A Day for Earth, but a Whole Week for Dark Skies

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Wednesday is Earth Day, but all week — Monday, April 20 through Saturday, April 26 — is National Dark Sky Week in America, when people are asked to dim the lights to see more stars.

If enough people participate, backyard and professional astronomers might be treated with a week of darker, starrier skies. The bigger idea is to raise awareness about sensible lighting practices, so skies might get a little bit darker all the time. And not just for astronomy buffs. Besides aesthetics, evidence is mounting that light pollution could have far-reaching effects for the environment and even public health.

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360-degree panoramic picture of the Milky Way as seen from Death Valley. Credit: Dan Duriscoe, National Park Service.

Jennifer Barlow, founder of the event, said the only way National Dark Sky Week can succeed is if more people participate every year. “No reduction in light pollution can be made unless a significant number of people turn off their lights,” she said.

Besides turning out the lights, the participating groups are encouraging people to attend star parties, visit local observatories, or “dust off the old telescope from the attic,” Barlow said.

Year-round, the International Dark Sky Association encourages people to shield lights, or use fixtures that focus light downward instead of up into the sky. Reducing extraneous light, especially at ball fields, is a major step in the right direction. And certain types of lighting — like low-pressure sodium — are better than others.

Flagstaff, Arizona became the world’s first International Dark-Sky City in 2001, owing to the presence of several important observatories — it’s the home of Lowell Observatory and the U.S. Naval Observatory — along with the dedicated efforts of a handful of astronomers. The city government and the vast majority of businesses have readily complied with responsible lighting codes to protect views of the night sky for residents and astronomers alike. 

The skies are noticeably dark over Flagstaff; the stars are rich at night. The Grand Canyon is even more impressive, especially on the north side. The views after dark are as stunning and magical as those during  the day.

But even those skies aren’t as good as they could be, because light pollution from cities up to 200 miles away — including Las Vegas and Phoenix — is gradually creeping in. Chad Moore, a dark skies advocate who works for the National Park Service in Denver, has spent nearly a decade documenting the skies over 55 of the nation’s parks, which are usually the best places to see stars.

Parts of rare parks — Capitol Reef, Great Basin and Big Bend among them — boast truly dark skies, he said.

Moore pointed out there are reasons besides beauty to rein in light pollution: “In the last 10 years there has been a revolution in our understanding of animal habitat and what animals require,” he said. “There are links between artificial light and cancer in humans. There’s a lot we didn’t know about.”

Second photo caption: 360-degree panoramic picture of the Milky Way as seen from Death Valley. Credit: Dan Duriscoe, National Park Service.

For more information:

National Dark Sky Week 
International Dark-Sky Association
IYA Dark Skies Awareness
Starlight Initiative
World Night in Defense of Starlight
American Astronomical Society
Astronomical League
NASA IYA site


Major Utility Company Makes Agreement for Space Based Solar Power

Solar Collecting Satellite. Image courtesy of Mafic Studios.

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One of the largest utility companies in the US has decided to look towards space to find more power. Pacific Gas and Electric (PG&E) in California announced a proposed agreement with startup company Solaren Corporation to provide 200 mega watts of space based solar power (SBSP) starting in 2016. PG&E is now seeking approval from California state regulators for permission to sign this agreement. While PG&E is not making any financial investment at this time, the announcement shows that SBSP is being taken seriously as a viable energy source. PG&E and the two other California utilities are required by the state to source 20 percent of their power from renewable sources by 2010 and 30 percent by 2017. None are producing the required amount so far.

Solaren Corporation is a small, 8-year-old company based in California whose executives have experience working for Boeing and Lockheed Martin. According to PG&E’s website, Solaren says it plans to generate the power using solar panels in earth orbit, then convert it to radio frequency energy for transmission to a receiving station in California. From there, the energy will be converted to electricity and fed into PG&E’s power grid

The proposed agreement is for the delivery of 200MW starting in 2016 for 15 years.

Earlier this year Universe Today interviewed Peter Sage from Space Energy, another SBSP company. Sage said in a statement released today that this announcement is a
“huge step forward for both Solaren and Space Energy as it highlights to the investment community that utility firms are willing to recognize Space-Based Solar Power as a credible and viable source of energy.” Sage added that while the 200 mega watts Solaren is planning to provide represents only 20% of the planned capacity of one of Space Energy’s satellites, it successfully validates the overall business case for SBSP within the larger energy industry.

The U.S. Department of Energy and NASA began seriously studying the concept of solar power satellites in the 1970s, again in the 1990’s and in 2007, a major study by the Defense Department’s National Security Space Office gave the concept another boost, concluding that “there is enormous potential for energy security, economic development, improved environmental stewardship … and overall national security for those nations who construct and possess a SBSP capability.”

It seems like a win-win situation for PG&E. They told their customers, “If Solaren succeeds, PG&E’s customers have a great opportunity to benefit from affordable clean energy. There is no risk to PG&E customers; PG&E has contracted only to pay for power that Solaren delivers.”

PG&E has 5.1 million electric customer accounts and 4.2 million natural-gas customer accounts in Northern and Central California.

Sources: Space Energy press release, PG&E website

Without Nickel, Life on Earth Could Finally Breathe

Caption: Banded iron formations like this from northern Michigan contain evidence of a drop in dissolved nickel in ancient oceans. Credit: Carnegie Institution for Science

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Researchers have long puzzled over why oxygen flourished in Earth’s atmosphere starting around 2.4 billion years.

Called the “Great Oxidation Event,” the transition “irreversibly changed surface environments on Earth and ultimately made advanced life possible,” said Dominic Papineau of the Carnegie Institution’s Geophysical Laboratory.

Now, Papineau has co-authored a new study in the journal Nature,  which reveals new clues to the mystery in ancient sedimentary rocks.

The research team, led by Kurt Konhauser of the University of Alberta in Edmonton, analyzed the trace element composition of sedimentary rocks known as banded-iron formations, or BIFs, from dozens of different localities around the world, ranging in age from 3,800 to 550 million years. Banded iron formations are unique, water-laid deposits often found in extremely old rock strata that formed before the atmosphere or oceans contained abundant oxygen. As their name implies, they are made of alternating bands of iron and silicate minerals.

They also contain minor amounts of nickel and other trace elements. And the history of nickel, the researchers think, may reveal a secret to the origin of modern life.

Nickel exists in today’s oceans in trace amounts, but was up to 400 times more abundant in the Earth’s primordial oceans. Methane-producing microorganisms, called methanogens, thrive in such environments, and the methane they released to the atmosphere might have prevented the buildup of oxygen gas, which would have reacted with the methane to produce carbon dioxide and water.

A drop in nickel concentration would have led to a “nickel famine” for the methanogens, who rely on nickel-based enzymes for key metabolic processes. Algae and other organisms that release oxygen during photosynthesis use different enzymes, and so would have been less affected by the nickel famine. As a result, atmospheric methane would have declined, and the conditions for the rise of oxygen would have been set in place.

The researchers found that nickel levels in the BIFs began dropping around 2.7 billion years ago and by 2.5 billion years ago was about half its earlier value.

“The timing fits very well. The drop in nickel could have set the stage for the Great Oxidation Event,” Papineau said. “And from what we know about living methanogens, lower levels of nickel would have severely cut back methane production.”

As for why nickel dropped in the first place, the researchers point to geology. During earlier phases of the Earth’s history, while its mantle was extremely hot, lavas from volcanic eruptions would have been relatively high in nickel. Erosion would have washed the nickel into the sea, keeping levels high. But as the mantle cooled, and the chemistry of lavas changed, volcanoes spewed out less nickel, and less would have found its way to the sea.

“The nickel connection was not something anyone had considered before,” Papineau said. “It’s just a trace element in seawater, but our study indicates that it may have had a huge impact on the Earth’s environment and on the history of life.”

Source: Carnegie Institution for Science, via Eurekalert.

Was the Tunguska Fireball a Comet Chemical Bomb?

It was an energetic event that occurred over Tunguska, but what caused it? (Don Davis)

[/caption]Over a century ago, on June 30th, 1908 a huge explosion detonated over an unpopulated region of Russia called Tunguska. It is probably one of the most enduring mysteries of this planet. What could cause such a huge explosion in the atmosphere, with the energy of a thousand Hiroshima atomic bombs, flattening a forest the area of Luxembourg and yet leaving no crater? It is little wonder that the Tunguska event has become great material for science fiction writers; how could such a huge blast, that shook the Earth’s magnetic field and lit up the Northern Hemisphere skies for three days leave no crater and just a bunch of flattened, scorched trees?

Although there are many theories as to how the Tunguska event may have unfolded, scientists are still divided over what kind of object could have hit the Earth from space. Now a Russian scientist believes he has uncovered the best answer yet. The Earth was glanced by a large comet, that skipped off the upper atmosphere, dropping a chunk of comet material as it did so. As the comet chunk heated up as it dropped through the atmosphere, the material, packed with volatile chemicals, exploded as the biggest chemical explosion mankind had ever seen…

12,000 years ago, a large object smashed into North America, causing global destruction. Dust and ash was released into the atmosphere, triggering global cooling and possibly causing the extinction of a number of large mammals around this time. The Tunguska event was of a similar energy to that catastrophic impact, but fortunately for us, Tunguska had a benign effect on the world. It simply exploded high in the atmosphere, flattened a region of Russia and vaporized.

Significantly, the energy of the chemical explosion is substantially lower than the kinetic energy of the body,” says Edward Drobyshevski of the Russian Academy of Sciences in St Petersburg, who has published his research into the Tunguska event. The fact that the Tunguska explosion energy is lower than what is expected of the kinetic energy of an object that hit the Earth from space is key to his work. Drobyshevski therefore concludes that the event must have been caused not by an asteroid or whole comet, it was actually caused by a fragment of comet material that fell off as the main cometary body skipped off the Earth’s upper atmosphere. This means that the Earth was hit on a tangent and the fragment dropped comparatively slowly toward the surface.

Sounds reasonable so far, but how did the fragment explode? Using our new understanding as to what chemicals comets contain, Drobyshevski surmises the fragment was rich in hydrogen peroxide. This is where the magic happened. The explosion was not due to a rapid release of kinetic energy, it was in fact a hydrogen peroxide bomb. As the fragment descended, it heated up. As the reactive chemicals in the material got hot, they explosively disassociated to form oxygen and water, ripping the fragment apart. The Tunguska event was therefore a huge chemical bomb and not a “regular” comet-hits-Earth impact.

An interesting study. Not content with dropping asteroids on our planet, the Universe has started throwing hydrogen peroxide explosives at us too. Whatever next?

Source: The Physics arXiv Blog

Countdown to Earth Hour 2009…


There’s less than 24 hours left before Earth Hour 2009 will begin. While you may hotly debate whether or not turning out your lights for one hour can impact our global climate – it’s not about what actually happens to our planet during that hour, but about showing you care. 3,900 cities and towns in 84 countries around the world will be shutting down the lights at 8:30 pm local time in one of the biggest events in history. Even if you don’t care, take the time to read just a little bit more… Where will you be when the lights go out?

According the latest Earth Hour bulletin: “More than 300 cities and towns in the U.S. representing 43 states and the District of Columbia are going dark as part of the largest global climate event in history. Before the rooster crows in most American cities on Saturday morning, lights will already have gone dark in cities like Christchurch, Sydney and Brisbane. By breakfast time on the U.S. East Coast, the cities of Beijing, Kuala Lumpur, Jakarta, Singapore and Manila will be celebrating the arrival of the largest global climate event in history. Just before lunchtime in America, the lights will be dimming in Mumbai, Amman and Dubai. And by early afternoon in New York, it will be lights out in Paris, Istanbul, London and Copenhagen.”

Can you imagine places that you would never dream of going dark participating in such an event? During Earth Hour you’ll find The European Union Headquarters in Brussels, St. Peter’s Basilica in Vatican City, Bird’s Nest Olympic Stadium in Beijing, Washington, D.C, The Pyramids in Egypt, the Acropolis in Athens, the Broadway Theater District, the Space Needle in Seattle, and the Chrysler Building will all go dark for Earth Hour.

Read the Earth Hour Mission: “For the first time in history, people of all ages, nationalities, race and background have the opportunity to use their light switch as their vote – Switching off your lights is a vote for Earth, or leaving them on is a vote for global warming. WWF are urging the world to VOTE EARTH and reach the target of 1 billion votes, which will be presented to world leaders at the Global Climate Change Conference in Copenhagen 2009.

This meeting will determine official government policies to take action against global warming, which will replace the Kyoto Protocol. It is the chance for the people of the world to make their voice heard. We all have a vote, and every single vote counts. Together we can take control of the future of our planet, for future generations.”

VOTE EARTH by simply switching off your lights for one hour, and join the world for Earth Hour – Saturday, March 28, 8:30-9:30pm.

With much love to all of those who took the time to care and spread the word. Special thanks to Kim B. for all of her hard work in promoting Earth Hour!

Redoubt Re-ignites

An ash cloud looms in the distance near Kachemak Bay Bluffs. Credit: Steve Baird, AVO

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Alaska’s Mount Redoubt erupted twice Thursday morning, creating a 12-mile-high cloud of ash. The Alaska Volcano Observatory reported the first eruption came about 8:30 a.m., sending an ash cloud more than 9,100 meters (30,000) feet in the air. A second eruption came about an hour later, and blasted ash 20,000 meters (65,000 feet) high. After the second eruption, mud flows called lahars near the base of the volcano ran into the nearby Drift River. The National Weather Service also issued a flash flood warning for regions surrounding the Drift River, as eruptions can cause snow and ice to melt, causing the river to swell with melt water. The ash is predicted to drift as far as Anchorage, which lies about 160 km (100 miles) northeast of the volcano.

Redoubt ash plume. NASA images created by Jesse Allen, using data provided courtesy of the MODIS Rapid Response team
Redoubt ash plume. NASA images created by Jesse Allen, using data provided courtesy of the MODIS Rapid Response team

The volcano erupted with five smaller blasts on Monday, but had been relatively quiet for the past two days. Since the earlier eruptions occurred during the night, satellite images were not available during the peak times of eruptions, but scientists are hoping satellites were able to capture the latest eruptions in action.

Airlines have canceled flights around the area, as ash poses a significant threat to aircraft engines. Some regions surrounding Mount Redoubt have been evacuated.

Geologists with the U.S. Geological Survey have said a lot of snow and ice remains on the mountain, increasing the danger from mud flows that already have downed hundreds of trees and carved a huge gouge out of a glacier.

AVO, NASA Earth Observatory, Yahoo News

Former Astronaut To Take Social Media to New Heights

Scott Parazynski during his attempt to climb Mt. Everest. Credit: OnOrbit.com

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In 2008, astronaut Scott Parazynski came within 24 hours of reaching the summit of Mt. Everest when a painful back injury forced him to abandon his climb. Now, Parazynski is on his way back for another attempt at summitting the world’s highest mountain peak. But this time, he wants to take the rest of the world with him. If everything works as planned, Parazynski will blog, podcast, vodcast and more during the climb, and he even wants to Twitter from the summit. “I want to tell the story of exploration here on Earth and the corollaries it has with space exploration,” Parazynski told Universe Today before he left for Kathmandu, Nepal. “They are both very hostile, unforgiving environments that require a lot of training, a lot of gear, and a lot of thought. The intent is to share the story with as many people as we can, particularly young people.” Parazynski and his team have even agreed to take questions from readers of Universe Today and answer them during their climb.

Mt. Everest mosaic.  Credit: OnOrbit.com
Mt. Everest mosaic. Credit: OnOrbit.com

Parazynski has teamed up with the Challenger Centers for Space Science Education and the Boy Scouts of America to offer educational activities in association with his trek, and is working with various scientists to do field science along the way.

“We’ll be collecting data for astrobiologists, looking for extremophile life,” Parazynski said. “If you understand how extremophiles live, you might be able to understand how life may have once evolved on Mars, or may still exist on Mars.”

As an astronaut, Parazynski was part of 5 space shuttle missions; his last mission to the International Space Station included a daring repair of the ISS’s solar panels.

Parazynski during an EVA. Credit: NASA
Parazynski during an EVA. Credit: NASA

Parazynski will also be testing some NASA-derived hardware, taking along a prototype lunar geology camera and other hardware for extreme environments. “Up high on the mountain there are limestone formations, which are wonderful places to look for fossilized life,” he said,” and we’ll also look for melt water and primitive forms of life there; algae lichens, etc. If liquid water exists even for brief periods on Mars it may be in similar conditions to what we’ll find on Mt. Everest. We hope to bring samples back for scientists to look at.”

To help Parazynski, he has enlisted the help of a couple of “media sherpas;” Keith Cowing from NASAWatch and Miles O’Brien, former CNN correspondent. Cowing will definitely be at the base camp, coordinating the media blitz, while O’Brien is still working out his schedule, but hopes to be there as well.

“Scott has the chance to something interesting and wants to share it with as many people as possible,” said Cowing. “This is participatory exploration, where we’ll bring as many people as possible to where we’re going. This is enabled by high end internet connection capable of streaming video. The idea is to open up a vista of participation to a very large audience.”

Cowing said they will have access to email to answer as many questions as possible, and Universe Today will be one of the venues supplying questions from readers. “We’ll be Twittering, videocasting, podcasting, Skyping, emailing, SMSing, blogging , you name it. We’re using every gizmo we’ve got and every avenue of interaction with people, giving them the opportunity to see what it’s like to live in a tent at 17,600 feet.”

The entire expedition will take between 6 -10 weeks, depending on the weather and health of the climbers. Parazyski said it will take several weeks just for the climbers’ bodies to acclimate to the decreased amount of oxygen at those heights. The peak of Mount Everest is 8,848 meters (29,028 feet) above sea level. “We’ll be going up and down to get body used to the conditions,” he said. “Essentially what happens, you need to increase your body’s oxygen carrying capacity, and grow more red blood cells. Your blood chemistry changes to enable you to exchange oxygen more efficiently and that just takes time.” Parazynski, an MD, will be the official physician for the group.

Map of Nepal.  Credit: OnOrbit.com
Map of Nepal. Credit: OnOrbit.com

The Discovery Channel will also be part of the climb, with hopes of creating a documentary of the expedition for their “Everest: Beyond the Limits” series. Cameras will be mounted on the climbers to take video of the experience.

Parazynski is part of a team of 23 climbers. Another team will also be part of the climb, and there will be an additional 20 or 30 climbers to help create the documentary.

The climb officially starts in early May. You can follow the climb via OnOrbit.com/Everest. Parazynski’s whereabouts can also be followed on Google Earth, via his SPOT, a GPS location and message device, which is a commercial sponsor of the climb. The expedition is completely privately funded.

Parazynski is now a “former” NASA astronaut. He announced two weeks ago that he left NASA to work in private industry, at Wyle Labs in Houston. “I had a wonderful experience in the role of astronaut, but now it’s time to pursue other opportunities.”

One other hope for this expedition is to have people participating both on this Earth and off. “If the stars align and everything works just right, we hope to have a satellite phone call between our group and the Hubble repair space shuttle mission,” Parazynski said. Of course, that would depend on if the Hubble mission launches during Parazynski’s climb.

Despite Parazynski’s wish to share his experience with the world, he admits there’s also a strong personal element to this climb. “I went almost the entire way last year and came within 24 hours of summitting,” he said. “It is something I’ve thought of and dreamt about every day since I left the mountain last May, wondering what that last 24 hours will be like, and what it will be like to complete one of the great aspirationa of my entire life.”

Follow OnOrbit.com/Everest for complete coverage. You can follow Parazynski’s Twitter feed, too, SPOTScott, and the OnOrbit Everest Twitter feed. We’ll post regular updates here on Universe Today, along with reminders to submit questions for Parazynski, Cowing and O’Brien by posting your questions in the comments section.

Ozone Success Story: NASA Video of Enviro Action That Worked

Ozone layer hole. Image credit: NASA
Ozone layer hole. Image credit: NASA

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Imagine the year 2065. Two-thirds of Earth’s ozone is gone. The infamous ozone hole over Antarctica is a year-round fixture with a twin over the North Pole. People living in mid-latitude cities like Washington, D.C., get sunburned after five minutes. DNA-mutating UV radiation is up 650 percent, with likely harmful effects on plants, animals and human skin cancer rates.

Such is the world we would have inherited if 193 nations had not agreed to ban ozone-depleting substances, according to atmospheric chemists at NASA, Johns Hopkins University in Baltimore and the Netherlands Environmental Assessment Agency in Bilthoven. The researchers have unveiled new computer simulations this week of a worldwide disaster that humans managed to avoid.

In retrospect, the researchers say, the Montreal Protocol was a “remarkable international agreement that should be studied by those involved with global warming and the attempts to reach international agreement on that topic.”

ozone-simulation
This time series from the ozone "World Avoided" model shows the concentration of ozone over the South Pole at four key times. Reds represent normal to high concentrations; blues show depleted areas. Credit: NASA Goddard's Scientific Visualization Studio

Ozone is Earth’s natural sunscreen, absorbing and blocking most of the incoming UV radiation from the sun and protecting life from DNA-damaging radiation. The gas is naturally created and replenished by a photochemical reaction in the upper atmosphere where UV rays break oxygen molecules into individual atoms that then recombine into three-part molecules (O3). As it is moved around the globe by upper level winds, ozone is slowly depleted by naturally occurring atmospheric gases. It is a system in natural balance.

But chlorofluorocarbons — invented in 1928 as refrigerants and as inert carriers for chemical sprays — upset that balance. Researchers discovered in the 1970s and 1980s that while CFCs are inert at Earth’s surface, they are quite reactive in the stratosphere (10 to 50 kilometers altitude, or 6 to 31 miles), where roughly 90 percent of the planet’s ozone accumulates. UV radiation causes CFCs and similar bromine compounds in the stratosphere to break up into elemental chlorine and bromine that readily destroy ozone molecules. 

In the 1980s, ozone-depleting substances opened a wintertime “hole” over Antarctica and opened the eyes of the world to the effects of human activity on the atmosphere.  In January 1989, the Montreal Protocol went into force, the first-ever international agreement on regulation of chemical pollutants.

In the new study, published online in the journal Atmospheric Chemistry and Physics, Goddard scientist Paul Newman and his team simulated “what might have been” if chlorofluorocarbons (CFCs) and similar chemicals were not banned. The simulation used a comprehensive model that included atmospheric chemical effects, wind changes, and radiation changes. The “World avoided” video can be viewed here in Quicktime (for more formats, go here).

By the simulated year 2020, 17 percent of all ozone is depleted globally. An ozone hole starts to form each year over the Arctic, which was once a place of prodigious ozone levels.

By 2040, global ozone concentrations fall below the same levels that currently comprise the “hole” over Antarctica. The UV index in mid-latitude cities reaches 15 around noon on a clear summer day, giving a perceptible sunburn in about 10 minutes. Over Antarctica, the ozone hole becomes a year-round fixture.

By the end of the model run in 2065, global ozone drops 67 percent compared to 1970s levels. The intensity of UV radiation at Earth’s surface doubles; at certain shorter wavelengths, intensity rises by as much as 10,000 times. Skin cancer-causing radiation soars.

“Our world avoided calculation goes a little beyond what I thought would happen,” said Goddard scientist and study co-author Richard Stolarski, who was among the pioneers of atmospheric ozone chemistry in the 1970s. “The quantities may not be absolutely correct, but the basic results clearly indicate what could have happened to the atmosphere.”

“We simulated a world avoided,” added Newman, “and it’s a world we should be glad we avoided.”

As it is, production of ozone-depleting substances was mostly halted about 15 years ago, though their abundance is only beginning to decline because the chemicals can reside in the atmosphere for 50 to 100 years. The peak abundance of CFCs in the atmosphere occurred around 2000, and has decreased by roughly 4 percent to date. Stratospheric ozone was depleted by 5 to 6 percent at middle latitudes, but has somewhat rebounded in recent years.

Vernal Equinox – Busting the Myth of Balancing Eggs

Season Diagram courtesy of NOAA

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Spring officially arrives for everyone, including astronomers on March 20. The word “Equinox” literally means “equal night”. It’s all about the balance of light – not the myth of balancing eggs. On the universal date (UTC) of Friday, March 20, 2009 at 11:44 (am) both the day and night are the same length. But what’s so special about it? It’s a date that most of us recognize as symbolic of changing seasons. North of Earth’s equator we welcome Spring, while people south of the equator are gearing up for the cooler temperatures of Autumn. But what’s all this about balancing eggs?

These all too brief, but monumental moments in Earth-time, owe their significance to the slightly more than 23 degree tilt of the Earth’s axis. Because of our planetary angle, we in the northern hemisphere receive the Sun’s rays most directly during the Summer. In the Winter, when we are tilted away from the Sun, the rays pass through the atmosphere at a greater slant, bringing lower temperatures. If the Earth rotated on an axis perpendicular to the plane of the Earth’s orbit around the Sun, there would be no variation in day lengths or temperatures throughout the year, and we would not have seasons. At Equinox, the midway between these two times in Spring and Autumn, the spin axis of the Earth points 90 degrees away from the Sun.

analemma_vr_bigIf your head is spinning from all of this, sit and ponder for a moment. Now is a great time to choose a marker and observe what’s happening for yourself. Trying a real science experiment for equinox is much better than the myth of balancing eggs. Just place a stake of some type into the ground (or use a fencepost or signpost) and periodically over the next few weeks measure the length of the shadow when the Sun is at its highest and write down your measurements. I use my south facing deck railing and mark its shadow on the deck boards in chalk. It won’t take long before your marker’s shadow length changes and you notice how the Sun’s position changes in the sky, and with it the ecliptic plane.

In the language of astronomy, an equinox is either of two points on the celestial sphere where the ecliptic and the celestial equator intersect. The Vernal Equinox is also known as “the first point of Aries” – a the point at which the Sun appears to cross the celestial equator from south to north. This is also the the zero point of longitude – the reference plane at which right ascension is defined as 0. Believe it or not, this was defined in 1950 as the northern vernal equinox, but it has moved to the constellation of Pisces now! Why? The equinoxes are not fixed points on the celestial sphere but move westward along the ecliptic, passing through all the constellations of the zodiac in 26,000 years. This is what’s known as the precession of the equinoxes – a motion first noted by Hipparchus roughly in 120 B.C. But what causes it?

full-526px-earth_precessionsvgThe precession is caused the gravitational attraction of both the Moon and Sun on the equatorial bulge of the Earth. Imagine the Earth’s axis patterning itself in a cone as it moves, like a spinning top. As a result, the celestial equator, which lies in the plane of the Earth’s equator, moves on the celestial sphere, while the ecliptic, which lies in the plane of the Earth’s orbit around the Sun, is not affected by this motion. The equinoxes, which lie at the intersections of the celestial equator and the ecliptic, now move on the celestial sphere. Much the same, the celestial poles move in circles on the celestial sphere, so that there is a continual change in the star at or near one of these poles.

After a period of about 26,000 years the equinoxes and poles lie once again at nearly the same points on the celestial sphere. Because the gravitational effects of the Sun and Moon aren’t always the same, there is some wobble in the motion of the Earth’s axis called nutation. This wobble causes the celestial poles to move, not in perfect circles, but in a series of S-shaped curves with a period of 18.6 years that was first explained by Isaac Newton in 1687.

So where did the urban myth of balance eggs on vernal equinox come from? Probably because at one time Easter was celebrated at this time and eggs play a very big role in the whole Esotere, rebirth, and cultural symbolism of this holiday. It may very well have been the good folks in China who orginally began the myth by patiently practicing standing eggs on end during vernal equinox to symbolize the restoration of balance to the world after a season of darkness. If this symbol of fertility could be balanced on such a day of significance, then surely nature was in harmony!

Go ahead and balance eggs for fun… But believe in science.

P.S. The Bad Astronomer Phil Plait has a tutorial video on his website, teaching you how to stand an egg on end, any time of the year. Click here to watch it.

Many thanks to Vasilij Rumyantsev (Crimean Astrophysical Obsevatory) for the excellent solar analemma as it appeared in the July 9, 2002 APOD.

Indian Balloon Experiment Nets Three New Bacteria

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Indian scientists flying a giant balloon experiment have announced the discovery of three new species of bacteria from the stratosphere.

In all, 12 bacterial and six fungal colonies were detected, nine of which, based on gene sequencing, showed greater than 98 percent similarity with reported known species on earth. Three bacterial colonies, however, represented totally new species. All three boast significantly higher UV resistance compared to their nearest phylogenetic neighbors on Earth.

The experiment was conducted using a balloon that measures 26.7 million cubic feet  (756,059 cubic meters) carrying 1,000 pounds (459 kg) of scientific payload soaked in liquid Neon. It was flown from the National Balloon Facility in Hyderabad, operated by the Tata Institute of Fundamental Research (TIFR). 

An onboard cryosampler contained sixteen evacuated and sterilized stainless steel probes. Throughout the flight, the probes remained immersed in liquid Neon to create a cryopump effect. The cylinders, after collecting air samples from different heights ranging from 20 km to 41 km (12 to 25 miles) above the Earth’s surface, were parachuted down and retrieved. The samples were analyzed by scientists at the Center for Cellular and Molecular Biology in Hyderabad as well as the National Center for Cell Science in Pune for independent confirmation.

One of the new species has been named as Janibacter hoylei, after the astrophysicist Fred Hoyle, the second as Bacillus isronensis recognizing the contribution of ISRO in the balloon experiments which led to its discovery, and the third as Bacillus aryabhata after India’s celebrated ancient astronomer Aryabhata (also the name of ISRO’s first satellite).

The researchers have pointed out in a press release that precautionary measures and controls operating in the experiment inspire confidence that the new species were picked up in the stratosphere.

“While the present study does not conclusively establish the extra-terrestrial origin of microorganisms, it does provide positive encouragement to continue the work in our quest to explore the origin of life,” they added.

This was the second such experiment conducted by ISRO, with the first one in 2001. Even though the first experiment had yielded positive results, the researchers decided to repeat the experiment while exercising extra care to ensure that it was totally free from any terrestrial contamination.

Source: Indian Space Research Organisation

Additional links: Center for Cellular and Molecular BiologyNational Center for Cell Science, Tata Institute of Fundamental Research