Red sprites over the Andes

Dark sky with 3 fluorescent pink blobs wiht red lightning trailing down from them over mountains.

View larger. | Image via Yuri Beletsky.

Red sprites are large-scale electrical discharges – high above thunderstorm clouds – flickering in the night. They can be tens of miles high, but are very brief, lasting only a few tens of milliseconds. Photographer Yuri Beletsky captured these red sprites in early January 2020. Yuri described his image:

Red sprites over the Andes … The weather in the mountains [around now] is dominated by intense thunderstorms which develop over the Argentinean side. Here in Chile we have a perfect viewing spot from where we can safely watch the spectacle :) I captured this image during one of such storms developing across the mountains. On the crystal clear sky, you can see gorgeous red sprites and the blueish glow from the distant lightings, although the storm itself was not visible for us. I hope you will enjoy the view

What an amazing image! Thank you Yuri!

Bottom line: Photographer Yuri Beletsky captured red sprites flashing over the Chilean Andes Mountains in South America.

EarthSky 2020 lunar calendars are available! They make great gifts. Order now. Going fast!



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Dark sky with 3 fluorescent pink blobs wiht red lightning trailing down from them over mountains.

View larger. | Image via Yuri Beletsky.

Red sprites are large-scale electrical discharges – high above thunderstorm clouds – flickering in the night. They can be tens of miles high, but are very brief, lasting only a few tens of milliseconds. Photographer Yuri Beletsky captured these red sprites in early January 2020. Yuri described his image:

Red sprites over the Andes … The weather in the mountains [around now] is dominated by intense thunderstorms which develop over the Argentinean side. Here in Chile we have a perfect viewing spot from where we can safely watch the spectacle :) I captured this image during one of such storms developing across the mountains. On the crystal clear sky, you can see gorgeous red sprites and the blueish glow from the distant lightings, although the storm itself was not visible for us. I hope you will enjoy the view

What an amazing image! Thank you Yuri!

Bottom line: Photographer Yuri Beletsky captured red sprites flashing over the Chilean Andes Mountains in South America.

EarthSky 2020 lunar calendars are available! They make great gifts. Order now. Going fast!



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'Bilingual' molecule connects two basic codes for life

The new molecule holds the potential for diverse biomedical applications, says Emory chemist Jennifer Heemstra (right), in her lab with graduate student Colin Swenson, first author of the paper. (Photo by Kay Hinton)

By Carol Clark

The nucleic acids of DNA encode genetic information, while the amino acids of proteins contain the code to turn that information into structures and functions. Together, they provide the two fundamental codes underlying all of life.

Now scientists have found a way to combine these two main coding languages into a single “bilingual” molecule.

The Journal of the American Chemical Society published the work by chemists at Emory University. The synthesized molecule could become a powerful tool for applications such as diagnostics, gene therapy and drug delivery targeted to specific cells.

“Much like a translator enables communication between two people from different regions of the world, we envision that our bilingual molecule will enable us to mediate new forms of communications between nucleic acids and proteins in the cellular environment,” says Jennifer Heemstra, associate professor of chemistry at Emory University and senior author of the study. 

Nucleic acids store information in an “alphabet” of four bases, known as nucleotides. Peptides and proteins use an entirely different alphabet, made up of 20 different amino acids.

“The nucleic acid language is easy to speak, but kind of limited,” Heemstra says. “While the protein language is incredibly complex and difficult to predict. Both of these molecules have developed exquisite properties over billions of years of evolution.”

Previously synthesized molecules have focused on the properties of either nucleic acids or amino acids. The Emory researchers wanted to harness the powers of both information systems within a single molecule.

The challenge was enormous, drawing on techniques from organic chemistry, molecular and cellular biology, materials science and analytical chemistry. The researchers built a protein scaffold and then attached functioning fragments of nucleotides and amino acids to this framework.

“The two different codes needed to be synthesized separately and then brought together into the scaffold,” says Colin Swenson, first author of the paper and a graduate student in the Heemstra Lab.

The resulting bilingual molecule is stable, made of inexpensive materials, and highly generalizable, giving it the potential for diverse biomedical and nanotechnology applications. “It’s like a programmable, universal adaptor that brings proteins and nucleic acids together,” Heemstra says. “We hope that other researchers are inspired to think about different ways that it might be applied.” 

The Emory chemists are now exploring using the bilingual molecule for targeted drug delivery to particular cells. “It’s essentially a stimuli-sensitive container,” Heemstra says. “We’ve demonstrated that it can bind to drug molecules. And it’s programmable to fall apart in the presence of specific RNA molecules that are more abundant in cancer cells.”

Related:
Chemists teach old drug new tricks to target deadly staph bacteria
DNA 'origami' takes flight in emerging field of nano machines

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The new molecule holds the potential for diverse biomedical applications, says Emory chemist Jennifer Heemstra (right), in her lab with graduate student Colin Swenson, first author of the paper. (Photo by Kay Hinton)

By Carol Clark

The nucleic acids of DNA encode genetic information, while the amino acids of proteins contain the code to turn that information into structures and functions. Together, they provide the two fundamental codes underlying all of life.

Now scientists have found a way to combine these two main coding languages into a single “bilingual” molecule.

The Journal of the American Chemical Society published the work by chemists at Emory University. The synthesized molecule could become a powerful tool for applications such as diagnostics, gene therapy and drug delivery targeted to specific cells.

“Much like a translator enables communication between two people from different regions of the world, we envision that our bilingual molecule will enable us to mediate new forms of communications between nucleic acids and proteins in the cellular environment,” says Jennifer Heemstra, associate professor of chemistry at Emory University and senior author of the study. 

Nucleic acids store information in an “alphabet” of four bases, known as nucleotides. Peptides and proteins use an entirely different alphabet, made up of 20 different amino acids.

“The nucleic acid language is easy to speak, but kind of limited,” Heemstra says. “While the protein language is incredibly complex and difficult to predict. Both of these molecules have developed exquisite properties over billions of years of evolution.”

Previously synthesized molecules have focused on the properties of either nucleic acids or amino acids. The Emory researchers wanted to harness the powers of both information systems within a single molecule.

The challenge was enormous, drawing on techniques from organic chemistry, molecular and cellular biology, materials science and analytical chemistry. The researchers built a protein scaffold and then attached functioning fragments of nucleotides and amino acids to this framework.

“The two different codes needed to be synthesized separately and then brought together into the scaffold,” says Colin Swenson, first author of the paper and a graduate student in the Heemstra Lab.

The resulting bilingual molecule is stable, made of inexpensive materials, and highly generalizable, giving it the potential for diverse biomedical and nanotechnology applications. “It’s like a programmable, universal adaptor that brings proteins and nucleic acids together,” Heemstra says. “We hope that other researchers are inspired to think about different ways that it might be applied.” 

The Emory chemists are now exploring using the bilingual molecule for targeted drug delivery to particular cells. “It’s essentially a stimuli-sensitive container,” Heemstra says. “We’ve demonstrated that it can bind to drug molecules. And it’s programmable to fall apart in the presence of specific RNA molecules that are more abundant in cancer cells.”

Related:
Chemists teach old drug new tricks to target deadly staph bacteria
DNA 'origami' takes flight in emerging field of nano machines

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What is an eclipse season?

A totally eclipsed sun with a bright light emerging on one side: the diamond ring effect.

View larger. | EarthSky community member Beverley Sinclair captured this beautiful view of a total solar eclipse outside Charleston, South Carolina on August 21, 2017 and wrote: “The skies were very cloudy leading up to totality but, miraculously, slowly cleared as totality approached. This photo shows the diamond ring and Bailey’s beads.” Thank you, Beverley!

Here are some words you need to know to understand eclipse seasons: lunar nodes and ecliptic. The ecliptic is the plane of the Earth’s orbit around the sun. A lunar node is the point where, in its monthly orbit of Earth, the moon’s orbit intersects that plane. An eclipse season is when – from Earth’s perspective – the sun is close enough to a lunar node to allow an eclipse to take place. If the sun is close to a lunar node at full moon, we see a lunar eclipse. If the sun is close to a lunar node at new moon, we see a solar eclipse.

To put it another way, if the moon turns new or full in close concert with the moon’s crossing of one of its nodes, then an eclipse is not only possible – but inevitable.

Illustration of lunar nodes pointing at sun in the middle of an eclipse season.

Lunar nodes are where the moon’s orbit cuts through the ecliptic, or Earth-sun plane. When these nodes point directly at the sun, it marks the midpoint of an approximate 35-day eclipse season. The middle of an eclipse season occurred on December 30, 2019. Another will occur on June 20, 2020. Image via Go Science GO.

There are four to seven eclipses every calendar year, and two eclipse seasons. In some years, it’s possible to have a third eclipse season straddling into the previous or following year (as, for example, the eclipse season of December 2019/January 2020).

An eclipse season lasts for approximately 35 days, and recurs in cycles of 173.3 days (somewhat shy of six calendar months).

Given that the lunar month (period of time between successive new moons or successive full moons) is about 29.5 days long, a minimum of two eclipses (one solar and one lunar, in either order) happens in one eclipse season. A maximum of 3 eclipses is possible (either lunar/solar/lunar, or solar/lunar/solar), though the first eclipse of the eclipse season has to come quite early to allow for a third eclipse near the end.

If there are seven eclipses in one calendar year, there are a few possibilities. The 1st one belongs to an eclipse season that started in the previous year – and/or the 7th eclipse belongs to an eclipse season that ends in the following year. It’s rare for seven eclipses to occur in one calendar year, however. It last happened in the year 1982, and will next occur in the year 2038.

At this writing (January 8, 2020), we are in the midst of an eclipse season, whose midpoint came on December 30, 2019. The first eclipse of the present eclipse season came when the new moon swung smack-dab in front of the solar disk to showcase an annular (ring of fire) solar eclipse on December 26, 2019. See the photo below.

Three images, narrow rings around sun, two on sides with gaps.

View at EarthSky Community Photos. | Progression into and out of the annular eclipse on December 26, 2019, from Tumon Bay, Guam. Eliot Herman reported: “It was a beautiful day in Guam to observe the eclipse mostly clear blue skies with a little marine haze on the coast. These images were captured with a Questar telescope and a Nikon D850 camera using a Baader solar filter.” Thank you, Eliot!

The second eclipse of the current eclipse season will come with a penumbral eclipse of the full moon on January 10, 2020. Any lunar eclipse that comes early, or late, in an eclipse season finds the full moon missing the Earth’s umbra (inner dark shadow), and passing through the penumbra (outer faint shadow) instead. Because the upcoming lunar eclipse occurs rather late in the eclipse season, it’ll be a penumbral lunar eclipse. See the diagram below.

Chart of moon moving through Earth's outer shadow - a penumbral eclipse.

On January 10, 2020, the full moon misses Earth’s dark umbral shadow but goes through our world’s fainter penumbral shadow, to present a barely perceptible eclipse. This eclipse would be more impressive from the moon, where you’d see a partial eclipse of the sun.

A solar eclipse can happen only at new moon. A lunar eclipse can happen only at full moon. Additionally – for an eclipse to occur – the new moon or full moon has to take place within an eclipse season. Otherwise, the new moon passes too far north, or south, of the sun for a solar eclipse to take place, and the full moon sweeps too far north, or south, of the Earth’s shadow for a lunar eclipse to take place.

Graphic of Earth, moon, and sun showing moon's shadow blocking the sun.

Eclipses are all about alignments. In a solar eclipse, the sun, moon and Earth line up, with the moon in the middle. Image via NASA.

Graphic of Earth, moon, and sun with Earth shading the moon.

In a lunar eclipse, the sun, Earth and moon line up, with the Earth in the middle. Image via NASA.

Why do we have eclipse seasons?

There are many cycles in the heavens. An eclipse season is just one of these many celestial cycles.

Consider that if the moon orbited Earth on the same plane that the Earth orbits the sun, then we’d have a solar eclipse at every new moon, and a lunar eclipse at every full moon.

But – in reality – the moon’s orbit is inclined by 5 degrees to the ecliptic (Earth’s orbital plane), so most of the time the new moon or full moon swings too far north, or south, of the ecliptic for an eclipse to take place. For instance, in the year 2020, we will have 12 new moons and 13 full moons, but only 2 solar eclipses and 4 lunar eclipses (all of the lunar eclipses in 2020, unfortunately, will be faint and hard-to-see penumbral lunar eclipses).

Moon phases 2020.

In the year 2020, there are 12 new moons and 13 full moons. A = annular solar eclipse, T = total solar eclipse, and n = penumbral lunar elcipse. Moon phases via Astropixels.

Twice every month, as the moon circles Earth in its orbit, the moon crosses the ecliptic (Earth’s orbital plane) at points called nodes. If the moon is going from south to north, it’s called the moon’s ascending node, and if the moon is moving from north to south, it’s called the moon’s descending node. The moon was last at its descending node on December 26, 2019, and will reach its ascending node on January 9, 2020.

Read more: Node passages of the Moon: 2001 to 2100

Whenever the lunar nodes point directly at the sun, that momentous event marks the middle of the eclipse season. The alignment of the moon, sun and Earth is most exact when an eclipse happens at the middle of an eclipse season, and the least so when an eclipse occurs at the start, or the end, of an eclipse season. Any lunar eclipse happening early or late in the eclipse season presents a penumbral lunar eclipse, whereas any solar eclipse happening early or late in the eclipse season features a skimpy partial eclipse of the sun.

In the year 2019, the middle of the eclipse seasons took place on January 17, July 10, and December 30, 2019. This year, in 2020, the middle of the eclipse seasons falls on June 20, 2020, and December 11, 2020.

Middle of eclipse season: December 30, 2019
First eclipse (solar): December 26, 2019
Second eclipse (lunar): January 10, 2020

Middle of eclipse season: June 20, 2020
First eclipse (lunar): June 5, 2020
Second eclipse (solar): June 21, 2020
Third eclipse (lunar): July 5, 2020

Middle of eclipse season: December 11, 2020
First eclipse (lunar): November 30, 2020
Second eclipse (solar): December 14, 2020

Line drawing of sphere with oblique view of orbits.

The plane of the moon’s orbit is inclined at 5 degrees to the plane of Earth’s orbit around the sun (the ecliptic). In this diagram, however, the ecliptic is portrayed as the sun’s apparent annual path in front of the constellations of the zodiac. The moon’s orbit intersects the ecliptic at two points called nodes (labeled here as N1 and N2). It’s the middle of the eclipse season whenever this line of nodes points directly at the sun. In the above diagram, the line of nodes does not point at the sun.

Bottom line: An eclipse season is when – from Earth’s perspective – the sun is close enough to a lunar node to allow an eclipse to take place. If the sun is close to a node at full moon, we see a lunar eclipse. If the sun is close to a node at new moon, we see a solar eclipse. A minimum of two eclipses (one solar and one lunar, in either order) happens in one eclipse season. A maximum of 3 eclipses is possible (either lunar/solar/lunar, or solar/lunar/solar).



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A totally eclipsed sun with a bright light emerging on one side: the diamond ring effect.

View larger. | EarthSky community member Beverley Sinclair captured this beautiful view of a total solar eclipse outside Charleston, South Carolina on August 21, 2017 and wrote: “The skies were very cloudy leading up to totality but, miraculously, slowly cleared as totality approached. This photo shows the diamond ring and Bailey’s beads.” Thank you, Beverley!

Here are some words you need to know to understand eclipse seasons: lunar nodes and ecliptic. The ecliptic is the plane of the Earth’s orbit around the sun. A lunar node is the point where, in its monthly orbit of Earth, the moon’s orbit intersects that plane. An eclipse season is when – from Earth’s perspective – the sun is close enough to a lunar node to allow an eclipse to take place. If the sun is close to a lunar node at full moon, we see a lunar eclipse. If the sun is close to a lunar node at new moon, we see a solar eclipse.

To put it another way, if the moon turns new or full in close concert with the moon’s crossing of one of its nodes, then an eclipse is not only possible – but inevitable.

Illustration of lunar nodes pointing at sun in the middle of an eclipse season.

Lunar nodes are where the moon’s orbit cuts through the ecliptic, or Earth-sun plane. When these nodes point directly at the sun, it marks the midpoint of an approximate 35-day eclipse season. The middle of an eclipse season occurred on December 30, 2019. Another will occur on June 20, 2020. Image via Go Science GO.

There are four to seven eclipses every calendar year, and two eclipse seasons. In some years, it’s possible to have a third eclipse season straddling into the previous or following year (as, for example, the eclipse season of December 2019/January 2020).

An eclipse season lasts for approximately 35 days, and recurs in cycles of 173.3 days (somewhat shy of six calendar months).

Given that the lunar month (period of time between successive new moons or successive full moons) is about 29.5 days long, a minimum of two eclipses (one solar and one lunar, in either order) happens in one eclipse season. A maximum of 3 eclipses is possible (either lunar/solar/lunar, or solar/lunar/solar), though the first eclipse of the eclipse season has to come quite early to allow for a third eclipse near the end.

If there are seven eclipses in one calendar year, there are a few possibilities. The 1st one belongs to an eclipse season that started in the previous year – and/or the 7th eclipse belongs to an eclipse season that ends in the following year. It’s rare for seven eclipses to occur in one calendar year, however. It last happened in the year 1982, and will next occur in the year 2038.

At this writing (January 8, 2020), we are in the midst of an eclipse season, whose midpoint came on December 30, 2019. The first eclipse of the present eclipse season came when the new moon swung smack-dab in front of the solar disk to showcase an annular (ring of fire) solar eclipse on December 26, 2019. See the photo below.

Three images, narrow rings around sun, two on sides with gaps.

View at EarthSky Community Photos. | Progression into and out of the annular eclipse on December 26, 2019, from Tumon Bay, Guam. Eliot Herman reported: “It was a beautiful day in Guam to observe the eclipse mostly clear blue skies with a little marine haze on the coast. These images were captured with a Questar telescope and a Nikon D850 camera using a Baader solar filter.” Thank you, Eliot!

The second eclipse of the current eclipse season will come with a penumbral eclipse of the full moon on January 10, 2020. Any lunar eclipse that comes early, or late, in an eclipse season finds the full moon missing the Earth’s umbra (inner dark shadow), and passing through the penumbra (outer faint shadow) instead. Because the upcoming lunar eclipse occurs rather late in the eclipse season, it’ll be a penumbral lunar eclipse. See the diagram below.

Chart of moon moving through Earth's outer shadow - a penumbral eclipse.

On January 10, 2020, the full moon misses Earth’s dark umbral shadow but goes through our world’s fainter penumbral shadow, to present a barely perceptible eclipse. This eclipse would be more impressive from the moon, where you’d see a partial eclipse of the sun.

A solar eclipse can happen only at new moon. A lunar eclipse can happen only at full moon. Additionally – for an eclipse to occur – the new moon or full moon has to take place within an eclipse season. Otherwise, the new moon passes too far north, or south, of the sun for a solar eclipse to take place, and the full moon sweeps too far north, or south, of the Earth’s shadow for a lunar eclipse to take place.

Graphic of Earth, moon, and sun showing moon's shadow blocking the sun.

Eclipses are all about alignments. In a solar eclipse, the sun, moon and Earth line up, with the moon in the middle. Image via NASA.

Graphic of Earth, moon, and sun with Earth shading the moon.

In a lunar eclipse, the sun, Earth and moon line up, with the Earth in the middle. Image via NASA.

Why do we have eclipse seasons?

There are many cycles in the heavens. An eclipse season is just one of these many celestial cycles.

Consider that if the moon orbited Earth on the same plane that the Earth orbits the sun, then we’d have a solar eclipse at every new moon, and a lunar eclipse at every full moon.

But – in reality – the moon’s orbit is inclined by 5 degrees to the ecliptic (Earth’s orbital plane), so most of the time the new moon or full moon swings too far north, or south, of the ecliptic for an eclipse to take place. For instance, in the year 2020, we will have 12 new moons and 13 full moons, but only 2 solar eclipses and 4 lunar eclipses (all of the lunar eclipses in 2020, unfortunately, will be faint and hard-to-see penumbral lunar eclipses).

Moon phases 2020.

In the year 2020, there are 12 new moons and 13 full moons. A = annular solar eclipse, T = total solar eclipse, and n = penumbral lunar elcipse. Moon phases via Astropixels.

Twice every month, as the moon circles Earth in its orbit, the moon crosses the ecliptic (Earth’s orbital plane) at points called nodes. If the moon is going from south to north, it’s called the moon’s ascending node, and if the moon is moving from north to south, it’s called the moon’s descending node. The moon was last at its descending node on December 26, 2019, and will reach its ascending node on January 9, 2020.

Read more: Node passages of the Moon: 2001 to 2100

Whenever the lunar nodes point directly at the sun, that momentous event marks the middle of the eclipse season. The alignment of the moon, sun and Earth is most exact when an eclipse happens at the middle of an eclipse season, and the least so when an eclipse occurs at the start, or the end, of an eclipse season. Any lunar eclipse happening early or late in the eclipse season presents a penumbral lunar eclipse, whereas any solar eclipse happening early or late in the eclipse season features a skimpy partial eclipse of the sun.

In the year 2019, the middle of the eclipse seasons took place on January 17, July 10, and December 30, 2019. This year, in 2020, the middle of the eclipse seasons falls on June 20, 2020, and December 11, 2020.

Middle of eclipse season: December 30, 2019
First eclipse (solar): December 26, 2019
Second eclipse (lunar): January 10, 2020

Middle of eclipse season: June 20, 2020
First eclipse (lunar): June 5, 2020
Second eclipse (solar): June 21, 2020
Third eclipse (lunar): July 5, 2020

Middle of eclipse season: December 11, 2020
First eclipse (lunar): November 30, 2020
Second eclipse (solar): December 14, 2020

Line drawing of sphere with oblique view of orbits.

The plane of the moon’s orbit is inclined at 5 degrees to the plane of Earth’s orbit around the sun (the ecliptic). In this diagram, however, the ecliptic is portrayed as the sun’s apparent annual path in front of the constellations of the zodiac. The moon’s orbit intersects the ecliptic at two points called nodes (labeled here as N1 and N2). It’s the middle of the eclipse season whenever this line of nodes points directly at the sun. In the above diagram, the line of nodes does not point at the sun.

Bottom line: An eclipse season is when – from Earth’s perspective – the sun is close enough to a lunar node to allow an eclipse to take place. If the sun is close to a node at full moon, we see a lunar eclipse. If the sun is close to a node at new moon, we see a solar eclipse. A minimum of two eclipses (one solar and one lunar, in either order) happens in one eclipse season. A maximum of 3 eclipses is possible (either lunar/solar/lunar, or solar/lunar/solar).



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These 2 stars in Sagitta will merge and explode by this century’s end

Two white flattened spheres, one much larger. Material is flowing from the larger to the smaller.

Artist’s concept of the pair of stars making up the binary system V Sagittae. According to astronomers, they’re due to merge – and shine brightly – before this century ends. Image via LSU.

The American Astronomical Society – the biggest and most established organization of professional astronomers in the United States – is meeting this week (January 4-8, 2020) in Honolulu, Hawaii. One of the more interesting stories to come from the meeting involves a faint star in our night sky. The star is V Sagittae (V Sge) – a barely visible star even in mid-sized telescopes, astronomers said – located in the direction of one of the sky’s smallest constellations, Sagitta the Arrow. This “innocent” star, they said will explode around the year 2083, becoming as bright as Sirius, brightest star in our night sky. According to astronomers Bradley E. Schaefer, Juhan Frank, and Manos Chatzopoulos, all at Louisiana State University:

During this time of eruption, V Sge will be the most luminous star in the Milky Way galaxy.

V Sagittae is what astronomers call a cataclysmic variable star. From Earth, astronomers peering through telescopes see its brightness rise and fall rapidly. Astronomers describe this rapid variability as flickering. The flickering is thought to result from the relationship between the two stars in the system, which orbit close to one another.

One star is an ordinary star, not dissimilar from our sun. The other is a small, compact white dwarf. The brightness changes take place as material from the ordinary star falls onto the white dwarf. There is a classic accretion disk (similar to that seen around black holes) around the white dwarf. Material from the ordinary star falls onto the accretion disk first, before being funneled down onto the white dwarf’s surface.

So you can imagine it: a star spilling material onto a disk around smaller, very dense star. It’s a highly dynamic natural event, which we’re viewing from a great distance. If you could see it up close, you’d surely see differently sized clumps of material moving from one star to the other, and bright spots where that material is striking the accretion disk, more bright spots where material from the disk lands on the star, and maybe some flares here and there. Some portion of all this activity is visible as rapid brightness changes – on timescales of seconds – to astronomers watching from Earth. Hence, flickering.

Plus, it’s now understood that the two stars aren’t fixed in their distance from one another. They’re spiraling toward one another, their distance constantly decreasing. What will happen? Schaefer explained:

We now have a strong prediction for the future of V Sge. Over the next few decades, the star will brighten rapidly. Around the year 2083, its accretion rate will rise catastrophically, spilling mass at incredibly high rates onto the white dwarf, with this material blazing away.

In the final days of this death-spiral, all of the mass from the companion star will fall onto the white dwarf, creating a super-massive wind from the merging star, appearing as bright as Sirius, possibly even as bright as Venus.

EarthSky 2020 moon phase calendars are available! Nearly sold out. Order now. Going fast!

Chart of the Summer Triangle, with the 3 small constellations Sagitta, Vulpecula and Delphinus.

The Summer Triangle isn’t a constellation but a large asterism consisting of 3 bright stars in 3 separate constellations. These stars are Vega, Deneb and Altair. If you can find the Summer Triangle, you can use it to locate 3 of the sky’s smallest constellations: Vulpecula the Fox, Delphinus the Dolphin and Sagitta the Arrow. All 3 would be impossible to see from the city, but they’re lots of fun to see in a dark sky. The binary system V Sagittae is located in the constellation Sagitta.

By definition, cataclysmic variables (CVs) are all binary stars, but they vary spectacularly in behavior. These astronomers said:

V Sge is the most extreme of all the CVs, approximately 100 times more luminous than all other known CVs, and is powering a massive stellar wind, equal to the winds of the most massive stars prior to their deaths. These two extreme properties are caused by the fact that the normal star is 3.9 times more massive than the white dwarf.

Schaefer explained:

In all other known CVs the white dwarf is more massive than the orbiting normal star, so V Sge is utterly unique.

Frank added:

Previously, astronomers have studied V Sge, realizing that it is an unusual system with extreme properties. However, no one had realized that the binary orbit was in-spiraling very fast.

This realization came from routine measures of V Sge’s brightness on old sky photos now archived at the Harvard College Observatory, providing a detailed history going back to the year 1890, these astronomers said. They explained:

Startlingly, V Sge has been systematically brightening by a factor of 10 times, and 2.5 magnitudes, from the early 1890s up until the last decade. This unprecedented behavior was confirmed with archival data collected from the database of the American Association of Variable Star Observers (AAVSO), showing V Sge brightening by nearly a factor of 10 times, 2.4 magnitudes, from 1907 until the last few years.

Frank added:

V Sge is exponentially gaining luminosity with a doubling time scale of 89 years. This brightening can only result with the rate of mass falling off the normal companion star increasing exponentially, ultimately because the binary orbit is in-spiraling rapidly.

Star chart showing Sagitta the Arrow with V Sagittae marked beyond one end of it.

Here is the constellation Sagitta the Arrow again, with the location of V Sagittae marked. As Schaefer commented, the Arrow is pointing to V Sagittae and the future nova. Chart via LSU.

Schaefer said:

In anticipation of this fast decaying of the orbit, the fate of V Sge is sealed. The critical and simple physics are derived from V Sge having the companion star being much more massive than the white dwarf star, so forcing the rate of mass transfer to rise exponentially. Anticipating the next few decades, V Sge will in-spiral at a rapid pace with increasing brightness. Inevitably, this in-spiral will climax with the majority of the gas in the normal star falling onto the white dwarf, all within the final weeks and days. This falling mass will release a tremendous amount of gravitational potential energy, driving a stellar wind as never before seen, and raise the system luminosity to just short of that of supernovae at peak.

This explosive event will have peak brightness over a month, with two stars merging into one star. The end result of the merger will produce a single star with a degenerate white dwarf core, a hydrogen-burning layer, surrounded by a vast gas envelope mostly of hydrogen. Schaefer said:

From this critical new input of the doubling time scale of 89 years, it becomes possible to directly calculate the future evolution of V Sge, all using standard equations describing the many physical mechanisms involved.

These astronomers used the word “robust” to describe their calculations. In other words, they are confident that the final merger of the two stars will be around the year 2083. Frank commented:

The uncertainty in this date is ±16 years, arising mostly from not having a perfect measure of the doubling time scale due to the large intrinsic jitter of the brightness in the historical record.

Therefore, the merge will be approximately between 2067 and 2099, most likely near the middle of this range.

Schaefer said:

Thus, V Sge will appear startlingly bright in the night sky. This is substantially brighter than the all-time brightest known nova (at -0.5) just over a century ago, and the last time any ‘guest star’ appeared brighter was Kepler’s Supernova in the year 1604.

Now people the world over can know that they will see a wondrous guest star shining as the brightest in the sky for a month or so, being pointed at by the Arrow just below Cygnus the Swan.

Bottom line: At the 235th meeting of the American Astronomical Society on January 4-8, 2020, astronomers said that the 2 stars in the binary star system V Sagittae are spiraling inward and due for an explosion, called a nova, which should happen around the year 2083. The nova will temporarily outshine all the stars in our Milky Way galaxy.



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Two white flattened spheres, one much larger. Material is flowing from the larger to the smaller.

Artist’s concept of the pair of stars making up the binary system V Sagittae. According to astronomers, they’re due to merge – and shine brightly – before this century ends. Image via LSU.

The American Astronomical Society – the biggest and most established organization of professional astronomers in the United States – is meeting this week (January 4-8, 2020) in Honolulu, Hawaii. One of the more interesting stories to come from the meeting involves a faint star in our night sky. The star is V Sagittae (V Sge) – a barely visible star even in mid-sized telescopes, astronomers said – located in the direction of one of the sky’s smallest constellations, Sagitta the Arrow. This “innocent” star, they said will explode around the year 2083, becoming as bright as Sirius, brightest star in our night sky. According to astronomers Bradley E. Schaefer, Juhan Frank, and Manos Chatzopoulos, all at Louisiana State University:

During this time of eruption, V Sge will be the most luminous star in the Milky Way galaxy.

V Sagittae is what astronomers call a cataclysmic variable star. From Earth, astronomers peering through telescopes see its brightness rise and fall rapidly. Astronomers describe this rapid variability as flickering. The flickering is thought to result from the relationship between the two stars in the system, which orbit close to one another.

One star is an ordinary star, not dissimilar from our sun. The other is a small, compact white dwarf. The brightness changes take place as material from the ordinary star falls onto the white dwarf. There is a classic accretion disk (similar to that seen around black holes) around the white dwarf. Material from the ordinary star falls onto the accretion disk first, before being funneled down onto the white dwarf’s surface.

So you can imagine it: a star spilling material onto a disk around smaller, very dense star. It’s a highly dynamic natural event, which we’re viewing from a great distance. If you could see it up close, you’d surely see differently sized clumps of material moving from one star to the other, and bright spots where that material is striking the accretion disk, more bright spots where material from the disk lands on the star, and maybe some flares here and there. Some portion of all this activity is visible as rapid brightness changes – on timescales of seconds – to astronomers watching from Earth. Hence, flickering.

Plus, it’s now understood that the two stars aren’t fixed in their distance from one another. They’re spiraling toward one another, their distance constantly decreasing. What will happen? Schaefer explained:

We now have a strong prediction for the future of V Sge. Over the next few decades, the star will brighten rapidly. Around the year 2083, its accretion rate will rise catastrophically, spilling mass at incredibly high rates onto the white dwarf, with this material blazing away.

In the final days of this death-spiral, all of the mass from the companion star will fall onto the white dwarf, creating a super-massive wind from the merging star, appearing as bright as Sirius, possibly even as bright as Venus.

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Chart of the Summer Triangle, with the 3 small constellations Sagitta, Vulpecula and Delphinus.

The Summer Triangle isn’t a constellation but a large asterism consisting of 3 bright stars in 3 separate constellations. These stars are Vega, Deneb and Altair. If you can find the Summer Triangle, you can use it to locate 3 of the sky’s smallest constellations: Vulpecula the Fox, Delphinus the Dolphin and Sagitta the Arrow. All 3 would be impossible to see from the city, but they’re lots of fun to see in a dark sky. The binary system V Sagittae is located in the constellation Sagitta.

By definition, cataclysmic variables (CVs) are all binary stars, but they vary spectacularly in behavior. These astronomers said:

V Sge is the most extreme of all the CVs, approximately 100 times more luminous than all other known CVs, and is powering a massive stellar wind, equal to the winds of the most massive stars prior to their deaths. These two extreme properties are caused by the fact that the normal star is 3.9 times more massive than the white dwarf.

Schaefer explained:

In all other known CVs the white dwarf is more massive than the orbiting normal star, so V Sge is utterly unique.

Frank added:

Previously, astronomers have studied V Sge, realizing that it is an unusual system with extreme properties. However, no one had realized that the binary orbit was in-spiraling very fast.

This realization came from routine measures of V Sge’s brightness on old sky photos now archived at the Harvard College Observatory, providing a detailed history going back to the year 1890, these astronomers said. They explained:

Startlingly, V Sge has been systematically brightening by a factor of 10 times, and 2.5 magnitudes, from the early 1890s up until the last decade. This unprecedented behavior was confirmed with archival data collected from the database of the American Association of Variable Star Observers (AAVSO), showing V Sge brightening by nearly a factor of 10 times, 2.4 magnitudes, from 1907 until the last few years.

Frank added:

V Sge is exponentially gaining luminosity with a doubling time scale of 89 years. This brightening can only result with the rate of mass falling off the normal companion star increasing exponentially, ultimately because the binary orbit is in-spiraling rapidly.

Star chart showing Sagitta the Arrow with V Sagittae marked beyond one end of it.

Here is the constellation Sagitta the Arrow again, with the location of V Sagittae marked. As Schaefer commented, the Arrow is pointing to V Sagittae and the future nova. Chart via LSU.

Schaefer said:

In anticipation of this fast decaying of the orbit, the fate of V Sge is sealed. The critical and simple physics are derived from V Sge having the companion star being much more massive than the white dwarf star, so forcing the rate of mass transfer to rise exponentially. Anticipating the next few decades, V Sge will in-spiral at a rapid pace with increasing brightness. Inevitably, this in-spiral will climax with the majority of the gas in the normal star falling onto the white dwarf, all within the final weeks and days. This falling mass will release a tremendous amount of gravitational potential energy, driving a stellar wind as never before seen, and raise the system luminosity to just short of that of supernovae at peak.

This explosive event will have peak brightness over a month, with two stars merging into one star. The end result of the merger will produce a single star with a degenerate white dwarf core, a hydrogen-burning layer, surrounded by a vast gas envelope mostly of hydrogen. Schaefer said:

From this critical new input of the doubling time scale of 89 years, it becomes possible to directly calculate the future evolution of V Sge, all using standard equations describing the many physical mechanisms involved.

These astronomers used the word “robust” to describe their calculations. In other words, they are confident that the final merger of the two stars will be around the year 2083. Frank commented:

The uncertainty in this date is ±16 years, arising mostly from not having a perfect measure of the doubling time scale due to the large intrinsic jitter of the brightness in the historical record.

Therefore, the merge will be approximately between 2067 and 2099, most likely near the middle of this range.

Schaefer said:

Thus, V Sge will appear startlingly bright in the night sky. This is substantially brighter than the all-time brightest known nova (at -0.5) just over a century ago, and the last time any ‘guest star’ appeared brighter was Kepler’s Supernova in the year 1604.

Now people the world over can know that they will see a wondrous guest star shining as the brightest in the sky for a month or so, being pointed at by the Arrow just below Cygnus the Swan.

Bottom line: At the 235th meeting of the American Astronomical Society on January 4-8, 2020, astronomers said that the 2 stars in the binary star system V Sagittae are spiraling inward and due for an explosion, called a nova, which should happen around the year 2083. The nova will temporarily outshine all the stars in our Milky Way galaxy.



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Twenty years of discoveries changing story of human evolution

Brown, barren canyon with many layers of rock.

Nearly a century ago, archaeologists started to shift the focus of human origins research from Europe to Africa’s ‘cradles of humankind’ like Oldupai (Olduvai) Gorge in Tanzania. What will the next big shifts be? Image via Manuel Domínguez-Rodrigo.

By Elizabeth Sawchuk, Stony Brook University (The State University of New York) and Mary Prendergast, Saint Louis University – Madrid

In 1924, a 3-year-old child’s skull found in South Africa forever changed how people think about human origins.

The Taung Child, our first encounter with an ancient group of proto-humans or hominins called australopithecines, was a turning point in the study of human evolution. This discovery shifted the focus of human origins research from Europe and Asia onto Africa, setting the stage for the last century of research on the continent and into its “Cradles of Humankind.”

Few people back then would’ve been able to predict what scientists know about evolution today, and now the pace of discovery is faster than ever. Even since the turn of the 21st century, human origins textbooks have been rewritten over and over again. Just 20 years ago, no one could have imagined what scientists know two decades later about humanity’s deep past, let alone how much knowledge could be extracted from a thimble of dirt, a scrape of dental plaque or satellites in space.

Human fossils are outgrowing the family tree

In Africa, there are now several fossil candidates for the earliest hominin dated to between 5 and 7 million years ago, when we know humans likely split off from other Great Apes based on differences in our DNA.

Although discovered in the 1990s, publication of the 4.4 million year old skeleton nicknamed “Ardi” in 2009 changed scientists’ views on how hominins began walking.

Rounding out our new relatives are a few australopithecines, including Australopithecus deryiremeda and Australopithecus sediba, as well as a potentially late-surviving species of early Homo that reignited debate about when humans first began burying their dead.

Human skull, much flatter head than a modern human.

Fossils like that of Australopithecus sediba, discovered in South Africa by a 9-year-old boy, are reshaping the human family tree. Image via Brett Eloff/ Courtesy Prof Berger and Wits University.

Perspectives on our own species have also changed. Archaeologists previously thought Homo sapiens evolved in Africa around 200,000 years ago, but the story has become more complicated. Fossils
discovered in Morocco have pushed that date back to 300,000 years ago, consistent with ancient DNA evidence. This raises doubts that our species emerged in any single place.

This century has also brought unexpected discoveries from Europe and Asia. From enigmatic “hobbits” on the Indonesian island of Flores to the Denisovans in Siberia, our ancestors may have encountered a variety of other hominins when they spread out of Africa. Just this year, researchers reported a new species from the Philippines.

Anthropologists are realizing that our Homo sapiens ancestors had much more contact with other human species than previously thought. Today, human evolution looks less like Darwin’s tree and more like a muddy, braided stream.

Person in white lab coat, cap, and goggles, with liquid-filled test tubes.

The rise of biomolecular archaeology means new opportunities for interdisciplinary collaboration among field- and lab-based scientists. Image via Christina Warinner.

Ancient DNA reveals old relationships

Many recent discoveries have been made possible by the new science of ancient DNA.

Since scientists fully sequenced the first ancient human genome in 2010, data from thousands of individuals have shed new insights on our species’ origins and early history.

One shocking discovery is that although our lineages split up to 800,000 years ago, modern humans and Neanderthals mated a number of times during the last Ice Age. This is why many people today possess some Neanderthal DNA.

In a cave, people look down from a wooden platform into an excavation.

The 2010 excavation in the East Gallery of Denisova Cave, where the ancient hominin species known as the Denisovans were discovered. Image via Bence Viola. Dept. of Anthropology, University of Toronto.

Ancient DNA is how researchers first identified the mysterious Denisovans, who interbred with us and Neanderthals. And while most studies are still conducted on bones and teeth, it is now possible to extract ancient DNA from other sources like cave dirt and 6,000-year-old chewing gum.

Genetic methods are also reconstructing individual and family relationships, and connecting ancient individuals to living peoples to end decades-long debates.

The applications go far beyond humans. Paleogenomics is yielding surprising discoveries about plants and animals from ancient seeds and skeletons hidden in the back rooms of museums.

Walls of hall lined with hundreds of animal skulls many with antlers.

Natural history museums hold a wealth of information, some of which can only be tapped through new biomolecular methods. Scientists analyze modern and fossil animal skeletons to ask questions about the past using ancient proteins. Image via Mary Prendergast at National Museums of Kenya.

Biomolecules are making the invisible visible

DNA is not the only molecule revolutionizing studies of the past.

Paleoproteomics, the study of ancient proteins, can determine the species of a fossil and recently linked a 9-foot tall, 1,300-pound extinct ape that lived nearly 2 million years ago to today’s orangutans.

Dental calculus – the hardened plaque that your dentist scrapes off your teeth – is particularly informative, revealing everything from who was drinking milk 6,000 years ago to the surprising diversity of plants, some likely medicinal, in Neanderthal diets. Calculus can help scientists understand ancient diseases and how the human gut microbiome has changed over time. Researchers even find cultural clues – bright blue lapis lazuli trapped in a medieval nun’s calculus led historians to reconsider who penned illuminated manuscripts.

Tooth and examples of powdered blue lazurite rock.

Scientists unexpectedly found lazurite pigment in calcified plaque clinging to an 11th- to 12th-century woman’s tooth, challenging the assumption that male monks were the primary makers of medieval manuscripts. Image via Christina Warinner.

Lipid residues trapped in pottery have revealed the origins of milk consumption in the Sahara and showed that oddly shaped pots found throughout Bronze and Iron Age Europe were ancient baby bottles.

Researchers use collagen-based “barcodes” of different animal species to answer questions ranging from when Asian rats arrived as castaways on Africa-bound ships to what animals were used to produce medieval parchment or even to detect microbes left by a monk’s kiss on a page.

Big data is revealing big patterns

While biomolecules help researchers zoom into microscopic detail, other approaches let them zoom out. Archaeologists have used aerial photography since the 1930s, but widely available satellite imagery now enables researchers to discover new sites and monitor existing ones at risk. Drones flying over sites help investigate how and why they were made and combat looting.

Aerial view of barren, brown landscape with a road and small hill.

Archaeologists increasingly use technology to understand how sites fit into their environment and to document sites at risk. Here, a drone captured a tell (a mound indicating build-up of ancient settlements) in the Kurdistan Region of Iraq. Image via Jason Ur.

Originally developed for space applications, scientists now use LIDAR – a remote sensing technique that uses lasers to measure distance – to map 3D surfaces and visualize landscapes here on Earth. As a result, ancient cities are emerging from dense vegetation in places like Mexico, Cambodia and South Africa.

Technologies that can peer underground from the surface, such as Ground Penetrating Radar, are also revolutionizing the field – for example, revealing previously unknown structures at Stonehenge. More and more, archaeologists are able to do their work without even digging a hole.

Brownish field with a mountain in the background and a scientist with two white rods.

Geophysical survey methods enable archaeologists to detect buried features without digging large holes, maximizing knowledge while minimizing destruction. Image via Mary Prendergast and Thomas Fitton.

Teams of archaeologists are combining big datasets in new ways to understand large-scale processes. In 2019, over 250 archaeologists pooled their findings to show that humans have altered the planet for thousands of years, for example, with a 2,000-year-old irrigation system in China. This echoes other studies that challenge the idea that the Anthropocene, the current period defined by human influences on the planet, only began in the 20th century.

New connections are raising new possibilities

These advances bring researchers together in exciting new ways. Over 140 new Nazca Lines, ancient images carved into a Peruvian desert, were discovered using artificial intelligence to sift through drone and satellite imagery. With the wealth of high-resolution satellite imagery online, teams are also turning to crowdsourcing to find new archaeological sites.

Although new partnerships among archaeologists and scientific specialists are not always tension-free, there is growing consensus that studying the past means reaching across fields.

The Open Science movement aims to makes this work accessible to all. Scientists including archaeologists are sharing data more freely within and beyond the academy. Public archaeology programs, community digs and digital museum collections are becoming common. You can even print your own copy of famous fossils from freely available 3D scans, or an archaeological coloring book in more than 30 languages.

Team of scientists addressing an outdoor classrom with many children.

Archaeologists are increasingly reaching out to communities to share their findings, for example at this school presentation in Tanzania. Image via Agness Gidna.

Efforts to make archaeology and museums more equitable and engage indigenous research partners are gaining momentum as archaeologists consider whose past is being revealed. Telling the human story requires a community of voices to do things right.

Studying the past to change our present

As new methods enable profound insight into humanity’s shared history, a challenge is to ensure that these insights are relevant and beneficial in the present and future.

In a year marked by youth-led climate strikes and heightened awareness of a planet in crisis, it may seem counterproductive to look back in time.

Yet in so doing, archaeologists are providing empirical support for climate change and revealing how ancient peoples coped with challenging environments.

As one example, studies show that while industrial meat production has serious environmental costs, transhumance – a traditional practice of seasonally moving livestock, now recognized by UNESCO as intangible cultural heritage – is not only light on the land today, but helped promote biodiversity and healthy landscapes in the past.

Archaeologists today are contributing their methods, data and perspectives toward a vision for a less damaged, more just planet. While it’s difficult to predict exactly what the next century holds in terms of archaeological discoveries, a new focus on “usable pasts” points in a positive direction.

Elizabeth Sawchuk, Postdoctoral Fellow and Research Assistant Professor of Anthropology, Stony Brook University (The State University of New York) and Mary Prendergast, Professor of Anthropology, Saint Louis University – Madrid

This article is republished from The Conversation under a Creative Commons license. Read the original article.

Bottom line: Twenty years of archeological discoveries and newest ideas about human evolution.

The Conversation



from EarthSky https://ift.tt/2N5V38e
Brown, barren canyon with many layers of rock.

Nearly a century ago, archaeologists started to shift the focus of human origins research from Europe to Africa’s ‘cradles of humankind’ like Oldupai (Olduvai) Gorge in Tanzania. What will the next big shifts be? Image via Manuel Domínguez-Rodrigo.

By Elizabeth Sawchuk, Stony Brook University (The State University of New York) and Mary Prendergast, Saint Louis University – Madrid

In 1924, a 3-year-old child’s skull found in South Africa forever changed how people think about human origins.

The Taung Child, our first encounter with an ancient group of proto-humans or hominins called australopithecines, was a turning point in the study of human evolution. This discovery shifted the focus of human origins research from Europe and Asia onto Africa, setting the stage for the last century of research on the continent and into its “Cradles of Humankind.”

Few people back then would’ve been able to predict what scientists know about evolution today, and now the pace of discovery is faster than ever. Even since the turn of the 21st century, human origins textbooks have been rewritten over and over again. Just 20 years ago, no one could have imagined what scientists know two decades later about humanity’s deep past, let alone how much knowledge could be extracted from a thimble of dirt, a scrape of dental plaque or satellites in space.

Human fossils are outgrowing the family tree

In Africa, there are now several fossil candidates for the earliest hominin dated to between 5 and 7 million years ago, when we know humans likely split off from other Great Apes based on differences in our DNA.

Although discovered in the 1990s, publication of the 4.4 million year old skeleton nicknamed “Ardi” in 2009 changed scientists’ views on how hominins began walking.

Rounding out our new relatives are a few australopithecines, including Australopithecus deryiremeda and Australopithecus sediba, as well as a potentially late-surviving species of early Homo that reignited debate about when humans first began burying their dead.

Human skull, much flatter head than a modern human.

Fossils like that of Australopithecus sediba, discovered in South Africa by a 9-year-old boy, are reshaping the human family tree. Image via Brett Eloff/ Courtesy Prof Berger and Wits University.

Perspectives on our own species have also changed. Archaeologists previously thought Homo sapiens evolved in Africa around 200,000 years ago, but the story has become more complicated. Fossils
discovered in Morocco have pushed that date back to 300,000 years ago, consistent with ancient DNA evidence. This raises doubts that our species emerged in any single place.

This century has also brought unexpected discoveries from Europe and Asia. From enigmatic “hobbits” on the Indonesian island of Flores to the Denisovans in Siberia, our ancestors may have encountered a variety of other hominins when they spread out of Africa. Just this year, researchers reported a new species from the Philippines.

Anthropologists are realizing that our Homo sapiens ancestors had much more contact with other human species than previously thought. Today, human evolution looks less like Darwin’s tree and more like a muddy, braided stream.

Person in white lab coat, cap, and goggles, with liquid-filled test tubes.

The rise of biomolecular archaeology means new opportunities for interdisciplinary collaboration among field- and lab-based scientists. Image via Christina Warinner.

Ancient DNA reveals old relationships

Many recent discoveries have been made possible by the new science of ancient DNA.

Since scientists fully sequenced the first ancient human genome in 2010, data from thousands of individuals have shed new insights on our species’ origins and early history.

One shocking discovery is that although our lineages split up to 800,000 years ago, modern humans and Neanderthals mated a number of times during the last Ice Age. This is why many people today possess some Neanderthal DNA.

In a cave, people look down from a wooden platform into an excavation.

The 2010 excavation in the East Gallery of Denisova Cave, where the ancient hominin species known as the Denisovans were discovered. Image via Bence Viola. Dept. of Anthropology, University of Toronto.

Ancient DNA is how researchers first identified the mysterious Denisovans, who interbred with us and Neanderthals. And while most studies are still conducted on bones and teeth, it is now possible to extract ancient DNA from other sources like cave dirt and 6,000-year-old chewing gum.

Genetic methods are also reconstructing individual and family relationships, and connecting ancient individuals to living peoples to end decades-long debates.

The applications go far beyond humans. Paleogenomics is yielding surprising discoveries about plants and animals from ancient seeds and skeletons hidden in the back rooms of museums.

Walls of hall lined with hundreds of animal skulls many with antlers.

Natural history museums hold a wealth of information, some of which can only be tapped through new biomolecular methods. Scientists analyze modern and fossil animal skeletons to ask questions about the past using ancient proteins. Image via Mary Prendergast at National Museums of Kenya.

Biomolecules are making the invisible visible

DNA is not the only molecule revolutionizing studies of the past.

Paleoproteomics, the study of ancient proteins, can determine the species of a fossil and recently linked a 9-foot tall, 1,300-pound extinct ape that lived nearly 2 million years ago to today’s orangutans.

Dental calculus – the hardened plaque that your dentist scrapes off your teeth – is particularly informative, revealing everything from who was drinking milk 6,000 years ago to the surprising diversity of plants, some likely medicinal, in Neanderthal diets. Calculus can help scientists understand ancient diseases and how the human gut microbiome has changed over time. Researchers even find cultural clues – bright blue lapis lazuli trapped in a medieval nun’s calculus led historians to reconsider who penned illuminated manuscripts.

Tooth and examples of powdered blue lazurite rock.

Scientists unexpectedly found lazurite pigment in calcified plaque clinging to an 11th- to 12th-century woman’s tooth, challenging the assumption that male monks were the primary makers of medieval manuscripts. Image via Christina Warinner.

Lipid residues trapped in pottery have revealed the origins of milk consumption in the Sahara and showed that oddly shaped pots found throughout Bronze and Iron Age Europe were ancient baby bottles.

Researchers use collagen-based “barcodes” of different animal species to answer questions ranging from when Asian rats arrived as castaways on Africa-bound ships to what animals were used to produce medieval parchment or even to detect microbes left by a monk’s kiss on a page.

Big data is revealing big patterns

While biomolecules help researchers zoom into microscopic detail, other approaches let them zoom out. Archaeologists have used aerial photography since the 1930s, but widely available satellite imagery now enables researchers to discover new sites and monitor existing ones at risk. Drones flying over sites help investigate how and why they were made and combat looting.

Aerial view of barren, brown landscape with a road and small hill.

Archaeologists increasingly use technology to understand how sites fit into their environment and to document sites at risk. Here, a drone captured a tell (a mound indicating build-up of ancient settlements) in the Kurdistan Region of Iraq. Image via Jason Ur.

Originally developed for space applications, scientists now use LIDAR – a remote sensing technique that uses lasers to measure distance – to map 3D surfaces and visualize landscapes here on Earth. As a result, ancient cities are emerging from dense vegetation in places like Mexico, Cambodia and South Africa.

Technologies that can peer underground from the surface, such as Ground Penetrating Radar, are also revolutionizing the field – for example, revealing previously unknown structures at Stonehenge. More and more, archaeologists are able to do their work without even digging a hole.

Brownish field with a mountain in the background and a scientist with two white rods.

Geophysical survey methods enable archaeologists to detect buried features without digging large holes, maximizing knowledge while minimizing destruction. Image via Mary Prendergast and Thomas Fitton.

Teams of archaeologists are combining big datasets in new ways to understand large-scale processes. In 2019, over 250 archaeologists pooled their findings to show that humans have altered the planet for thousands of years, for example, with a 2,000-year-old irrigation system in China. This echoes other studies that challenge the idea that the Anthropocene, the current period defined by human influences on the planet, only began in the 20th century.

New connections are raising new possibilities

These advances bring researchers together in exciting new ways. Over 140 new Nazca Lines, ancient images carved into a Peruvian desert, were discovered using artificial intelligence to sift through drone and satellite imagery. With the wealth of high-resolution satellite imagery online, teams are also turning to crowdsourcing to find new archaeological sites.

Although new partnerships among archaeologists and scientific specialists are not always tension-free, there is growing consensus that studying the past means reaching across fields.

The Open Science movement aims to makes this work accessible to all. Scientists including archaeologists are sharing data more freely within and beyond the academy. Public archaeology programs, community digs and digital museum collections are becoming common. You can even print your own copy of famous fossils from freely available 3D scans, or an archaeological coloring book in more than 30 languages.

Team of scientists addressing an outdoor classrom with many children.

Archaeologists are increasingly reaching out to communities to share their findings, for example at this school presentation in Tanzania. Image via Agness Gidna.

Efforts to make archaeology and museums more equitable and engage indigenous research partners are gaining momentum as archaeologists consider whose past is being revealed. Telling the human story requires a community of voices to do things right.

Studying the past to change our present

As new methods enable profound insight into humanity’s shared history, a challenge is to ensure that these insights are relevant and beneficial in the present and future.

In a year marked by youth-led climate strikes and heightened awareness of a planet in crisis, it may seem counterproductive to look back in time.

Yet in so doing, archaeologists are providing empirical support for climate change and revealing how ancient peoples coped with challenging environments.

As one example, studies show that while industrial meat production has serious environmental costs, transhumance – a traditional practice of seasonally moving livestock, now recognized by UNESCO as intangible cultural heritage – is not only light on the land today, but helped promote biodiversity and healthy landscapes in the past.

Archaeologists today are contributing their methods, data and perspectives toward a vision for a less damaged, more just planet. While it’s difficult to predict exactly what the next century holds in terms of archaeological discoveries, a new focus on “usable pasts” points in a positive direction.

Elizabeth Sawchuk, Postdoctoral Fellow and Research Assistant Professor of Anthropology, Stony Brook University (The State University of New York) and Mary Prendergast, Professor of Anthropology, Saint Louis University – Madrid

This article is republished from The Conversation under a Creative Commons license. Read the original article.

Bottom line: Twenty years of archeological discoveries and newest ideas about human evolution.

The Conversation



from EarthSky https://ift.tt/2N5V38e

New view of Milky Way’s center

On January 5, 2020, astronomers at the American Astronomical Society annual meeting in Honolulu, Hawaii, presented a new, extremely crisp infrared image of the center of our Milky Way galaxy.

The panoramic image spans a distance of more than 600 light-years, and reveals new details within the galactic center’s dense swirls of gas and dust. According to a NASA statement about the image:

Among the features coming into focus are the jutting curves of the Arches Cluster containing the densest concentration of stars in our galaxy, as well as the Quintuplet Cluster with stars a million times brighter than our sun. Our galaxy’s black hole takes shape with a glimpse of the fiery-looking ring of gas surrounding it.

EarthSky 2020 lunar calendars are available! Nearly sold out. Order now!

Long oval of swirls, narrowing toward both ends.

View larger. | Composite infrared image of the center of our Milky Way galaxy. It shows a region spanning 600+ light-years. The new image is helping scientists understand how many massive stars are forming in our galaxy’s center. Image via NASA/ SOFIA/ JPL-Caltech/ ESA/ Herschel.

Astronomers created the image using a special infrared camera aboard NASA’s SOFIA (Stratospheric Observatory for Infrared Astronomy) flying telescope, that captured images of warm, galactic material emitting wavelengths of light that other telescopes could not detect. The data was collected in July 2019, during SOFIA’s annual deployment to Christchurch, New Zealand, where scientists study the skies over the Southern Hemisphere. The new panoramic image combines SOFIA’s new perspective with previous data exposing very hot and cold material from NASA’s Spitzer Space Telescope and the European Space Agency’s Herschel Space Observatory.

The astronomers said this new image opens a door to future research into how massive stars form and into what’s feeding the supermassive black hole at our galaxy’s core. James Radomski at NASA’s Ames Research Center commented:

It’s incredible to see our galactic center in detail we’ve never seen before. Studying this area has been like trying to assemble a puzzle with missing pieces. The SOFIA data fills in some of the holes, putting us significantly closer to having a complete picture.

Here’s more from NASA’s statement about the image:

The Milky Way’s central regions have significantly more of the dense gas and dust that are the building blocks for new stars compared to other parts of the galaxy. Yet, there are 10 times fewer massive stars born here than expected. Understanding why this discrepancy exists has been difficult because of all the dust between Earth and the galactic core getting in the way – but observing with infrared light offers a closer look at the situation.

The new infrared data illuminates structures indicative of star birth near the Quintuplet Cluster and warm material near the Arches Cluster that could be the seeds for new stars.

Scientists can also more clearly see the material that may be feeding the ring around our galaxy’s central supermassive black hole. The ring is about 10 light-years in diameter and plays a key role in bringing matter closer to the black hole, where it may eventually be devoured. The origin of this ring has long been a puzzle for scientists because it may be depleted over time, but the SOFIA data reveal several structures which could represent material being incorporated into it.

An overview paper highlighting initial results has been submitted for publication to the Astrophysical Journal.

Bottom line: New image shows the center of the Milky Way galaxy in never-seen-before detail.

Via NASA



from EarthSky https://ift.tt/2t0NGYK

On January 5, 2020, astronomers at the American Astronomical Society annual meeting in Honolulu, Hawaii, presented a new, extremely crisp infrared image of the center of our Milky Way galaxy.

The panoramic image spans a distance of more than 600 light-years, and reveals new details within the galactic center’s dense swirls of gas and dust. According to a NASA statement about the image:

Among the features coming into focus are the jutting curves of the Arches Cluster containing the densest concentration of stars in our galaxy, as well as the Quintuplet Cluster with stars a million times brighter than our sun. Our galaxy’s black hole takes shape with a glimpse of the fiery-looking ring of gas surrounding it.

EarthSky 2020 lunar calendars are available! Nearly sold out. Order now!

Long oval of swirls, narrowing toward both ends.

View larger. | Composite infrared image of the center of our Milky Way galaxy. It shows a region spanning 600+ light-years. The new image is helping scientists understand how many massive stars are forming in our galaxy’s center. Image via NASA/ SOFIA/ JPL-Caltech/ ESA/ Herschel.

Astronomers created the image using a special infrared camera aboard NASA’s SOFIA (Stratospheric Observatory for Infrared Astronomy) flying telescope, that captured images of warm, galactic material emitting wavelengths of light that other telescopes could not detect. The data was collected in July 2019, during SOFIA’s annual deployment to Christchurch, New Zealand, where scientists study the skies over the Southern Hemisphere. The new panoramic image combines SOFIA’s new perspective with previous data exposing very hot and cold material from NASA’s Spitzer Space Telescope and the European Space Agency’s Herschel Space Observatory.

The astronomers said this new image opens a door to future research into how massive stars form and into what’s feeding the supermassive black hole at our galaxy’s core. James Radomski at NASA’s Ames Research Center commented:

It’s incredible to see our galactic center in detail we’ve never seen before. Studying this area has been like trying to assemble a puzzle with missing pieces. The SOFIA data fills in some of the holes, putting us significantly closer to having a complete picture.

Here’s more from NASA’s statement about the image:

The Milky Way’s central regions have significantly more of the dense gas and dust that are the building blocks for new stars compared to other parts of the galaxy. Yet, there are 10 times fewer massive stars born here than expected. Understanding why this discrepancy exists has been difficult because of all the dust between Earth and the galactic core getting in the way – but observing with infrared light offers a closer look at the situation.

The new infrared data illuminates structures indicative of star birth near the Quintuplet Cluster and warm material near the Arches Cluster that could be the seeds for new stars.

Scientists can also more clearly see the material that may be feeding the ring around our galaxy’s central supermassive black hole. The ring is about 10 light-years in diameter and plays a key role in bringing matter closer to the black hole, where it may eventually be devoured. The origin of this ring has long been a puzzle for scientists because it may be depleted over time, but the SOFIA data reveal several structures which could represent material being incorporated into it.

An overview paper highlighting initial results has been submitted for publication to the Astrophysical Journal.

Bottom line: New image shows the center of the Milky Way galaxy in never-seen-before detail.

Via NASA



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What is a full moon?

Full moon next to a large Christmas-lighted tower.

John Jairu Lumbera Roldan caught the full moon on December 11-12, 2019 and wrote: “The last full moon of this decade. Love, from the Philippines.” Back at you, John!

The moon appears full to the eye for two to three nights. However, astronomers regard the moon as full at a precisely defined instant, when the moon is exactly 180 degrees opposite the sun in ecliptic longitude.

Read more: Full Wolf Moon eclipse on January 10

Read more: What are the full moon names?

EarthSky 2020 lunar calendars are available! They make great gifts. Order now. Going fast!

Full moon reflecting in a bay, with a very small couple embracing in the lower left corner.

A kiss under the full moon of November 3, 2017, via our friend Steven Sweet of Lunar 101-Moon Book. He was at Port Credit, a neighborhood in the city of Mississauga, Ontario, Canada … at the mouth of the Credit River on the north shore of Lake Ontario.

Why does a full moon look full? Remember that half the moon is always illuminated by the sun. That lighted half is the moon’s day side. In order to appear full to us on Earth, we have to see the entire day side of the moon. That happens only when the moon is opposite the sun in our sky. So a full moon looks full because it’s opposite the sun.

That’s also why every full moon rises in the east around sunset – climbs highest up for the night midway between sunset and sunrise (around midnight) – and sets around sunrise. Stand outside tonight around sunset and look for the moon. Sun going down while the moon is coming up? That’s a full moon, or close to one.

Just be aware that the moon will look full for at least a couple of night around the instant of full moon.

Diagram showing a full moon on the opposite side of Earth from the sun.

A full moon is opposite the sun. We see all of its dayside. Illustration via Bob King.

Often, you’ll find two different dates on calendars for the date of full moon. That’s because some calendars list moon phases in Coordinated Universal Time, also called Universal Time Coordinated (UTC). And other calendars list moon phases in local time, a clock time of a specific place, usually the place that made and distributed the calendars. Translate UTC to your local time.

Want to know the instant of full moon in your part of the world, as well as the moonrise and moonset times? Visit Sunrise Sunset Calendars, remembering to check the moon phases plus moonrise and moonset boxes.

If a full moon is opposite the sun, why doesn’t Earth’s shadow fall on the moon at every full moon? The reason is that the moon’s orbit is tilted by 5.1 degrees with respect to Earth’s orbit around the sun. At every full moon, Earth’s shadow sweeps near the moon. But, in most months, there’s no eclipse.

Oblique diagram of earth, sun, moon orbits. Moon orbit slightly slanted in relation to Earth's.

A full moon normally passes above or below Earth’s shadow, with no eclipse. Illustration by Bob King.

As the moon orbits Earth, it changes phase in an orderly way. Follow these links to understand the various phases of the moon.

New moon
Waxing crescent moon
First quarter moon
Waxing gibbous moon
Full moon
Waning gibbous moon
Last quarter moon
Waning crescent moon

EarthSky lunar calendars show the phases of the moon throughout 2020. They make great gifts. Order now. Going fast!

Bottom line: Full moon happens when the moon is most opposite the sun for any given month. The next full moon is January 10 at 19:21 UTC. Translate UTC to your time).

Read more: 4 keys to understanding moon phases



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Full moon next to a large Christmas-lighted tower.

John Jairu Lumbera Roldan caught the full moon on December 11-12, 2019 and wrote: “The last full moon of this decade. Love, from the Philippines.” Back at you, John!

The moon appears full to the eye for two to three nights. However, astronomers regard the moon as full at a precisely defined instant, when the moon is exactly 180 degrees opposite the sun in ecliptic longitude.

Read more: Full Wolf Moon eclipse on January 10

Read more: What are the full moon names?

EarthSky 2020 lunar calendars are available! They make great gifts. Order now. Going fast!

Full moon reflecting in a bay, with a very small couple embracing in the lower left corner.

A kiss under the full moon of November 3, 2017, via our friend Steven Sweet of Lunar 101-Moon Book. He was at Port Credit, a neighborhood in the city of Mississauga, Ontario, Canada … at the mouth of the Credit River on the north shore of Lake Ontario.

Why does a full moon look full? Remember that half the moon is always illuminated by the sun. That lighted half is the moon’s day side. In order to appear full to us on Earth, we have to see the entire day side of the moon. That happens only when the moon is opposite the sun in our sky. So a full moon looks full because it’s opposite the sun.

That’s also why every full moon rises in the east around sunset – climbs highest up for the night midway between sunset and sunrise (around midnight) – and sets around sunrise. Stand outside tonight around sunset and look for the moon. Sun going down while the moon is coming up? That’s a full moon, or close to one.

Just be aware that the moon will look full for at least a couple of night around the instant of full moon.

Diagram showing a full moon on the opposite side of Earth from the sun.

A full moon is opposite the sun. We see all of its dayside. Illustration via Bob King.

Often, you’ll find two different dates on calendars for the date of full moon. That’s because some calendars list moon phases in Coordinated Universal Time, also called Universal Time Coordinated (UTC). And other calendars list moon phases in local time, a clock time of a specific place, usually the place that made and distributed the calendars. Translate UTC to your local time.

Want to know the instant of full moon in your part of the world, as well as the moonrise and moonset times? Visit Sunrise Sunset Calendars, remembering to check the moon phases plus moonrise and moonset boxes.

If a full moon is opposite the sun, why doesn’t Earth’s shadow fall on the moon at every full moon? The reason is that the moon’s orbit is tilted by 5.1 degrees with respect to Earth’s orbit around the sun. At every full moon, Earth’s shadow sweeps near the moon. But, in most months, there’s no eclipse.

Oblique diagram of earth, sun, moon orbits. Moon orbit slightly slanted in relation to Earth's.

A full moon normally passes above or below Earth’s shadow, with no eclipse. Illustration by Bob King.

As the moon orbits Earth, it changes phase in an orderly way. Follow these links to understand the various phases of the moon.

New moon
Waxing crescent moon
First quarter moon
Waxing gibbous moon
Full moon
Waning gibbous moon
Last quarter moon
Waning crescent moon

EarthSky lunar calendars show the phases of the moon throughout 2020. They make great gifts. Order now. Going fast!

Bottom line: Full moon happens when the moon is most opposite the sun for any given month. The next full moon is January 10 at 19:21 UTC. Translate UTC to your time).

Read more: 4 keys to understanding moon phases



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