — the telltale signs of volcanic explosions — peppering the planet’s surface. It was a clue that at some point in its history Mercury’s interior wasn’t as bereft of volatiles as had been assumed.

The new conclusions have not only found evidence of explosive volcanism, it found a wide range of ages for these deposits, indicating that the explosive volcanism took place across an extended period of time.

Climate scientists think the first major El Niño since 1997-1998 is beginning to brew in the Pacific.

Climate scientists think the first major El Niño since 1997-1998 is beginning to brew in the Pacific.

The first sign of a brewing El Niño weather pattern came in January, as trade winds that normally blow from the east reversed course near Papua New Guinea. Barrelling back across the tropical Pacific Ocean, they began to push warm water towards South America. Now climate scientists and forecasters are on high alert.

A major El Niño event — a periodic warming of waters in the eastern equatorial Pacific — could boost temperatures and scramble weather worldwide. The most recent major event, in 1997–98, was linked to thousands of deaths and tens of billions of dollars in damage from droughts, fires and floods across several continents. Yet more than 15 years later, forecasting the timing and intensity of El Niño remains tricky, with incremental improvements in climate models threatened by the partial collapse of an ocean-monitoring system that delivers the data to feed those models.

Note the date of the last event, 1997-1998. This was also the last time the world’s global temperature saw an increase. At the time global warming scientists were saying that global warming would increase the number and severity of El Niño events, which in turn would raise havoc with the climate. Instead, we have gone more than a decade and a half without any significant El Niño event, and the global temperature rise has ceased.

Note also that the article focuses on the difficulty scientists have had in predicting El Niño. These are the same global warming scientists who are also certain they can predict the exact temperature rise for the next two hundred years.

Astronomers have found an asteroid with its own rings.

Astronomers have found an asteroid with its own rings.

Chariklo is the largest member of a class known as the Centaurs and it orbits between Saturn and Uranus in the outer Solar System. Predictions had shown that it would pass in front of the star UCAC4 248-108672 on 3 June 2013, as seen from South America. Astronomers using telescopes at seven different locations, including the 1.54-metre Danish and TRAPPIST telescopes at ESO’s La Silla Observatory in Chile, were able to watch the star apparently vanish for a few seconds as its light was blocked by Chariklo — an occultation.

But they found much more than they were expecting. A few seconds before, and again a few seconds after the main occultation there were two further very short dips in the star’s apparent brightness. Something around Chariklo was blocking the light! By comparing what was seen from different sites the team could reconstruct not only the shape and size of the object itself but also the shape, width, orientation and other properties of the newly discovered rings.

The team found that the ring system consists of two sharply confined rings only seven and three kilometres wide, separated by a clear gap of nine kilometres — around a small 250-kilometre diameter object orbiting beyond Saturn.

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