aads

Bacteria in a beetle makes it a leaf-eater

The tortoise beetle, which eats thistle leaves, has evolved a symbiotic relationship with bacteria that allows it to have such a specialized diet. Photo by Hassan Salem.

By Carol Clark

A leaf-eating beetle has evolved a symbiotic relationship with bacteria that allows the insect to break down pectin — part of a plant’s cell wall that is indigestible to most animals.

The journal Cell published the findings on the novel function of the bacterium, which has a surprisingly tiny genome — much smaller than previous reports on the minimum size required for an organism not subsisting within a host cell.

“This insect is a leaf eater largely because of these bacteria,” says Hassan Salem, lead author of the study and a post-doctoral fellow in Emory University’s Department of Biology. “And the bacteria have actually become developmentally integrated into the insect’s body.”

Two organs alongside the foregut of the beetle Cassida rubiginosa house the bacteria and appear to have no other function than to maintain these microbes. “The organs are equivalent to the liver in humans, in the sense that they contain the tools to break down and process food,” Salem says.

The newly characterized bacterium has only 270,000 DNA base pairs in its genome, compared to the millions that are more typical for bacterial strains. That makes its genome closer to that of intracellular bacteria and organelles than to free-living microbes. Mitochondria, for example, the organelles that regulate metabolism within cells, have 100,000 base pairs.

The two symbiotic organs of the tortoise beetle, dyed a fluorescent green, are shown on either side of the insect's foregut. Microscopy image by Hassan Salem.

Salem is a researcher in the lab of Emory biologist Nicole Gerardo, an associate professor who specializes in the evolutionary ecology of insect-microbe interactions. The lab combines genomic and experimental approaches to learn how both beneficial and harmful microbes establish and maintain relationships with their hosts.

A human gut holds about 10,000 species of bacteria. These microbial communities, which can be genetically characterized as microbiomes, are transferred generationally but are also dynamic and respond to environmental changes. The microbiome of an urbanite, for example, has different characteristics from that of a hunter-gatherer.

Unlike humans, insects tend to have specialized feeding ecologies. They offer simple models to study symbiotic relationships between microbes and their hosts.

Salem with Buchner's book
Salem became fascinated by Cassida rubiginosa, more commonly known as the tortoise beetle, while he was a graduate student at the Max Planck Institute for Chemical Ecology in Jena, Germany. He was leafing through a 1953 edition of a book by the late Paul Buchner, a German scientist and one of the pioneers of systematic symbiosis research in insects. Buchner referenced a paper published in 1936 by one of his students, Hans-Jurgen Stammer, on Cassida rubiginosa.

“Stammer wrote that, unlike most leaf-eating beetles that he had studied, this one had sac-like organs that he had never seen before and the organs were filled with micro-organisms,” says Salem, who looked up Stammer’s original paper in a now-obscure journal. “He didn’t have the high-powered microscopes that we have now, or genome sequencing technology, so he wasn’t able to comment on the functionality of the mysterious microbes. At that point, the idea that microbes could do anything beneficial for an animal was mushy science.”

Intrigued by the article, Salem went to a nearby woodland to collect some of the leaf beetles. “To find these beetles, you don’t go looking for them,” he explains. “You go looking for the plants they eat.”

The tortoise beetle feeds on the tough, spiny leaves of the Californian thistle (Asteraceae). This prolific weed grows throughout much of the world and is difficult to control. “It pops up in a lot of areas where sheep are maintained,” Salem says. “In fact, it’s a huge pest to New Zealand sheep farmers. The more thistles covering a farmland, the less food the sheep have to eat and the lower the yield. But the thistle is hard to get rid of because its roots run so deep.”

Salem followed the trail of his curiosity to New Zealand, spending time with an agricultural researcher, Michael Cripps, who breeds the tortoise beetle as a bio-control model for thistles. “You drop 100 beetles on a thistle plant and the insects will just drain the plant metabolically until it dies,” Salem explains.

As an herbivore that specializes in eating leaves, the tortoise beetle must consume large amounts of plant cell walls, made of hard-to-digest materials like pectin. One of nature’s most complex polysaccharides, pectin is a gelatinous substance that gives plant cell walls their shape and rigidity. While it was unclear how the beetle obtained needed nutrients of amino acids and vitamins from such a diet, Salem suspected that symbiotic bacteria played a role.

In this cross-section of the symbiotic organ the bacteria it contains are lit up in fluorescent green dye. Microscopy image by Hassan Salem.

When he joined the Gerado lab at Emory, Salem continued to study the tortoise beetle and its micro-organisms with the help of fellow post-doc Aileen Berasategui, a co-author of the Cell paper.

They used genome sequencing technology to characterize the microorganisms as a new species of bacterium. Despite its tiny genome, the bacterium has the power to degrade pectin.

“Just as an apex predator has claws and strong mandibles to obtain the nutritional value that it needs from its prey, the bacterium has pectin-digesting genes that enable the beetle host to deconstruct a plant cell,” Salem says.

After the bacterium breaks down the pectin, the beetle’s digestive system can then access all of the amino acids and vitamins within the plant’s cells for its nutrients.

Salem christened the new bacterium Candidatus Stammera capleta, after Hans-Jurgen Stammer, the ecologist who first glimpsed it and wondered about it more than 80 years ago.

“The most amazing thing to me is that we made this discovery because I read a really old book,” Salem says. “It speaks to the importance of natural history collections and libraries for old journals. We truly stand on the shoulders of giants, extending the work of those who came before us.”

Additional co-authors of the paper are from the Max Planck Institute for Chemical Ecology, the University of Luxembourg, the Lincoln Research Centre in New Zealand, Johannes Gutenberg University in Germany and the National Institute for Advanced Industrial Science and Technology in Japan.

Related:
Tiny aphids hold big surprises in the genome
Farming ants reveal evolution secrets

from eScienceCommons http://ift.tt/2jvq6hT
The tortoise beetle, which eats thistle leaves, has evolved a symbiotic relationship with bacteria that allows it to have such a specialized diet. Photo by Hassan Salem.

By Carol Clark

A leaf-eating beetle has evolved a symbiotic relationship with bacteria that allows the insect to break down pectin — part of a plant’s cell wall that is indigestible to most animals.

The journal Cell published the findings on the novel function of the bacterium, which has a surprisingly tiny genome — much smaller than previous reports on the minimum size required for an organism not subsisting within a host cell.

“This insect is a leaf eater largely because of these bacteria,” says Hassan Salem, lead author of the study and a post-doctoral fellow in Emory University’s Department of Biology. “And the bacteria have actually become developmentally integrated into the insect’s body.”

Two organs alongside the foregut of the beetle Cassida rubiginosa house the bacteria and appear to have no other function than to maintain these microbes. “The organs are equivalent to the liver in humans, in the sense that they contain the tools to break down and process food,” Salem says.

The newly characterized bacterium has only 270,000 DNA base pairs in its genome, compared to the millions that are more typical for bacterial strains. That makes its genome closer to that of intracellular bacteria and organelles than to free-living microbes. Mitochondria, for example, the organelles that regulate metabolism within cells, have 100,000 base pairs.

The two symbiotic organs of the tortoise beetle, dyed a fluorescent green, are shown on either side of the insect's foregut. Microscopy image by Hassan Salem.

Salem is a researcher in the lab of Emory biologist Nicole Gerardo, an associate professor who specializes in the evolutionary ecology of insect-microbe interactions. The lab combines genomic and experimental approaches to learn how both beneficial and harmful microbes establish and maintain relationships with their hosts.

A human gut holds about 10,000 species of bacteria. These microbial communities, which can be genetically characterized as microbiomes, are transferred generationally but are also dynamic and respond to environmental changes. The microbiome of an urbanite, for example, has different characteristics from that of a hunter-gatherer.

Unlike humans, insects tend to have specialized feeding ecologies. They offer simple models to study symbiotic relationships between microbes and their hosts.

Salem with Buchner's book
Salem became fascinated by Cassida rubiginosa, more commonly known as the tortoise beetle, while he was a graduate student at the Max Planck Institute for Chemical Ecology in Jena, Germany. He was leafing through a 1953 edition of a book by the late Paul Buchner, a German scientist and one of the pioneers of systematic symbiosis research in insects. Buchner referenced a paper published in 1936 by one of his students, Hans-Jurgen Stammer, on Cassida rubiginosa.

“Stammer wrote that, unlike most leaf-eating beetles that he had studied, this one had sac-like organs that he had never seen before and the organs were filled with micro-organisms,” says Salem, who looked up Stammer’s original paper in a now-obscure journal. “He didn’t have the high-powered microscopes that we have now, or genome sequencing technology, so he wasn’t able to comment on the functionality of the mysterious microbes. At that point, the idea that microbes could do anything beneficial for an animal was mushy science.”

Intrigued by the article, Salem went to a nearby woodland to collect some of the leaf beetles. “To find these beetles, you don’t go looking for them,” he explains. “You go looking for the plants they eat.”

The tortoise beetle feeds on the tough, spiny leaves of the Californian thistle (Asteraceae). This prolific weed grows throughout much of the world and is difficult to control. “It pops up in a lot of areas where sheep are maintained,” Salem says. “In fact, it’s a huge pest to New Zealand sheep farmers. The more thistles covering a farmland, the less food the sheep have to eat and the lower the yield. But the thistle is hard to get rid of because its roots run so deep.”

Salem followed the trail of his curiosity to New Zealand, spending time with an agricultural researcher, Michael Cripps, who breeds the tortoise beetle as a bio-control model for thistles. “You drop 100 beetles on a thistle plant and the insects will just drain the plant metabolically until it dies,” Salem explains.

As an herbivore that specializes in eating leaves, the tortoise beetle must consume large amounts of plant cell walls, made of hard-to-digest materials like pectin. One of nature’s most complex polysaccharides, pectin is a gelatinous substance that gives plant cell walls their shape and rigidity. While it was unclear how the beetle obtained needed nutrients of amino acids and vitamins from such a diet, Salem suspected that symbiotic bacteria played a role.

In this cross-section of the symbiotic organ the bacteria it contains are lit up in fluorescent green dye. Microscopy image by Hassan Salem.

When he joined the Gerado lab at Emory, Salem continued to study the tortoise beetle and its micro-organisms with the help of fellow post-doc Aileen Berasategui, a co-author of the Cell paper.

They used genome sequencing technology to characterize the microorganisms as a new species of bacterium. Despite its tiny genome, the bacterium has the power to degrade pectin.

“Just as an apex predator has claws and strong mandibles to obtain the nutritional value that it needs from its prey, the bacterium has pectin-digesting genes that enable the beetle host to deconstruct a plant cell,” Salem says.

After the bacterium breaks down the pectin, the beetle’s digestive system can then access all of the amino acids and vitamins within the plant’s cells for its nutrients.

Salem christened the new bacterium Candidatus Stammera capleta, after Hans-Jurgen Stammer, the ecologist who first glimpsed it and wondered about it more than 80 years ago.

“The most amazing thing to me is that we made this discovery because I read a really old book,” Salem says. “It speaks to the importance of natural history collections and libraries for old journals. We truly stand on the shoulders of giants, extending the work of those who came before us.”

Additional co-authors of the paper are from the Max Planck Institute for Chemical Ecology, the University of Luxembourg, the Lincoln Research Centre in New Zealand, Johannes Gutenberg University in Germany and the National Institute for Advanced Industrial Science and Technology in Japan.

Related:
Tiny aphids hold big surprises in the genome
Farming ants reveal evolution secrets

from eScienceCommons http://ift.tt/2jvq6hT

Four decades of Vilspa

As part of ESA’s strategy to foster commercial competitiveness in Europe while focusing on its core aims, the agency has transferred ownership of several ground tracking stations for reuse by external organisations.

By the end of 2017, ESA will have transferred three stations to national organisations in Spain and Portugal, who will take over the provision of satellite tracking services to a wide variety of commercial customers.

The three stations involved in the transfer are all equipped with 15 m-diameter dish antennas, suitable for supporting near-Earth missions, and are located in Spain, at Maspalomas and at ESA’s space astronomy centre near Madrid, and in Perth, Western Australia.

The new operators will be able to use the stations to offer tracking services on a commercial basis to customers worldwide, which also includes ESA, leaving the Agency free to focus on meeting the demanding technical requirements of its deep-space stations, in Spain, Argentina and Australia, and on operation of a select group of four other stations.

ESA’s Lionel Hernandez, current Cebreros station manager and former manager for the ESAC antenna, provided some background on the station’s history.

On 1 September 2017, ESA’s VIL-2 antenna and its supporting facilities was formally retired after 36 years’ service supporting some of Europe’s most ambitious and successful missions.

Villafranca tracking station 1977 Credit: ESA

Villafranca tracking station 1977 Credit: ESA

ESAC was inaugurated in May 1975 as the Vilspa station and has been responsible for providing telemetry, tracking and command support to not only ESA satellites but also to several agencies like NOAA, NASA, DLR (The German Aerospace Centre), the Chinese National Space Administration (CNSA) and to intergovernmental organisations such as Eumetsat.

It also supported missions flown by entities that later became private companies including Eutelsat, a French-based satellite communications provider and the UK’s Inmarsat plc (formerly INMARSAT), both leaders in global mobile satellite communications.

The station, now an ESA Establishment, continues to host the Science Operation Centres of almost all of ESA’s scientific missions.

From the early days of the International Ultraviolet Explorer (IUE) mission, the work now performed at ESAC continues to reach into the depths of space and across the electromagnetic spectrum; providing scientific data to the world.

What began as one of Europe’s first links to the stars has become the heart of European space science.

Satellites/missions supported by the Vilspa ground station

IUE, OTS-2, GOES-1, Marecs-A, Exosat, ECS-1, Marecs-B2, ECS-2, ECS-4,ECS-5, Olympus, Hipparcos, Giotto, Italsat-F1, ERS-1, Meteosat-4 (MOP-1), Meteosat-5 (MOP-2), Meteosat-6 (MOP-3), Meteosat-7(MOP-4), ISO, ERS-2, Italsat-F2, SOHO, XMM-Newton, Cluster ESA’s four-satellites flotilla, Envisat, Eutelsat-W3, MSG-1, Integral, SMART-1, Double Star Programme (TC-1 and TC-2 satellites) belonging to China National Space Administration, Bird, Meteosat-9 (MSG-2), ASTRA´s four Atlantic satellites fleet, MetOp-A and MetOp-B.

It has also supported Jules Verne (ATV-1), Johannes Kepler (ATV-2), Edoardo Amaldi (ATV-3), Albert Einstein (ATV-4), Georges Lemaitre (ATV-5) and the International Space Station (ISS).

 



from Rocket Science http://ift.tt/2ATMhSX
v

As part of ESA’s strategy to foster commercial competitiveness in Europe while focusing on its core aims, the agency has transferred ownership of several ground tracking stations for reuse by external organisations.

By the end of 2017, ESA will have transferred three stations to national organisations in Spain and Portugal, who will take over the provision of satellite tracking services to a wide variety of commercial customers.

The three stations involved in the transfer are all equipped with 15 m-diameter dish antennas, suitable for supporting near-Earth missions, and are located in Spain, at Maspalomas and at ESA’s space astronomy centre near Madrid, and in Perth, Western Australia.

The new operators will be able to use the stations to offer tracking services on a commercial basis to customers worldwide, which also includes ESA, leaving the Agency free to focus on meeting the demanding technical requirements of its deep-space stations, in Spain, Argentina and Australia, and on operation of a select group of four other stations.

ESA’s Lionel Hernandez, current Cebreros station manager and former manager for the ESAC antenna, provided some background on the station’s history.

On 1 September 2017, ESA’s VIL-2 antenna and its supporting facilities was formally retired after 36 years’ service supporting some of Europe’s most ambitious and successful missions.

Villafranca tracking station 1977 Credit: ESA

Villafranca tracking station 1977 Credit: ESA

ESAC was inaugurated in May 1975 as the Vilspa station and has been responsible for providing telemetry, tracking and command support to not only ESA satellites but also to several agencies like NOAA, NASA, DLR (The German Aerospace Centre), the Chinese National Space Administration (CNSA) and to intergovernmental organisations such as Eumetsat.

It also supported missions flown by entities that later became private companies including Eutelsat, a French-based satellite communications provider and the UK’s Inmarsat plc (formerly INMARSAT), both leaders in global mobile satellite communications.

The station, now an ESA Establishment, continues to host the Science Operation Centres of almost all of ESA’s scientific missions.

From the early days of the International Ultraviolet Explorer (IUE) mission, the work now performed at ESAC continues to reach into the depths of space and across the electromagnetic spectrum; providing scientific data to the world.

What began as one of Europe’s first links to the stars has become the heart of European space science.

Satellites/missions supported by the Vilspa ground station

IUE, OTS-2, GOES-1, Marecs-A, Exosat, ECS-1, Marecs-B2, ECS-2, ECS-4,ECS-5, Olympus, Hipparcos, Giotto, Italsat-F1, ERS-1, Meteosat-4 (MOP-1), Meteosat-5 (MOP-2), Meteosat-6 (MOP-3), Meteosat-7(MOP-4), ISO, ERS-2, Italsat-F2, SOHO, XMM-Newton, Cluster ESA’s four-satellites flotilla, Envisat, Eutelsat-W3, MSG-1, Integral, SMART-1, Double Star Programme (TC-1 and TC-2 satellites) belonging to China National Space Administration, Bird, Meteosat-9 (MSG-2), ASTRA´s four Atlantic satellites fleet, MetOp-A and MetOp-B.

It has also supported Jules Verne (ATV-1), Johannes Kepler (ATV-2), Edoardo Amaldi (ATV-3), Albert Einstein (ATV-4), Georges Lemaitre (ATV-5) and the International Space Station (ISS).

 



from Rocket Science http://ift.tt/2ATMhSX
v

Crossing Phobos

Editor’s note: Today’s update comes from ESA’s Armelle Hubault, a spacecraft operations engineer working on the ExoMars/TGO team at ESOC. The news? ESA’s ExoMars/TGO orbiter – now conducting a year-long aerobraking campaign at Mars – crossed the orbit of Phobos today (spoiler alert: we avoided a collision!), marking a notable milestone in progress toward attaining its final, ca. 400-km altitude circular science orbit.

While photographing Mars, NASA’s Hubble Space Telescope captured a cameo appearance of the tiny moon Phobos on its trek around the Red Planet. Discovered in 1877, the diminutive, potato-shaped moon is so small that it appears star-like in the Hubble pictures. Phobos orbits Mars in just 7 hours and 39 minutes, which is faster than Mars rotates. The moon’s orbit is very slowly shrinking, meaning it will eventually shatter under Mars’ gravitational pull, or crash onto the planet. Hubble took 13 separate exposures over 22 minutes to create a time-lapse video showing the moon’s orbital path. Credit: NASA, ESA and Z. Levay (STScI) Acknowledgment: J. Bell (ASU) and M. Wolff (Space Science Institute)

Phobos seen by Hubble: While photographing Mars, The ESA/NASA Hubble Space Telescope captured a cameo appearance of the tiny moon Phobos on its trek around the Red Planet (click on image for full details). Credit: NASA/ESA/Z. Levay (STScI) – Acknowledgment: J. Bell (ASU) & M. Wolff (Space Science Institute)

Armelle wrote:

Here are the facts about the Phobos orbit crossing today.

The orbit crossing is not a Phobos flyby. In fact, we did our best to ensure that Phobos would be at the farthest possible point away from TGO when we cross the moon’s orbit. The moon will basically be on the other side of Mars when our spacecraft crosses its orbit [Editor: Phobos will be 9320 km from the centre of Mars for the first crossing]. 

This results in two crossings today: one around 14:30 UT and a second at 20:00 UT (15:30 and 21:00 CET, respectively). On each crossing of Phobos’ orbit, TGO will ‘miss’ the Phobos orbit by 23 km (and 120 minutes) and 10 km (and 200 minutes), respectively.

Visualisation of the ExoMars Trace Gas Orbiter aerobraking at Mars. With aerobraking, the spacecraft's solar array experiences tiny amounts of drag owing to the wisps of martian atmosphere at very high altitudes, which slows the craft and lowers its orbit. Credit: ESA/ATG medialab

Visualisation of the ExoMars Trace Gas Orbiter aerobraking at Mars. With aerobraking, the spacecraft’s solar array experiences tiny amounts of drag owing to the wisps of martian atmosphere at very high altitudes, which slows the craft and lowers its orbit. Credit: ESA/ATG medialab

Note that the diameter of Phobos is about 20 km, so these passes by the orbit are very, very close!

Over the last few days, we adapted the phase of our orbit to ensure maximum ‘outphasing’ of Phobos and TGO, so today there is actually nothing for the flight control team to do but watch and monitor. 

The crossing is taking place around apocentre (point of farthest approach to Mars); remember that our pericentre (point of closest approach) remains on the order of 100 km from the martian surface, actually in the atmosphere, which is how we are obtaining the aerobraking effect. 



from Rocket Science http://ift.tt/2yPHHne
v

Editor’s note: Today’s update comes from ESA’s Armelle Hubault, a spacecraft operations engineer working on the ExoMars/TGO team at ESOC. The news? ESA’s ExoMars/TGO orbiter – now conducting a year-long aerobraking campaign at Mars – crossed the orbit of Phobos today (spoiler alert: we avoided a collision!), marking a notable milestone in progress toward attaining its final, ca. 400-km altitude circular science orbit.

While photographing Mars, NASA’s Hubble Space Telescope captured a cameo appearance of the tiny moon Phobos on its trek around the Red Planet. Discovered in 1877, the diminutive, potato-shaped moon is so small that it appears star-like in the Hubble pictures. Phobos orbits Mars in just 7 hours and 39 minutes, which is faster than Mars rotates. The moon’s orbit is very slowly shrinking, meaning it will eventually shatter under Mars’ gravitational pull, or crash onto the planet. Hubble took 13 separate exposures over 22 minutes to create a time-lapse video showing the moon’s orbital path. Credit: NASA, ESA and Z. Levay (STScI) Acknowledgment: J. Bell (ASU) and M. Wolff (Space Science Institute)

Phobos seen by Hubble: While photographing Mars, The ESA/NASA Hubble Space Telescope captured a cameo appearance of the tiny moon Phobos on its trek around the Red Planet (click on image for full details). Credit: NASA/ESA/Z. Levay (STScI) – Acknowledgment: J. Bell (ASU) & M. Wolff (Space Science Institute)

Armelle wrote:

Here are the facts about the Phobos orbit crossing today.

The orbit crossing is not a Phobos flyby. In fact, we did our best to ensure that Phobos would be at the farthest possible point away from TGO when we cross the moon’s orbit. The moon will basically be on the other side of Mars when our spacecraft crosses its orbit [Editor: Phobos will be 9320 km from the centre of Mars for the first crossing]. 

This results in two crossings today: one around 14:30 UT and a second at 20:00 UT (15:30 and 21:00 CET, respectively). On each crossing of Phobos’ orbit, TGO will ‘miss’ the Phobos orbit by 23 km (and 120 minutes) and 10 km (and 200 minutes), respectively.

Visualisation of the ExoMars Trace Gas Orbiter aerobraking at Mars. With aerobraking, the spacecraft's solar array experiences tiny amounts of drag owing to the wisps of martian atmosphere at very high altitudes, which slows the craft and lowers its orbit. Credit: ESA/ATG medialab

Visualisation of the ExoMars Trace Gas Orbiter aerobraking at Mars. With aerobraking, the spacecraft’s solar array experiences tiny amounts of drag owing to the wisps of martian atmosphere at very high altitudes, which slows the craft and lowers its orbit. Credit: ESA/ATG medialab

Note that the diameter of Phobos is about 20 km, so these passes by the orbit are very, very close!

Over the last few days, we adapted the phase of our orbit to ensure maximum ‘outphasing’ of Phobos and TGO, so today there is actually nothing for the flight control team to do but watch and monitor. 

The crossing is taking place around apocentre (point of farthest approach to Mars); remember that our pericentre (point of closest approach) remains on the order of 100 km from the martian surface, actually in the atmosphere, which is how we are obtaining the aerobraking effect. 



from Rocket Science http://ift.tt/2yPHHne
v

Battlefield Acupuncture Reduces Opioid Dependence, Returns Airmen to Flight

The Air Force is using alternative medicine to reduce opioid dependence and get airmen back to work.

from http://ift.tt/2zF67nb
The Air Force is using alternative medicine to reduce opioid dependence and get airmen back to work.

from http://ift.tt/2zF67nb

Scientists warn: Soon it will be too late to save Earth

A letter to all of us, signed by more than 15,000 scientists (and counting) in 184 countries, warns that human well-being will be severely jeopardized by continuing trends in environmental harm, including our changing climate, deforestation, loss of access to fresh water, species extinctions and human population growth.

Entitled World Scientists’ Warning to Humanity: A Second Notice, it was published in the international journal Bioscience on November 13, 2017.

In 1992, more than 1,700 scientists signed a World Scientists’ Warning to Humanity published by the Union of Concerned Scientists. But global trends have worsened since 1992, the authors wrote in the new letter. In the last 25 years, trends in nine environmental issues suggest that humanity is continuing to risk its future.

Read the letter here.

The scientists wrote:

Soon it will be too late to shift course away from our failing trajectory, and time is running out. We must recognize, in our day-to-day lives and in our governing institutions, that Earth with all its life is our only home.

The letter also says …

By failing to adequately limit population growth, reassess the role of an economy rooted in growth, reduce greenhouse gases, incentivize renewable energy, protect habitat, restore ecosystems, curb pollution, halt defaunation, and constrain invasive alien species, humanity is not taking the urgent steps needed to safeguard our imperiled biosphere.

The article was written by an international team led by William Ripple of Oregon State University led the international team of scientists who created the letter. Ripple said in a statement:

Some people might be tempted to dismiss this evidence and think we are just being alarmist. Scientists are in the business of analyzing data and looking at the long-term consequences. Those who signed this second warning aren’t just raising a false alarm. They are acknowledging the obvious signs that we are heading down an unsustainable path. We are hoping that our paper will ignite a wide-spread public debate about the global environment and climate.

Progress in some areas — such as a reduction in ozone-depleting chemicals and an increase in energy generated from renewable sources — shows that positive changes can be made, the authors wrote. There has been a rapid decline in fertility rates in some regions, which can be attributed to investments in education for women, they added. The rate of deforestation in some regions has also slowed.

The warning came with steps that can be taken to reverse negative trends, but the authors suggested that it may take a groundswell of public pressure to convince political leaders to take the right corrective actions. Such activities could include establishing more terrestrial and marine reserves, strengthening enforcement of anti-poaching laws and restraints on wildlife trade, expanding family planning and educational programs for women, promoting a dietary shift toward plant-based foods and massively adopting renewable energy and other “green” technologies.

Scientists who did not sign the warning prior to publication can endorse the published warning here.

Bottom line: A letter entitled World Scientists’ Warning to Humanity: A Second Notice, urging the world to address major environmental concerns. was signed by more than 15,000 scientists in 184 countries.

Read more from Oregon State University



from EarthSky http://ift.tt/2hzcWMl

A letter to all of us, signed by more than 15,000 scientists (and counting) in 184 countries, warns that human well-being will be severely jeopardized by continuing trends in environmental harm, including our changing climate, deforestation, loss of access to fresh water, species extinctions and human population growth.

Entitled World Scientists’ Warning to Humanity: A Second Notice, it was published in the international journal Bioscience on November 13, 2017.

In 1992, more than 1,700 scientists signed a World Scientists’ Warning to Humanity published by the Union of Concerned Scientists. But global trends have worsened since 1992, the authors wrote in the new letter. In the last 25 years, trends in nine environmental issues suggest that humanity is continuing to risk its future.

Read the letter here.

The scientists wrote:

Soon it will be too late to shift course away from our failing trajectory, and time is running out. We must recognize, in our day-to-day lives and in our governing institutions, that Earth with all its life is our only home.

The letter also says …

By failing to adequately limit population growth, reassess the role of an economy rooted in growth, reduce greenhouse gases, incentivize renewable energy, protect habitat, restore ecosystems, curb pollution, halt defaunation, and constrain invasive alien species, humanity is not taking the urgent steps needed to safeguard our imperiled biosphere.

The article was written by an international team led by William Ripple of Oregon State University led the international team of scientists who created the letter. Ripple said in a statement:

Some people might be tempted to dismiss this evidence and think we are just being alarmist. Scientists are in the business of analyzing data and looking at the long-term consequences. Those who signed this second warning aren’t just raising a false alarm. They are acknowledging the obvious signs that we are heading down an unsustainable path. We are hoping that our paper will ignite a wide-spread public debate about the global environment and climate.

Progress in some areas — such as a reduction in ozone-depleting chemicals and an increase in energy generated from renewable sources — shows that positive changes can be made, the authors wrote. There has been a rapid decline in fertility rates in some regions, which can be attributed to investments in education for women, they added. The rate of deforestation in some regions has also slowed.

The warning came with steps that can be taken to reverse negative trends, but the authors suggested that it may take a groundswell of public pressure to convince political leaders to take the right corrective actions. Such activities could include establishing more terrestrial and marine reserves, strengthening enforcement of anti-poaching laws and restraints on wildlife trade, expanding family planning and educational programs for women, promoting a dietary shift toward plant-based foods and massively adopting renewable energy and other “green” technologies.

Scientists who did not sign the warning prior to publication can endorse the published warning here.

Bottom line: A letter entitled World Scientists’ Warning to Humanity: A Second Notice, urging the world to address major environmental concerns. was signed by more than 15,000 scientists in 184 countries.

Read more from Oregon State University



from EarthSky http://ift.tt/2hzcWMl

Today in science: 1st intentional radio message to space

Aerial view of Arecibo Observatory via Wiki Commons

Arecibo Radio Telescope in Puerto Rico, used in 1974 to broadcast the 1st intentional radio signal into space. Image via Wikimedia Commons.

November 16, 1974. This is the anniversary of the most powerful broadcast ever deliberately beamed into space with the intention of contacting alien life. The broadcast formed part of the ceremonies held to mark a major upgrade to the Arecibo Radio Telescope in Puerto Rico. Some applauded this event as a mind-expanding attempt to remind people in 1974 that Earth is likely not the only planet where an intelligent civilization has evolved. At the time, others expressed concern. They felt we shouldn’t be attempting to reveal Earth’s location in space to unknown alien civilizations.

The broadcast itself was simple, and elegant. It consisted of a pattern of binary numbers. This message contained information about the basic chemicals of life, the structure of DNA, Earth’s place in our solar system and even a stick figure of a human. The actual message is below.

The Arecibo message as sent 1974 from the Arecibo Observatory. Via Wikimedia Commons.

The Arecibo message as sent 1974 from the Arecibo Observatory. Via Wikimedia Commons. Click here for an explanation of each part of the message.

It took three minutes to send 1,679 bits of information – a snail’s pace compared to modern computer modems. According to the SETI Institute:

The broadcast was particularly powerful because it used Arecibo’s megawatt transmitter attached to its 305 meter antenna. The latter concentrates the transmitter energy by beaming it into a very small patch of sky. The emission was equivalent to a 20 trillion watt omnidirectional broadcast, and would be detectable by a SETI experiment just about anywhere in the galaxy, assuming a receiving antenna similar in size to Arecibo’s.

The 1974 signal went out in the direction of M13, a globular star cluster orbiting the center of our Milky Way galaxy. It was chosen mainly because it’s a large collection of stars, that was available in the sky at the time and place of the ceremony

Global star clusters are very far away. M13 is about 23,000 light-years from Earth.

The 1974 signal is 39 light-years from us today.

Bottom line: The first radio signal intentionally sent to space with the idea of contacting alien life was beamed outward from the Arecibo radio telescope in Puerto Rico on November 16, 1974. What do you think? Should we be advertising our presence in space?



from EarthSky http://ift.tt/1ObJh5k
Aerial view of Arecibo Observatory via Wiki Commons

Arecibo Radio Telescope in Puerto Rico, used in 1974 to broadcast the 1st intentional radio signal into space. Image via Wikimedia Commons.

November 16, 1974. This is the anniversary of the most powerful broadcast ever deliberately beamed into space with the intention of contacting alien life. The broadcast formed part of the ceremonies held to mark a major upgrade to the Arecibo Radio Telescope in Puerto Rico. Some applauded this event as a mind-expanding attempt to remind people in 1974 that Earth is likely not the only planet where an intelligent civilization has evolved. At the time, others expressed concern. They felt we shouldn’t be attempting to reveal Earth’s location in space to unknown alien civilizations.

The broadcast itself was simple, and elegant. It consisted of a pattern of binary numbers. This message contained information about the basic chemicals of life, the structure of DNA, Earth’s place in our solar system and even a stick figure of a human. The actual message is below.

The Arecibo message as sent 1974 from the Arecibo Observatory. Via Wikimedia Commons.

The Arecibo message as sent 1974 from the Arecibo Observatory. Via Wikimedia Commons. Click here for an explanation of each part of the message.

It took three minutes to send 1,679 bits of information – a snail’s pace compared to modern computer modems. According to the SETI Institute:

The broadcast was particularly powerful because it used Arecibo’s megawatt transmitter attached to its 305 meter antenna. The latter concentrates the transmitter energy by beaming it into a very small patch of sky. The emission was equivalent to a 20 trillion watt omnidirectional broadcast, and would be detectable by a SETI experiment just about anywhere in the galaxy, assuming a receiving antenna similar in size to Arecibo’s.

The 1974 signal went out in the direction of M13, a globular star cluster orbiting the center of our Milky Way galaxy. It was chosen mainly because it’s a large collection of stars, that was available in the sky at the time and place of the ceremony

Global star clusters are very far away. M13 is about 23,000 light-years from Earth.

The 1974 signal is 39 light-years from us today.

Bottom line: The first radio signal intentionally sent to space with the idea of contacting alien life was beamed outward from the Arecibo radio telescope in Puerto Rico on November 16, 1974. What do you think? Should we be advertising our presence in space?



from EarthSky http://ift.tt/1ObJh5k

Platform reflecting

Image via John Entwistle.

John Entwistle captured this image of a wooden platform with great blue heron perched on the corner, reflecting in the glassy water on a foggy morning at the Manasquan Reservoir, New Jersey.



from EarthSky http://ift.tt/2yOifOY

Image via John Entwistle.

John Entwistle captured this image of a wooden platform with great blue heron perched on the corner, reflecting in the glassy water on a foggy morning at the Manasquan Reservoir, New Jersey.



from EarthSky http://ift.tt/2yOifOY

adds 2