aads

Mercury/Mars conjunction before sunrise

Want to see the super-close conjunction of the planets Mercury and Mars before sunrise on September 16, 2017? If you live in the Northern Hemisphere, you have a good chance of seeing the close-knit planetary twosome tomorrow morning. Get up at least 90 minutes before sunrise and look eastward (in the direction of sunrise). If it’s at all clear, you simply can’t miss the waning crescent moon and the dazzling planet Venus, the brightest and second-brightest celestial bodies, respectively, in the predawn sky. The moon and Venus help guide you to Mercury and Mars.

As darkness starts to give way to dawn, look for Mercury and Mars near the horizon, more or less on line with the moon and Venus. Given a level and unobstructed eastern horizon, you might see the two embracing worlds climbing into the sky 80 or so minutes before sunrise. Binoculars could come in handy!

The Northern Hemisphere has the big advantage. At mid-northern latitudes, Mercury and Mars rise around 90 minutes before the sun; but at temperate latitudes in the Southern Hemisphere, these two worlds only rise about 45 minutes before sunrise. But no matter where you live worldwide, an imaginary line from the moon through Venus points in the general direction of Mercury and Mars. Click here for recomended almanacs; they can help you find out the rising times of these planets in your sky.

Mercury and Mars will still be close together on the sky’s dome as the waning crescent moon swings close to them in a few more days.

Be mindful that the modestly-bright star a short hop below Venus is not Mercury or Mars. That’s Regulus, the brightest star in the constellation Leo the Lion. Although considered a 1st-magnitude star, Regulus pales next to Venus, which outshines Regulus by a solid hundredfold. If you can still see Regulus in the encroaching morning twilight, you can draw an imaginary line from Venus through Regulus to find Mercury and Mars’s spot near the horizon.

If you only see one starlike point of light, it’ll probably be Mercury. Mercury is quite bright, shining a good ten times more brilliantly than the rather faint planet Mars. In fact, you may need to aim binoculars (or a low-powered telescope) at Mercury to spot Mars taking stage with Mercury in the same binocular (or telescopic) field of view.

At conjunction, Mercury and Mars will only be 0.06o apart – the equivalent of about 1/8th the moon’s apparent diameter. The conjunction on September 16, 2017 features the closest conjunction of two planets since January 1, 2017. Also, a closer planetary conjunction won’t happen again until December 7, 2018. So enjoy the grand pairing of Mercury and Mars while the time is at hand.

Keep an eye on the morning sky after tomorrow’s planetary conjunction. Watch for Venus to sink downward day by day, toward Regulus and Mars. And watch for Mars to climb upward day by day, away from Mercury and toward Venus. Venus will pair up with Regulus on September 19, 2017, and then Mars will couple up with Venus on October 5, 2017.

Mario Pereira in Felgueiras, Portugal caught bright Venus – and much fainter Mercury and Mars – on the morning of September 12, 2017. The star Regulus in the constellation Leo also lies along this line.

Bottom line: No matter where you live worldwide, an imaginary line from the moon through brilliant Venus – in the east before dawn – points in the general direction of Mercury and Mars on September 16, 2017.



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

Want to see the super-close conjunction of the planets Mercury and Mars before sunrise on September 16, 2017? If you live in the Northern Hemisphere, you have a good chance of seeing the close-knit planetary twosome tomorrow morning. Get up at least 90 minutes before sunrise and look eastward (in the direction of sunrise). If it’s at all clear, you simply can’t miss the waning crescent moon and the dazzling planet Venus, the brightest and second-brightest celestial bodies, respectively, in the predawn sky. The moon and Venus help guide you to Mercury and Mars.

As darkness starts to give way to dawn, look for Mercury and Mars near the horizon, more or less on line with the moon and Venus. Given a level and unobstructed eastern horizon, you might see the two embracing worlds climbing into the sky 80 or so minutes before sunrise. Binoculars could come in handy!

The Northern Hemisphere has the big advantage. At mid-northern latitudes, Mercury and Mars rise around 90 minutes before the sun; but at temperate latitudes in the Southern Hemisphere, these two worlds only rise about 45 minutes before sunrise. But no matter where you live worldwide, an imaginary line from the moon through Venus points in the general direction of Mercury and Mars. Click here for recomended almanacs; they can help you find out the rising times of these planets in your sky.

Mercury and Mars will still be close together on the sky’s dome as the waning crescent moon swings close to them in a few more days.

Be mindful that the modestly-bright star a short hop below Venus is not Mercury or Mars. That’s Regulus, the brightest star in the constellation Leo the Lion. Although considered a 1st-magnitude star, Regulus pales next to Venus, which outshines Regulus by a solid hundredfold. If you can still see Regulus in the encroaching morning twilight, you can draw an imaginary line from Venus through Regulus to find Mercury and Mars’s spot near the horizon.

If you only see one starlike point of light, it’ll probably be Mercury. Mercury is quite bright, shining a good ten times more brilliantly than the rather faint planet Mars. In fact, you may need to aim binoculars (or a low-powered telescope) at Mercury to spot Mars taking stage with Mercury in the same binocular (or telescopic) field of view.

At conjunction, Mercury and Mars will only be 0.06o apart – the equivalent of about 1/8th the moon’s apparent diameter. The conjunction on September 16, 2017 features the closest conjunction of two planets since January 1, 2017. Also, a closer planetary conjunction won’t happen again until December 7, 2018. So enjoy the grand pairing of Mercury and Mars while the time is at hand.

Keep an eye on the morning sky after tomorrow’s planetary conjunction. Watch for Venus to sink downward day by day, toward Regulus and Mars. And watch for Mars to climb upward day by day, away from Mercury and toward Venus. Venus will pair up with Regulus on September 19, 2017, and then Mars will couple up with Venus on October 5, 2017.

Mario Pereira in Felgueiras, Portugal caught bright Venus – and much fainter Mercury and Mars – on the morning of September 12, 2017. The star Regulus in the constellation Leo also lies along this line.

Bottom line: No matter where you live worldwide, an imaginary line from the moon through brilliant Venus – in the east before dawn – points in the general direction of Mercury and Mars on September 16, 2017.



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

Reflections at the end of Cassini

On 25 December 2004, after a seven-year journey as part of the international NASA/ESA/ASI Cassini-Huygens mission to Saturn, ESA’s Huygens lander separated from NASA’s Cassini orbiter to make a lonely’, one-way voyage to Titan, Saturn’s largest moon.

On 14 January 2005, as the world watched breathlessly, Huygens plunged into Titan’s atmosphere, deployed parachutes and then spent a leisurely two-and-a-half hours descending to the surface, transmitting science data the entire time, which were relayed by Cassini back to NASA’s 70m deep-space network on Earth.

At 13:34 CET, that day, Titan time, Huygens landed with a bounce and confirmation was received at ESA’s ESOC mission control centre, Darmstadt, Germany, with the first data signals arriving at 17:19 CET. The probe continued transmitting data from the surface, even after Cassini had orbited out of view below Titan’s horizon. Huygens’ touchdown marked just the second time a moon was ever landed upon, and is still today the most distant landing ever made by an artificial object.

Titan is the largest of Saturn’s moons and is one of the most compelling destinations in our Solar System. Its 1000-km-thick atmosphere – many times thicker than Earth’s – comprises primarily nitrogen and methane, and the moon’s frigid, -180ºC surface features mountain ranges, methane seas, coastline estuaries and a complex mix of organic matter.

On that day at ESOC, ESA’s Huygens Spacecraft Operations Manager Claudio Sollazzo was on console in the Main Control Room, watching intently as the signals came in via Cassini. He had returned to ESOC just a few days earlier, after spending four years working as part of the Cassini mission team at NASA/JPL in California. For the better part of two decades, his job had been to ensure that Huygens was ready for its epic mission, and he was ESA’s point man for Huygens, first in Europe and later on the ground at JPL, as the Cassini mission went through numerous stages of proposals, approvals, US and European funding negotiations, threats of cancellation and – ultimately – launch on 15 October 1997.

After Huygens, Claudio too up duties at ESA’s Columbus Control Centre near Munich, and he continued working with many US and European colleagues as a Mission Director for European astronauts on the ISS. In 2015, he retired from ESA, but not from space flight! Today, he is working at Johnson Space Center in Houston as the Italian space agency (ASI) representative Mission Manager for ESA astronaut Paolo Nespoli, now on the ISS for his five-month VITA mission.

Claudio agreed to share some of his impressions of Cassini-Huygens, as the Cassini orbiter’s historic mission comes to an end tomorrow, on 15 September.

Huygens Spacecraft Operations Manager Claudio Sollazzo at ESOC on 14 January 2005. Credit: ESA/J. Mai

Huygens Spacecraft Operations Manager Claudio Sollazzo at ESOC on 14 January 2005. Credit: ESA/J. Mai

Cassini-Huygens was a huge part of my personal and professional life. My children were very small when I began working on the mission, and today they are all grown adults. They had just finished high school when Huygens landed on Titan!

I am sad to see Cassini finally end, but fuel is getting low and I am nonetheless very happy that, like Huygens itself, it has delivered so much incredible data from the Saturn system – including numerous flybys of Titan, where my little Huygens sits now, eternally frozen a billion km away.

I must say, I suffered a lot when the landing was complete. Yes, it was an epic triumph, and European and US scientists received a great deal of data from Huygens. But my professional life had been dedicated to the probe and with its mission complete, I was at a loss for what to do. Happily, I was able to shift my professional focus and move to ESA’s Columbus Control Centre in Oberpfaffenhofen, near Munich, where I could spend another decade working with many colleagues from Europe, NASA and the ISS partners.

If I have to think of my strongest memory of Huygens now, it’s not just the mission, or the scientific data, or the triumph of landing on a moon of Saturn. More importantly, I have very strong memories of working for many years with colleagues at ESA and at NASA – especially at JPL.

I am Italian, from Europe, and for me there was a bit of a culture shock when I moved to Pasadena. But I eventually got used to the American way and later I was struck by how deep our collaboration became. Make no mistake about it, once the Americans know you are competent, that you know your business and that you are trustworthy – they trust you; they accept you as one of their own.

Now, I am working at Johnson Space Center in Houston on Paolo Nespoli’s mission on the ISS, and I see the same deep collaboration – perhaps even more so.  I thoroughly enjoy working with the US colleagues: even today, after decades of work with NASA, our cultures may be different, but I and my European colleagues work well with the Americans; we solve problems and we get the job done. 

Cassini and Huygens have been scientific, engineering and technical triumphs. But more importantly, they have shown that we humans can work together across cultures and other barriers, and I hope this inspires others to do the same in the future.

 



from Rocket Science http://ift.tt/2js0bar
v

On 25 December 2004, after a seven-year journey as part of the international NASA/ESA/ASI Cassini-Huygens mission to Saturn, ESA’s Huygens lander separated from NASA’s Cassini orbiter to make a lonely’, one-way voyage to Titan, Saturn’s largest moon.

On 14 January 2005, as the world watched breathlessly, Huygens plunged into Titan’s atmosphere, deployed parachutes and then spent a leisurely two-and-a-half hours descending to the surface, transmitting science data the entire time, which were relayed by Cassini back to NASA’s 70m deep-space network on Earth.

At 13:34 CET, that day, Titan time, Huygens landed with a bounce and confirmation was received at ESA’s ESOC mission control centre, Darmstadt, Germany, with the first data signals arriving at 17:19 CET. The probe continued transmitting data from the surface, even after Cassini had orbited out of view below Titan’s horizon. Huygens’ touchdown marked just the second time a moon was ever landed upon, and is still today the most distant landing ever made by an artificial object.

Titan is the largest of Saturn’s moons and is one of the most compelling destinations in our Solar System. Its 1000-km-thick atmosphere – many times thicker than Earth’s – comprises primarily nitrogen and methane, and the moon’s frigid, -180ºC surface features mountain ranges, methane seas, coastline estuaries and a complex mix of organic matter.

On that day at ESOC, ESA’s Huygens Spacecraft Operations Manager Claudio Sollazzo was on console in the Main Control Room, watching intently as the signals came in via Cassini. He had returned to ESOC just a few days earlier, after spending four years working as part of the Cassini mission team at NASA/JPL in California. For the better part of two decades, his job had been to ensure that Huygens was ready for its epic mission, and he was ESA’s point man for Huygens, first in Europe and later on the ground at JPL, as the Cassini mission went through numerous stages of proposals, approvals, US and European funding negotiations, threats of cancellation and – ultimately – launch on 15 October 1997.

After Huygens, Claudio too up duties at ESA’s Columbus Control Centre near Munich, and he continued working with many US and European colleagues as a Mission Director for European astronauts on the ISS. In 2015, he retired from ESA, but not from space flight! Today, he is working at Johnson Space Center in Houston as the Italian space agency (ASI) representative Mission Manager for ESA astronaut Paolo Nespoli, now on the ISS for his five-month VITA mission.

Claudio agreed to share some of his impressions of Cassini-Huygens, as the Cassini orbiter’s historic mission comes to an end tomorrow, on 15 September.

Huygens Spacecraft Operations Manager Claudio Sollazzo at ESOC on 14 January 2005. Credit: ESA/J. Mai

Huygens Spacecraft Operations Manager Claudio Sollazzo at ESOC on 14 January 2005. Credit: ESA/J. Mai

Cassini-Huygens was a huge part of my personal and professional life. My children were very small when I began working on the mission, and today they are all grown adults. They had just finished high school when Huygens landed on Titan!

I am sad to see Cassini finally end, but fuel is getting low and I am nonetheless very happy that, like Huygens itself, it has delivered so much incredible data from the Saturn system – including numerous flybys of Titan, where my little Huygens sits now, eternally frozen a billion km away.

I must say, I suffered a lot when the landing was complete. Yes, it was an epic triumph, and European and US scientists received a great deal of data from Huygens. But my professional life had been dedicated to the probe and with its mission complete, I was at a loss for what to do. Happily, I was able to shift my professional focus and move to ESA’s Columbus Control Centre in Oberpfaffenhofen, near Munich, where I could spend another decade working with many colleagues from Europe, NASA and the ISS partners.

If I have to think of my strongest memory of Huygens now, it’s not just the mission, or the scientific data, or the triumph of landing on a moon of Saturn. More importantly, I have very strong memories of working for many years with colleagues at ESA and at NASA – especially at JPL.

I am Italian, from Europe, and for me there was a bit of a culture shock when I moved to Pasadena. But I eventually got used to the American way and later I was struck by how deep our collaboration became. Make no mistake about it, once the Americans know you are competent, that you know your business and that you are trustworthy – they trust you; they accept you as one of their own.

Now, I am working at Johnson Space Center in Houston on Paolo Nespoli’s mission on the ISS, and I see the same deep collaboration – perhaps even more so.  I thoroughly enjoy working with the US colleagues: even today, after decades of work with NASA, our cultures may be different, but I and my European colleagues work well with the Americans; we solve problems and we get the job done. 

Cassini and Huygens have been scientific, engineering and technical triumphs. But more importantly, they have shown that we humans can work together across cultures and other barriers, and I hope this inspires others to do the same in the future.

 



from Rocket Science http://ift.tt/2js0bar
v

Army Finds New Ways to Destroy Old Ammo

The Army is pioneering new ways to get rid of obsolete munitions and turn them into something local communities can use.

from http://ift.tt/2h3NBcO
The Army is pioneering new ways to get rid of obsolete munitions and turn them into something local communities can use.

from http://ift.tt/2h3NBcO

Juno sees Jupiter up-close and personal

View larger | Image via NASA/JPL-Caltech/SwRI/MSSS/ Gerald Eichstädt/Sean Doran.

NASA’s Juno spacecraft captured this series of images during its eighth close flyby of gas giant planet Jupiter on September 1, 2017.

See image larger here

When the spacecraft’s JunoCam snapped the images during the 8-minute flyby, Juno ranged from 7,545 to 14,234 miles (12,143 to 22,908 kilometers) from the tops of the Jupiter’s clouds, at a latitude range of -28.5406 to -44.4912 degrees.

Points of Interest include:

Dalmatian Zone/Eye of Odin
Dark Eye/STB Ghost East End
Coolest Place on Jupiter
Renslow/Hurricane Rachel

The final image in the series on the right shows Jupiter’s south pole coming into view.

Juno began orbiting the giant planet on July 4, 2016.

JunoCam’s raw images are available for the public to peruse and process into image products here.

Bottom line: A series of images of Jupiter taken by the Juno spacecraft on September 1, 2017.

Read more from NASA



from EarthSky http://ift.tt/2h4wIPn

View larger | Image via NASA/JPL-Caltech/SwRI/MSSS/ Gerald Eichstädt/Sean Doran.

NASA’s Juno spacecraft captured this series of images during its eighth close flyby of gas giant planet Jupiter on September 1, 2017.

See image larger here

When the spacecraft’s JunoCam snapped the images during the 8-minute flyby, Juno ranged from 7,545 to 14,234 miles (12,143 to 22,908 kilometers) from the tops of the Jupiter’s clouds, at a latitude range of -28.5406 to -44.4912 degrees.

Points of Interest include:

Dalmatian Zone/Eye of Odin
Dark Eye/STB Ghost East End
Coolest Place on Jupiter
Renslow/Hurricane Rachel

The final image in the series on the right shows Jupiter’s south pole coming into view.

Juno began orbiting the giant planet on July 4, 2016.

JunoCam’s raw images are available for the public to peruse and process into image products here.

Bottom line: A series of images of Jupiter taken by the Juno spacecraft on September 1, 2017.

Read more from NASA



from EarthSky http://ift.tt/2h4wIPn

Natural selection happening now in humans, say scientists

As genes are favored or phased out, human evolution continues. Image via ktsdesign/Shutterstock.com

By Hakhamanesh Mostafavi, Columbia University; Joe Pickrell, Columbia University, and Molly Przeworski, Columbia University

Human evolution can seem like a phenomenon of the distant past which applies only to our ancestors living millions of years ago. But human evolution is ongoing. To evolve simply means that mutations – the accidental changes to genes that happen normally in the process of copying DNA – are becoming more or less common in the population over time.

These changes can happen by chance, because the individuals who reproduced happened to carry a particular mutation somewhat more often than individuals who didn’t have children. They can also happen because of natural selection, when carriers of a specific mutation are better able to survive, reproduce or tend to their family members – and therefore leave more descendants. Every biological adaptation, from the ability of humans to walk upright on two feet to flight in birds, ultimately traces back to natural selection acting on these minute changes, generation after generation.

So humans are definitely still evolving. The question is whether we are still adapting: Are individuals who carry harmful mutations living less long, reproducing less – ultimately leaving fewer descendants? For instance, terrible eyesight may have been a major survival disadvantage living on the savanna, but with glasses and laser surgery, it’s unlikely to prevent people from living a long life today. How commonly then are mutations under selection in contemporary humans?

Long time scale makes evolution hard to study

Because adaptations involve tiny changes in the frequencies of mutations from generation to generation and their fortune plays out over tens to hundreds of thousands of years, they are incredibly hard to study directly – at least in long-lived organisms such as people.

So while there is overwhelming evidence for human evolution and unequivocal footprints of adaptation in the genome, rarely have scientists been able to directly observe natural selection operating in people. As a result, biologists still understand very little about the workings of natural selection in humans.

Indeed, one of the clearest footprints of a past adaptation in the human genome involves a mutation that permits milk to be digested in adulthood. This mutation in the lactase gene rapidly rose in frequency with the rise of dairy farming thousands of years ago, independently in multiple populations. It’s the reason some people can drink milk as adults, whereas most remain lactose intolerant.

But even in this well-studied case, let alone for the rest of the genome, researchers don’t know whether the mutation was beneficial for survival or for reproduction; whether the benefits were the same for both sexes, or across all ages; or whether the benefit depended on the environment (for instance, availability of other food sources). As pointed out by evolutionary biologist Richard Lewontin in the 1960s, to learn these properties of natural selection would require a massive study, in which genetic and genealogical information is obtained for hundreds of thousands of people.

Fifty years later, our group realized that this thought experiment is starting to become feasible. We sought large biomedical data sets that would let us learn about mutations that affect survival.

Looking at gene frequency across age groups

Our basic idea was that mutations that lower the chance of survival should be present at lower frequency in older individuals. For example, if a mutation becomes harmful at the age of 60 years, people who carry it have a lower chance to survive past 60 – and the mutation should be less common among those who live longer than that.

We therefore looked for mutations that change in frequency with age among around 60,000 individuals from California (part of the GERA cohort) and around 150,000 from the U.K. Biobank. To avoid the complication that people whose ancestors lived in different places carry a somewhat different set of mutations, we focused on the largest group with shared ancestry within each study.

Across the genome, we found two variants that endanger survival. The first is a variant of the APOE gene, which is a well-known risk factor for Alzheimer’s disease. It drops in frequency beyond age 70. The second harmful variant we found is a mutation in the CHRNA3 gene. Associated with heavy smoking, this inherited mutation starts to decrease in frequency at middle age in men, because carriers of this mutation are less likely to survive longer.

People who carry a variant of the APOE gene die at a higher rate and are less common among the old age categories. Image via Mostafavi et al, PLOS Biology

Both deleterious variants only had an effect long after the typical ages of reproduction for both females and males. Biologists usually consider such mutations to not be under selection. After all, by late middle age, most people have already passed their genes on to whatever offspring they’ll have, so it seems like it might not matter how long they live beyond that point.

Why then would we only find two, when our study was large enough to detect any such variant, if common in the population? One possibility is that mutations that only imperil survival so late in life almost never arise. While that is possible, the genome is a large place, so that seems unlikely.

The other intriguing possibility is that natural selection prevents even late-acting variants from becoming common in the population by natural selection, if they have large enough effects. Why might that be? For one, men can father children in old age. Even if only a tiny fraction of them do so, it may be enough of an evolutionary fitness cost for selection to act on. Survival beyond the age of reproduction could also be beneficial for the survival of related individuals who carry the same mutations, most directly children. In other words, surviving past typical reproductive ages may be beneficial for humans after all.

Smokers who carry a mutation in the CHRNA3 gene tend to smoke more cigarettes per day and so are more exposed to harmful effects of smoking. Image via NeONBRAND on Unsplash

Your mutations do influence your survival

In addition to examining one mutation at a time, we were also interested in considering sets of mutations that have all been shown to influence the same trait, and might have very subtle effects on survival individually. For example, researchers have identified approximately 700 common mutations that influence height, each contributing only millimeters. To this end, we considered tens to hundreds of mutations that shape variation in one of 42 traits.

We found genetic mutations linked to a number of diseases and metabolic traits that decrease survival rates: individuals who are genetically predisposed to have higher total cholesterol, LDL cholesterol, risk of heart disease, BMI, risk of asthma or lower HDL cholesterol tend to die younger than others.

Perhaps more surprisingly, we discovered that people who carry mutations that delay puberty or the age at which they have their first child tend to live longer. It was known from epidemiological studies that early puberty is associated with adverse effects later in life such as cancer and obesity. Our results indicate some of that effect is probably due to heritable factors.

The ConversationSo humans carry common mutations that affect their survival and natural selection appears to act on at least a subset, in some contemporary environments. But what is bad in one context may well not be in another; as one example, the CHRNA3 variant has an effect because people smoke. These are early days, however, and our findings offer only a first glimpse of what can soon be gleaned from millions of genomes, in combination with genealogical records. In future work, it will be important to study not only lifespan, but also the number of children and grandchildren individuals leave, as well as populations and environments worldwide.

Hakhamanesh Mostafavi, Ph.D. Student in Biological Sciences, Columbia University; Joe Pickrell, Adjunct Assistant Professor of Biological Sciences, Columbia University, and Molly Przeworski, Professor of Biological Sciences, Columbia University

Bottom line: Comparing genomes of more than 200,000 people, researchers identified genetic variants that are less common in older people, suggesting natural selection continues to weed out disadvantageous traits.

This article was originally published on The Conversation. Read the original article.



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

As genes are favored or phased out, human evolution continues. Image via ktsdesign/Shutterstock.com

By Hakhamanesh Mostafavi, Columbia University; Joe Pickrell, Columbia University, and Molly Przeworski, Columbia University

Human evolution can seem like a phenomenon of the distant past which applies only to our ancestors living millions of years ago. But human evolution is ongoing. To evolve simply means that mutations – the accidental changes to genes that happen normally in the process of copying DNA – are becoming more or less common in the population over time.

These changes can happen by chance, because the individuals who reproduced happened to carry a particular mutation somewhat more often than individuals who didn’t have children. They can also happen because of natural selection, when carriers of a specific mutation are better able to survive, reproduce or tend to their family members – and therefore leave more descendants. Every biological adaptation, from the ability of humans to walk upright on two feet to flight in birds, ultimately traces back to natural selection acting on these minute changes, generation after generation.

So humans are definitely still evolving. The question is whether we are still adapting: Are individuals who carry harmful mutations living less long, reproducing less – ultimately leaving fewer descendants? For instance, terrible eyesight may have been a major survival disadvantage living on the savanna, but with glasses and laser surgery, it’s unlikely to prevent people from living a long life today. How commonly then are mutations under selection in contemporary humans?

Long time scale makes evolution hard to study

Because adaptations involve tiny changes in the frequencies of mutations from generation to generation and their fortune plays out over tens to hundreds of thousands of years, they are incredibly hard to study directly – at least in long-lived organisms such as people.

So while there is overwhelming evidence for human evolution and unequivocal footprints of adaptation in the genome, rarely have scientists been able to directly observe natural selection operating in people. As a result, biologists still understand very little about the workings of natural selection in humans.

Indeed, one of the clearest footprints of a past adaptation in the human genome involves a mutation that permits milk to be digested in adulthood. This mutation in the lactase gene rapidly rose in frequency with the rise of dairy farming thousands of years ago, independently in multiple populations. It’s the reason some people can drink milk as adults, whereas most remain lactose intolerant.

But even in this well-studied case, let alone for the rest of the genome, researchers don’t know whether the mutation was beneficial for survival or for reproduction; whether the benefits were the same for both sexes, or across all ages; or whether the benefit depended on the environment (for instance, availability of other food sources). As pointed out by evolutionary biologist Richard Lewontin in the 1960s, to learn these properties of natural selection would require a massive study, in which genetic and genealogical information is obtained for hundreds of thousands of people.

Fifty years later, our group realized that this thought experiment is starting to become feasible. We sought large biomedical data sets that would let us learn about mutations that affect survival.

Looking at gene frequency across age groups

Our basic idea was that mutations that lower the chance of survival should be present at lower frequency in older individuals. For example, if a mutation becomes harmful at the age of 60 years, people who carry it have a lower chance to survive past 60 – and the mutation should be less common among those who live longer than that.

We therefore looked for mutations that change in frequency with age among around 60,000 individuals from California (part of the GERA cohort) and around 150,000 from the U.K. Biobank. To avoid the complication that people whose ancestors lived in different places carry a somewhat different set of mutations, we focused on the largest group with shared ancestry within each study.

Across the genome, we found two variants that endanger survival. The first is a variant of the APOE gene, which is a well-known risk factor for Alzheimer’s disease. It drops in frequency beyond age 70. The second harmful variant we found is a mutation in the CHRNA3 gene. Associated with heavy smoking, this inherited mutation starts to decrease in frequency at middle age in men, because carriers of this mutation are less likely to survive longer.

People who carry a variant of the APOE gene die at a higher rate and are less common among the old age categories. Image via Mostafavi et al, PLOS Biology

Both deleterious variants only had an effect long after the typical ages of reproduction for both females and males. Biologists usually consider such mutations to not be under selection. After all, by late middle age, most people have already passed their genes on to whatever offspring they’ll have, so it seems like it might not matter how long they live beyond that point.

Why then would we only find two, when our study was large enough to detect any such variant, if common in the population? One possibility is that mutations that only imperil survival so late in life almost never arise. While that is possible, the genome is a large place, so that seems unlikely.

The other intriguing possibility is that natural selection prevents even late-acting variants from becoming common in the population by natural selection, if they have large enough effects. Why might that be? For one, men can father children in old age. Even if only a tiny fraction of them do so, it may be enough of an evolutionary fitness cost for selection to act on. Survival beyond the age of reproduction could also be beneficial for the survival of related individuals who carry the same mutations, most directly children. In other words, surviving past typical reproductive ages may be beneficial for humans after all.

Smokers who carry a mutation in the CHRNA3 gene tend to smoke more cigarettes per day and so are more exposed to harmful effects of smoking. Image via NeONBRAND on Unsplash

Your mutations do influence your survival

In addition to examining one mutation at a time, we were also interested in considering sets of mutations that have all been shown to influence the same trait, and might have very subtle effects on survival individually. For example, researchers have identified approximately 700 common mutations that influence height, each contributing only millimeters. To this end, we considered tens to hundreds of mutations that shape variation in one of 42 traits.

We found genetic mutations linked to a number of diseases and metabolic traits that decrease survival rates: individuals who are genetically predisposed to have higher total cholesterol, LDL cholesterol, risk of heart disease, BMI, risk of asthma or lower HDL cholesterol tend to die younger than others.

Perhaps more surprisingly, we discovered that people who carry mutations that delay puberty or the age at which they have their first child tend to live longer. It was known from epidemiological studies that early puberty is associated with adverse effects later in life such as cancer and obesity. Our results indicate some of that effect is probably due to heritable factors.

The ConversationSo humans carry common mutations that affect their survival and natural selection appears to act on at least a subset, in some contemporary environments. But what is bad in one context may well not be in another; as one example, the CHRNA3 variant has an effect because people smoke. These are early days, however, and our findings offer only a first glimpse of what can soon be gleaned from millions of genomes, in combination with genealogical records. In future work, it will be important to study not only lifespan, but also the number of children and grandchildren individuals leave, as well as populations and environments worldwide.

Hakhamanesh Mostafavi, Ph.D. Student in Biological Sciences, Columbia University; Joe Pickrell, Adjunct Assistant Professor of Biological Sciences, Columbia University, and Molly Przeworski, Professor of Biological Sciences, Columbia University

Bottom line: Comparing genomes of more than 200,000 people, researchers identified genetic variants that are less common in older people, suggesting natural selection continues to weed out disadvantageous traits.

This article was originally published on The Conversation. Read the original article.



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

Moon and the Twins next few mornings

On the mornings of September 15 and 16, 2017, you’ll find the stars Castor and Pollux – the zodiacal constellation Gemini the Twins – near the waning crescent moon.

They’re up late at night, too, but highest in the sky around dawn. After the moon, Castor and Pollux rise late tonight, they’ll go westward and upward throughout the wee morning hours for the same reason that the sun goes westward and upward after sunrise. The Earth spins eastward beneath the heavens, causing the sun, moon, planets and stars to rise in the east and to set in the west each day. Any celestial object – such as the sun, moon, planet or star – transits (reaches its highest point in the sky) midway between rising and setting.

If you’d like to know when any major solar system body rises/sets/transits in your sky, check out this U.S. Naval observatory page. The Gemini stars and Procyon fade into the glare of dawn before they transit in September. However, when the month of October comes rolling around, these bright stars will transit before dawn.

The moon actually moves eastward relative to the constellations of the zodiac, even as it moves westward across Earth’s sky each day. Therefore, watch for the moon to move away from the Gemini stars, Castor and Pollux, and toward the constellation Cancer over the next few days. If you’re up before dawn on September 15 and 16, note the change of the moon’s position after just one day.

Because the moon orbits Earth on nearly the same plane that Earth orbits the sun, you'll always see the moon near the ecliptic - Earth's orbital plane projected outward onto the constellations of the zodiac.

Because the moon orbits Earth on nearly the same plane that Earth orbits the sun, you’ll always see the moon near the ecliptic – Earth’s orbital plane projected outward onto the constellations of the zodiac.

On the average, the moon moves 13o eastward in front of the constellations of the zodiac each day. (For reference, the diameter of the moon spans about one-half degree.) So, on the average, the moon rises and sets about 50 minutes later daily. The moon’s change of position relative to the backdrop stars is due to the moon’s orbital motion around Earth.

The stars rise and set about four minutes earlier each day. That’s because the Earth in its orbit goes about one degree around the sun, slightly changing our perspective of the starry heavens from day to day.

Each day, the moon moves an average of 12o eastward of the sun – yet 13o eastward in front of the backdrop stars of the zodiac. That’s because each day, as seen from Earth, the sun appears to travel one degree eastward in front of the backdrop stars.

Bottom line: Enjoy the moon and Gemini stars, Castor and Pollux, on the mornings of September 15 and 16, 2017.



from EarthSky http://ift.tt/2d22YiC

On the mornings of September 15 and 16, 2017, you’ll find the stars Castor and Pollux – the zodiacal constellation Gemini the Twins – near the waning crescent moon.

They’re up late at night, too, but highest in the sky around dawn. After the moon, Castor and Pollux rise late tonight, they’ll go westward and upward throughout the wee morning hours for the same reason that the sun goes westward and upward after sunrise. The Earth spins eastward beneath the heavens, causing the sun, moon, planets and stars to rise in the east and to set in the west each day. Any celestial object – such as the sun, moon, planet or star – transits (reaches its highest point in the sky) midway between rising and setting.

If you’d like to know when any major solar system body rises/sets/transits in your sky, check out this U.S. Naval observatory page. The Gemini stars and Procyon fade into the glare of dawn before they transit in September. However, when the month of October comes rolling around, these bright stars will transit before dawn.

The moon actually moves eastward relative to the constellations of the zodiac, even as it moves westward across Earth’s sky each day. Therefore, watch for the moon to move away from the Gemini stars, Castor and Pollux, and toward the constellation Cancer over the next few days. If you’re up before dawn on September 15 and 16, note the change of the moon’s position after just one day.

Because the moon orbits Earth on nearly the same plane that Earth orbits the sun, you'll always see the moon near the ecliptic - Earth's orbital plane projected outward onto the constellations of the zodiac.

Because the moon orbits Earth on nearly the same plane that Earth orbits the sun, you’ll always see the moon near the ecliptic – Earth’s orbital plane projected outward onto the constellations of the zodiac.

On the average, the moon moves 13o eastward in front of the constellations of the zodiac each day. (For reference, the diameter of the moon spans about one-half degree.) So, on the average, the moon rises and sets about 50 minutes later daily. The moon’s change of position relative to the backdrop stars is due to the moon’s orbital motion around Earth.

The stars rise and set about four minutes earlier each day. That’s because the Earth in its orbit goes about one degree around the sun, slightly changing our perspective of the starry heavens from day to day.

Each day, the moon moves an average of 12o eastward of the sun – yet 13o eastward in front of the backdrop stars of the zodiac. That’s because each day, as seen from Earth, the sun appears to travel one degree eastward in front of the backdrop stars.

Bottom line: Enjoy the moon and Gemini stars, Castor and Pollux, on the mornings of September 15 and 16, 2017.



from EarthSky http://ift.tt/2d22YiC

Invertebrate Investigators

by Jon Markovich

In the previous Healthy Waters blog, my colleague Micka Peck wrote about the stream sampling we did for benthic macroinvertebrates. Pulling on a pair of waders and kicking around in the stream sampling was only half the fun.  After the outdoor fieldwork, I changed wardrobe from field gear to lab coat. Ok, I didn’t really wear a lab coat, but I was in a lab processing the preserved macroinvertebrates for later identification.

It’s been established that macroinvertebrates are good indicators of water quality conditions. Identifying which macroinvertebrates are present in a stream sample provides a link to determining whether a stream has good water quality and supports a healthy aquatic community.

One sample collected from a stream can have hundreds, even thousands, of macroinvertebrates. Thankfully, my target was to process a small sub-sample – around 200 individuals. This involves spreading the entire sample onto a gridded pan, randomly selecting a grid and removing all materials within it, and “picking” through the leaves, dirt, gravel, and other debris to separate out macroinvertebrates. At times, it felt as though I was playing a game of “Where’s Waldo?” In this case, “Waldo” could have no tails, two tails, or three tails, gills or no gills, or a whole number of different features. Sorting through these samples is no joke – it takes serious skill to quickly pick out bugs from non-bug debris. But after they’ve been picked from the sub-samples, the macroinvertebrates are identified under a microscope.

Looking under the scope, I marveled at these creatures. The different features and shapes of each bug were jaw-dropping. One bug, a burrowing mayfly in the family Ephemeridae, has protruding tusks on the side of its mouth like an elephant. The tusks help this family of mayfly to burrow into soft sediment to feed. Another bug, a dragonfly in the family Aeshnidae, had a hinged-mouth that extended to be nearly half the length of its body! Dragonfly larvae are predatory and this super-extendable mouthpart allows them to quickly snap up prey. These kinds of distinguishing features and characteristics are what scientists look at under the microscope for macroinvertebrate identification.

Although they look way cooler under a microscope, you don’t need one to see macroinvertebrates. If you have the chance, go check out your local stream, flip over rocks and search the stream bottom. You too could become an invertebrate investigator!

 

About the Author: Jon Markovich joined EPA’s Water Protection Division in 2014 and works in the impaired waters and Total Maximum Daily Load programs. In his spare time, Jon enjoys hiking, kayaking and camping in the Mid-Atlantic Region’s many great state parks.



from The EPA Blog http://ift.tt/2y6qjuH

by Jon Markovich

In the previous Healthy Waters blog, my colleague Micka Peck wrote about the stream sampling we did for benthic macroinvertebrates. Pulling on a pair of waders and kicking around in the stream sampling was only half the fun.  After the outdoor fieldwork, I changed wardrobe from field gear to lab coat. Ok, I didn’t really wear a lab coat, but I was in a lab processing the preserved macroinvertebrates for later identification.

It’s been established that macroinvertebrates are good indicators of water quality conditions. Identifying which macroinvertebrates are present in a stream sample provides a link to determining whether a stream has good water quality and supports a healthy aquatic community.

One sample collected from a stream can have hundreds, even thousands, of macroinvertebrates. Thankfully, my target was to process a small sub-sample – around 200 individuals. This involves spreading the entire sample onto a gridded pan, randomly selecting a grid and removing all materials within it, and “picking” through the leaves, dirt, gravel, and other debris to separate out macroinvertebrates. At times, it felt as though I was playing a game of “Where’s Waldo?” In this case, “Waldo” could have no tails, two tails, or three tails, gills or no gills, or a whole number of different features. Sorting through these samples is no joke – it takes serious skill to quickly pick out bugs from non-bug debris. But after they’ve been picked from the sub-samples, the macroinvertebrates are identified under a microscope.

Looking under the scope, I marveled at these creatures. The different features and shapes of each bug were jaw-dropping. One bug, a burrowing mayfly in the family Ephemeridae, has protruding tusks on the side of its mouth like an elephant. The tusks help this family of mayfly to burrow into soft sediment to feed. Another bug, a dragonfly in the family Aeshnidae, had a hinged-mouth that extended to be nearly half the length of its body! Dragonfly larvae are predatory and this super-extendable mouthpart allows them to quickly snap up prey. These kinds of distinguishing features and characteristics are what scientists look at under the microscope for macroinvertebrate identification.

Although they look way cooler under a microscope, you don’t need one to see macroinvertebrates. If you have the chance, go check out your local stream, flip over rocks and search the stream bottom. You too could become an invertebrate investigator!

 

About the Author: Jon Markovich joined EPA’s Water Protection Division in 2014 and works in the impaired waters and Total Maximum Daily Load programs. In his spare time, Jon enjoys hiking, kayaking and camping in the Mid-Atlantic Region’s many great state parks.



from The EPA Blog http://ift.tt/2y6qjuH

adds 2