Watch it get hotter, 1880-2017

Check out this 40-second animation showing shows high and low temperatures of countries around the world over the period 1880 to 2017, created by researcher Antti Lipponen from the Finnish Meteorological Institute.

The animated timeline, based on NASA satellite data, shows unusual dips in year-to-year temperatures (in blue) and above-average spikes (in red).

Lipponen said:

It doesn’t look as if climate change is slowing down at all. Quite the opposite: the planet has warmed extremely quickly in the past two decades.

Bottom line: Animated timeline showing temperature anomalies by country, from 1880-2017 based on NASA data.



from EarthSky https://ift.tt/2wG9QhO

Check out this 40-second animation showing shows high and low temperatures of countries around the world over the period 1880 to 2017, created by researcher Antti Lipponen from the Finnish Meteorological Institute.

The animated timeline, based on NASA satellite data, shows unusual dips in year-to-year temperatures (in blue) and above-average spikes (in red).

Lipponen said:

It doesn’t look as if climate change is slowing down at all. Quite the opposite: the planet has warmed extremely quickly in the past two decades.

Bottom line: Animated timeline showing temperature anomalies by country, from 1880-2017 based on NASA data.



from EarthSky https://ift.tt/2wG9QhO

How far could you travel and still see Earth?

Earth and moon, as seen from Mars by NASA’s Curiosity rover on January 31, 2014. Read more about this image.

How far away from Earth can we be and see it still with our own eyes?

To find the answer, let’s take an imaginary trip through the solar system, to see how Earth looks from various other places, in our own neighborhood of space. Spacecraft exploring our solar system have given us marvelous views of Earth.

First, imagine blasting off and being about 200 miles (300 km) above Earth’s surface. That’s about the height of the orbit of the International Space Station (ISS). From the window of ISS, the surface of the Earth looms large. In the daytime, you can clearly see major landforms. At night, from Earth orbit, you see the lights of Earth’s cities.

Earth in daylight, from ISS in 2012. The U.S. Great Lakes shine in the sun. Read more about this image.

Earth in daylight, from ISS in 2012. The U.S. Great Lakes shine in the sun. Read more about this image.

ng at an altitude of about 240 miles over the eastern North Atlantic, the Expedition 30 crew aboard the International Space Station photographed this nighttime scene. This view looks northeastward. Center point coordinates are 46.8 degrees north latitude and 14.3 degrees west longitude. The night lights of the cities of Ireland, in the foreground, and the United Kingdom, in the back and to the right, are contrasted by the bright sunrise in the background. The greens and purples of the Aurora Borealis are seen along the rest of the horizon. This image was taken on March 28, 2012.

Earth at night, from ISS in 2012. Ireland is in the foreground, and the United Kingdom in the back and to the right. A bright sunrise is in the background. Greens and purples shows an aurora borealis along the rest of the horizon.

Let’s get farther away, say, the distance of the orbit of the moon.

As we pass the moon – some quarter million miles (about 380,000 km) away – Earth looks like a bright ball in space. It’s not terribly different from the way the moon looks to us.

The first images of the Earth from the moon came from the Apollo mission. Apollo 8 in 1968 was the first human spaceflight to leave Earth orbit. It was the first earthly spacecraft to be captured by and escape from the gravitational field of another celestial body, in this case the moon.

It was the first voyage in which humans visited another world and returned to return to Earth.

Earth seen from moon via Apollo 8 astronauts in 1968. Image via NASA.

In the decades since Voyager first began traveling outward, moon exploration has become more common. The robotic Kaguya spacecraft orbited around Earth’s moon in 2007. Launched by Japan, and officially named the Selenological and Engineering Explorer (SELENE), Kaguya studied the origin and evolution of the moon. The frame below is from Kaguya’s onboard HDTV camera.

The robotic Kaguya spacecraft orbited around Earth's moon in 2007. Japan launched this scientific mission of the Selenological and Engineering Explorer (SELENE), nicknamed Kaguya, in order to study the origin and evolution of the moon. This frame is from Kaguya's onboard HDTV camera.

Earth viewed from the moon by Kaguya in 2007. Image via SELENE Team, JAXA, NHK

Another image from ___, which captured the Japanese craft got footage and stills of Earth setting. Remember that, if you were on the moon, you would not see Earth rise or set. But spacecraft in orbit around the moon do experience this scene.

Another image from Kaguya, which got footage and stills of Earth setting. Remember that, if you were on the moon, you would not see Earth rise or set. But spacecraft in orbit around the moon do experience this scene.

Now let’s keep moving outward, until we can see both the Earth and moon together in space. The next picture was mind-blowing when first released. It shows a crescent-shaped Earth and moon – the first of its kind ever taken by a spacecraft – on September 18, 1977.

This picture of a crescent-shaped Earth and moon – 1st of its kind ever taken by a spacecraft – was recorded September 18, 1977, by Voyager 1 at a distance of 7.25 million miles (11.66 million km) from Earth. The moon is at the top of the picture and beyond the Earth as viewed by Voyager. Image via NASA.

Since 1977, many robot spacecraft have ventured outward into our solar system. The mosaic below shows images of Earth and the moon acquired by the multispectral imager on the Near Earth Asteroid Rendezvous Spacecraft (NEAR) on January 23, 1998, 19 hours after the spacecraft swung by Earth on its way to the asteroid 433 Eros. The images of both were taken from a range of 250,000 miles (400,000 km), approximately the same as the distance between the two bodies.

This mosaic shows images of Earth and the moon acquired by the multispectral imager on the Near Earth Asteroid Rendezvous Spacecraft (NEAR) on January 23, 1998, 19 hours after the spacecraft swung by Earth on its way to the asteroid 433 Eros. The images of both were taken from a range of 250,000 miles (400,000 kilometers), approximately the same as the distance between the two bodies. Read more about this image.

Earth and moon seen by NEAR spacecraft in 1998.

Speeding outward from the Earth and moon system, you pass the orbits of the planets Mars, Jupiter and Saturn. From all of these worlds, Earth looks like a star – which gets fainter as you get farther away.

View larger. | Earth seen behind the rings of Saturn. See us in the lower right? Mars and Venus are in the upper left. Image via the Cassini spacecraft, July 19, 2013.

View larger. | Earth seen behind the rings of Saturn. See us in the lower right? Mars and Venus are in the upper left. Image via the Cassini spacecraft, July 19, 2013.

This is the famous image known as Pale Blue Dot. It's a photograph of Earth taken on February 14, 1990, by the Voyager 1 space probe from a record distance of about 6 billion kilometers (3.7 billion miles).

This is the famous image known as Pale Blue Dot. It’s a photograph of Earth taken on February 14, 1990, by the Voyager 1 space probe from a record distance of about 6 billion kilometers (3.7 billion miles). Earth is the blueish-white speck approximately halfway down the brown band to the right.

The images above are from Saturn, the sixth planet outward in orbit around the sun. I’ve never seen any image of Earth from Uranus or Neptune or any other body beyond Saturn’s orbit. Only five spacecraft from Earth – the two Voyager spacecraft, the two Pioneers, and the New Horizons spacecraft, which passed Pluto in 2015 – have ever ventured that far. Those craft weren’t designed to look back at Earth, and, to my knowledge, they didn’t capture images of Earth from distances beyond Saturn.

But, speaking theoretically now, could Earth be seen from distances beyond Saturn?

Speaking only in terms of Earth’s brightness, the answer is yes. Our world doesn’t become too faint to see with the eye alone until far beyond Neptune’s orbit, at around 9 billion miles (14 billion km) from home. Now consider Pluto’s orbit. It’s highly elliptical, stretching from just 2.7 billion miles (4.4 billion km) to over 4.5 billion miles (7.3 billion km) from the sun. Pluto is within the limiting distance at which – if we just consider brightness alone, no other factors – we should be able to see Earth with the eye alone.

But there is another factor. As you go outward from Earth, our world appears closer and closer to the blazing sun. As you get farther away, the sun’s glare begins to overwhelm the view of Earth. From Pluto – even though Earth would be bright enough to see – you probably couldn’t see it in the sun’s glare.

So that is the answer. Although no one knows for sure because no one has tried it (and because human eyesight varies from person to person), the Earth would become impossible to see with the eye somewhere beyond Saturn’s orbit.

Now let’s change the game. Let’s say we could use instruments, and not just the eye alone. Suppose intrepid astronaut-astronomers went to Pluto. Suppose they took all the instruments they needed to view Earth in the sun’s glare. Could they use telescopes, obscuring disks, and other techniques to get a glimpse of Earth? Maybe!

But it still wouldn’t be easy.

Read more: Wikipedia has a long write-up on extraterrestrial skies

Bottom line: How far away in space could you view Earth with the eye alone? Considering only brightness, the answer is about 9 billion miles (14 billion km) away. In practice, though, seeing it from that distance would be a challenge because the sun’s glare would overwhelm the view of Earth.



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Earth and moon, as seen from Mars by NASA’s Curiosity rover on January 31, 2014. Read more about this image.

How far away from Earth can we be and see it still with our own eyes?

To find the answer, let’s take an imaginary trip through the solar system, to see how Earth looks from various other places, in our own neighborhood of space. Spacecraft exploring our solar system have given us marvelous views of Earth.

First, imagine blasting off and being about 200 miles (300 km) above Earth’s surface. That’s about the height of the orbit of the International Space Station (ISS). From the window of ISS, the surface of the Earth looms large. In the daytime, you can clearly see major landforms. At night, from Earth orbit, you see the lights of Earth’s cities.

Earth in daylight, from ISS in 2012. The U.S. Great Lakes shine in the sun. Read more about this image.

Earth in daylight, from ISS in 2012. The U.S. Great Lakes shine in the sun. Read more about this image.

ng at an altitude of about 240 miles over the eastern North Atlantic, the Expedition 30 crew aboard the International Space Station photographed this nighttime scene. This view looks northeastward. Center point coordinates are 46.8 degrees north latitude and 14.3 degrees west longitude. The night lights of the cities of Ireland, in the foreground, and the United Kingdom, in the back and to the right, are contrasted by the bright sunrise in the background. The greens and purples of the Aurora Borealis are seen along the rest of the horizon. This image was taken on March 28, 2012.

Earth at night, from ISS in 2012. Ireland is in the foreground, and the United Kingdom in the back and to the right. A bright sunrise is in the background. Greens and purples shows an aurora borealis along the rest of the horizon.

Let’s get farther away, say, the distance of the orbit of the moon.

As we pass the moon – some quarter million miles (about 380,000 km) away – Earth looks like a bright ball in space. It’s not terribly different from the way the moon looks to us.

The first images of the Earth from the moon came from the Apollo mission. Apollo 8 in 1968 was the first human spaceflight to leave Earth orbit. It was the first earthly spacecraft to be captured by and escape from the gravitational field of another celestial body, in this case the moon.

It was the first voyage in which humans visited another world and returned to return to Earth.

Earth seen from moon via Apollo 8 astronauts in 1968. Image via NASA.

In the decades since Voyager first began traveling outward, moon exploration has become more common. The robotic Kaguya spacecraft orbited around Earth’s moon in 2007. Launched by Japan, and officially named the Selenological and Engineering Explorer (SELENE), Kaguya studied the origin and evolution of the moon. The frame below is from Kaguya’s onboard HDTV camera.

The robotic Kaguya spacecraft orbited around Earth's moon in 2007. Japan launched this scientific mission of the Selenological and Engineering Explorer (SELENE), nicknamed Kaguya, in order to study the origin and evolution of the moon. This frame is from Kaguya's onboard HDTV camera.

Earth viewed from the moon by Kaguya in 2007. Image via SELENE Team, JAXA, NHK

Another image from ___, which captured the Japanese craft got footage and stills of Earth setting. Remember that, if you were on the moon, you would not see Earth rise or set. But spacecraft in orbit around the moon do experience this scene.

Another image from Kaguya, which got footage and stills of Earth setting. Remember that, if you were on the moon, you would not see Earth rise or set. But spacecraft in orbit around the moon do experience this scene.

Now let’s keep moving outward, until we can see both the Earth and moon together in space. The next picture was mind-blowing when first released. It shows a crescent-shaped Earth and moon – the first of its kind ever taken by a spacecraft – on September 18, 1977.

This picture of a crescent-shaped Earth and moon – 1st of its kind ever taken by a spacecraft – was recorded September 18, 1977, by Voyager 1 at a distance of 7.25 million miles (11.66 million km) from Earth. The moon is at the top of the picture and beyond the Earth as viewed by Voyager. Image via NASA.

Since 1977, many robot spacecraft have ventured outward into our solar system. The mosaic below shows images of Earth and the moon acquired by the multispectral imager on the Near Earth Asteroid Rendezvous Spacecraft (NEAR) on January 23, 1998, 19 hours after the spacecraft swung by Earth on its way to the asteroid 433 Eros. The images of both were taken from a range of 250,000 miles (400,000 km), approximately the same as the distance between the two bodies.

This mosaic shows images of Earth and the moon acquired by the multispectral imager on the Near Earth Asteroid Rendezvous Spacecraft (NEAR) on January 23, 1998, 19 hours after the spacecraft swung by Earth on its way to the asteroid 433 Eros. The images of both were taken from a range of 250,000 miles (400,000 kilometers), approximately the same as the distance between the two bodies. Read more about this image.

Earth and moon seen by NEAR spacecraft in 1998.

Speeding outward from the Earth and moon system, you pass the orbits of the planets Mars, Jupiter and Saturn. From all of these worlds, Earth looks like a star – which gets fainter as you get farther away.

View larger. | Earth seen behind the rings of Saturn. See us in the lower right? Mars and Venus are in the upper left. Image via the Cassini spacecraft, July 19, 2013.

View larger. | Earth seen behind the rings of Saturn. See us in the lower right? Mars and Venus are in the upper left. Image via the Cassini spacecraft, July 19, 2013.

This is the famous image known as Pale Blue Dot. It's a photograph of Earth taken on February 14, 1990, by the Voyager 1 space probe from a record distance of about 6 billion kilometers (3.7 billion miles).

This is the famous image known as Pale Blue Dot. It’s a photograph of Earth taken on February 14, 1990, by the Voyager 1 space probe from a record distance of about 6 billion kilometers (3.7 billion miles). Earth is the blueish-white speck approximately halfway down the brown band to the right.

The images above are from Saturn, the sixth planet outward in orbit around the sun. I’ve never seen any image of Earth from Uranus or Neptune or any other body beyond Saturn’s orbit. Only five spacecraft from Earth – the two Voyager spacecraft, the two Pioneers, and the New Horizons spacecraft, which passed Pluto in 2015 – have ever ventured that far. Those craft weren’t designed to look back at Earth, and, to my knowledge, they didn’t capture images of Earth from distances beyond Saturn.

But, speaking theoretically now, could Earth be seen from distances beyond Saturn?

Speaking only in terms of Earth’s brightness, the answer is yes. Our world doesn’t become too faint to see with the eye alone until far beyond Neptune’s orbit, at around 9 billion miles (14 billion km) from home. Now consider Pluto’s orbit. It’s highly elliptical, stretching from just 2.7 billion miles (4.4 billion km) to over 4.5 billion miles (7.3 billion km) from the sun. Pluto is within the limiting distance at which – if we just consider brightness alone, no other factors – we should be able to see Earth with the eye alone.

But there is another factor. As you go outward from Earth, our world appears closer and closer to the blazing sun. As you get farther away, the sun’s glare begins to overwhelm the view of Earth. From Pluto – even though Earth would be bright enough to see – you probably couldn’t see it in the sun’s glare.

So that is the answer. Although no one knows for sure because no one has tried it (and because human eyesight varies from person to person), the Earth would become impossible to see with the eye somewhere beyond Saturn’s orbit.

Now let’s change the game. Let’s say we could use instruments, and not just the eye alone. Suppose intrepid astronaut-astronomers went to Pluto. Suppose they took all the instruments they needed to view Earth in the sun’s glare. Could they use telescopes, obscuring disks, and other techniques to get a glimpse of Earth? Maybe!

But it still wouldn’t be easy.

Read more: Wikipedia has a long write-up on extraterrestrial skies

Bottom line: How far away in space could you view Earth with the eye alone? Considering only brightness, the answer is about 9 billion miles (14 billion km) away. In practice, though, seeing it from that distance would be a challenge because the sun’s glare would overwhelm the view of Earth.



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Meet the Gemini “twins” before sunup on September 5 or 6

The next two mornings – September 5 and 6, 2018 – you can see see the moon near the two brightest stars of the constellation constellation Gemini the Twins. They’re called Castor and Pollux, and they’re good stars to come to know.

See how bright they are, and how close together? Even without the moon, they’re noticeable on the sky’s dome.

Gemini is the constellation of the Twins, and Castor and Pollux are often called “twin” stars. But these two stars aren’t twins; they’re really very different. Although Castor and Pollux appear close, they’re not physically related or close together in space. Pollux, the closer star, lies about 34 light-years away, while Castor resides at a distance of about 52 light-years.

If you scrutinize Castor and Pollux, you might discern their difference in color. Castor appears white in contrast to the orange glow of Pollux. A white star is a relatively hot star in the heyday of youth. An orange star is a cool star in the autumn of its years.

Moreover, Pollux’s orange color reveals that it’s a giant star. According to the star expert Jim Kaler, any star with the mass of 0.8 to 5 times solar swells up and becomes a giant star in old age.

Pollux, the nearest giant star to Earth, has a diameter of about 10 of our suns. It’s also one of the very few giant stars known to harbor a planet.

You can see the comparative size of the star Pollux and our sun in this image, as well as some other stars.

The other “twin,” Castor, is remarkable in its own right. Castor is actually six stars in one, consisting of 3 pairs of binary stars, all revolving around a common center of mass.

By the way, the moon will move out of the constellation Gemini and into the faint constellation Cancer the Crab on or near September 7, 2018.

Then, on September 9, we’ll have a new moon, with the moon transitioning out of the morning sky and into the evening sky.

Even with no moon to guide you, however, you can notice Castor and Pollux for their brightness and nearness to each other on the sky’s dome. Not sure? Try using Orion’s Belt to star-hop to Castor and Pollux (see the sky chart below):

Sky chart of the constellation Gemini via IAU. Draw an imaginary line from the easternmost star of Orion’s Belt and through the bright ruddy star Betelgeuse to locate the Gemini stars, Castor and Pollux. Click here to learn more about Orion..

Bottom line: On September 5 and 6, 2018, use the waning crescent moon to find the Gemini stars, Castor and Pollux.



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The next two mornings – September 5 and 6, 2018 – you can see see the moon near the two brightest stars of the constellation constellation Gemini the Twins. They’re called Castor and Pollux, and they’re good stars to come to know.

See how bright they are, and how close together? Even without the moon, they’re noticeable on the sky’s dome.

Gemini is the constellation of the Twins, and Castor and Pollux are often called “twin” stars. But these two stars aren’t twins; they’re really very different. Although Castor and Pollux appear close, they’re not physically related or close together in space. Pollux, the closer star, lies about 34 light-years away, while Castor resides at a distance of about 52 light-years.

If you scrutinize Castor and Pollux, you might discern their difference in color. Castor appears white in contrast to the orange glow of Pollux. A white star is a relatively hot star in the heyday of youth. An orange star is a cool star in the autumn of its years.

Moreover, Pollux’s orange color reveals that it’s a giant star. According to the star expert Jim Kaler, any star with the mass of 0.8 to 5 times solar swells up and becomes a giant star in old age.

Pollux, the nearest giant star to Earth, has a diameter of about 10 of our suns. It’s also one of the very few giant stars known to harbor a planet.

You can see the comparative size of the star Pollux and our sun in this image, as well as some other stars.

The other “twin,” Castor, is remarkable in its own right. Castor is actually six stars in one, consisting of 3 pairs of binary stars, all revolving around a common center of mass.

By the way, the moon will move out of the constellation Gemini and into the faint constellation Cancer the Crab on or near September 7, 2018.

Then, on September 9, we’ll have a new moon, with the moon transitioning out of the morning sky and into the evening sky.

Even with no moon to guide you, however, you can notice Castor and Pollux for their brightness and nearness to each other on the sky’s dome. Not sure? Try using Orion’s Belt to star-hop to Castor and Pollux (see the sky chart below):

Sky chart of the constellation Gemini via IAU. Draw an imaginary line from the easternmost star of Orion’s Belt and through the bright ruddy star Betelgeuse to locate the Gemini stars, Castor and Pollux. Click here to learn more about Orion..

Bottom line: On September 5 and 6, 2018, use the waning crescent moon to find the Gemini stars, Castor and Pollux.



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Mars’ gala summer is ending

View full-sized image. | This Project Nightflight photo – released September 2, 2018 – shows Mars in mid-August. The Project Nightflight team photographed Mars with a DSLR, a 50mm lens and a diffusion filter to render the planet’s orange-red color as naturally as possible, from the Grossmugl Star Walk in Austria. Read more about this image.

AstroLina Photography in Antarctica calls this image Planetas (Planets). He captured the arc of planets in the evening sky now by combining 21 photos into this beautiful composite. Mars is the bright object at the lower left. Read more about this image.

Don Mills wrote from Wildwood, New Jersey: “While on vacation here, we saw the last fireworks display for the season and I captured some exploding shells over the beach with planet Mars as the bright speck to the left.” Thank you, Don!

Bottom line: A last few images of a very bright Mars, from the EarthSky Community. We won’t see Mars this bright again for another 15 years!

See more photos: Moon sweeps past Mars

See more photos: Mars, the moon and a bottle rocket

See more photos: Parade of moon and planets

Read more: Mars brighter in 2018 than since 2003



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View full-sized image. | This Project Nightflight photo – released September 2, 2018 – shows Mars in mid-August. The Project Nightflight team photographed Mars with a DSLR, a 50mm lens and a diffusion filter to render the planet’s orange-red color as naturally as possible, from the Grossmugl Star Walk in Austria. Read more about this image.

AstroLina Photography in Antarctica calls this image Planetas (Planets). He captured the arc of planets in the evening sky now by combining 21 photos into this beautiful composite. Mars is the bright object at the lower left. Read more about this image.

Don Mills wrote from Wildwood, New Jersey: “While on vacation here, we saw the last fireworks display for the season and I captured some exploding shells over the beach with planet Mars as the bright speck to the left.” Thank you, Don!

Bottom line: A last few images of a very bright Mars, from the EarthSky Community. We won’t see Mars this bright again for another 15 years!

See more photos: Moon sweeps past Mars

See more photos: Mars, the moon and a bottle rocket

See more photos: Parade of moon and planets

Read more: Mars brighter in 2018 than since 2003



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Why was Jupiter’s early growth delayed?

Spectacular view of Jupiter from the Juno spacecraft, acquired April 1, 2018. Image via NASA/JPL-Caltech/SwRI/MSSS. Citizen scientists Gerald Eichstädt and Seán Doran created this image using data from the spacecraft’s JunoCam imager.

Jupiter is sometimes called the king of the planets in our solar system, due to its enormous size. It has some 300 times Earth’s mass. Jupiter is thought to have become the largest planet early in our solar system’s history. Still, questions remained about how quickly (or not) Jupiter kept growing, with earlier evidence suggesting Jupiter’s growth was delayed for about two million years. The reason for this delay was unknown. Now, astrophysicists in Switzerland think they have an answer. Their work was published August 27, 2018, in the peer-reviewed journal Nature Astronomy.

The researchers are affiliated with two organizations, NCCR PlanetS and ETHzürich. Co-author Julia Venturini explained in a statement:

We … show that Jupiter grew in different, distinct phases.

Lead author Yann Alibert added:

Especially interesting is that it is not the same kind of bodies that bring mass and energy [to Jupiter].

In other words, these scientists used computer modeling to show that – billions of years ago, early in our solar system’s history – Jupiter underwent a delayed growth phase as material of varying sizes and types accreted onto it.

Artist’s concept of a very young Jupiter. Scientists think that Jupiter, Earth and the other planets in our solar system formed from a disk of gas and dust surrounding the young sun. Image via Lawrence Livermore National Laboratory.

Planets – like Earth or Jupiter – are thought to grow by accretion from the gas-and-dust clouds, or nebulae, surrounding young stars. That is, they grow as small bits of material in the cloud collide, stick together, and become increasingly bigger. Once the planets themselves get big enough, they begin to sweep up even more material from the solar nebula, via the power of their gravitational pull.

So what happened during these different phases of Jupiter’s growth? It’s thought that, during the first million years or so, Jupiter’s planetary core was built rather quickly from small, centimeter-sized pebbles of rocky material. During the next two million years, there was a slower accretion of larger, kilometer-sized rocks called planetesimals. A lot of heat was released during this period as the planetesimals collided with the young, growing planet. As explained by Alibert:

During the first stage the pebbles brought the mass. In the second phase, the planetesimals also added a bit of mass, but what is more important, they brought energy.

Jupiter continued to grow after this, reaching 50 Earth masses after about 3 million years. This led to the beginning of the third phase, where runaway concretion of gas fueled the continued growth of Jupiter, until the planet reached a staggering 300 Earth masses. This is the Jupiter we know and love today.

But why exactly was there the period of slowed growth? First, the researchers found that the period where Jupiter was between 15-50 Earth masses lasted longer than previously thought. The collisions with the larger planetesimals were intense enough that the atmosphere was heated sufficiently to prevent rapid cooling, contraction and further gas accretion. The growth process was therefore delayed. As noted in the new paper:

Pebbles are important in the first stages to build a core quickly, but the heat provided by planetesimals is crucial to delay gas accretion so that it matches the timescale given by the meteorite data.

Scientists now think they know why Jupiter’s growth went through 3 distinct stages. This diagram depicts the 3 stages of Jupiter’s growth, in millions of years. Image via Nature Astronomy/Yann Alibert (Universität Bern) et al.

Below are the three stages of Jupiter’s growth, in brief. Note that they relate to the image above:

Stage 1: until 1 million years: Jupiter grows by accretion of pebbles (blue dots). Large primordial planetesimals (big red dots) show high collision velocities (red arrows) leading to destructive collisions (yellow) and producing small, second generation planetesimals (small red dots).

Stage 2: 1-3 million years: The energy resulting from the accretion of small planetesimals prevents rapid gas accumulation and thus rapid growth (gray arrows).

Stage 3: beyond 3 million years: Jupiter is massive enough to accrete large amounts of gas.

The new formation scenario described by Alibert and team also fits nicely with previous data taken from meteorites. Based on analysis of the meteorites, scientists had concluded that the solar nebula in the primordial early solar system had somehow been divided into two different regions over two million years. When Jupiter had grown to 20-50 Earth masses, it acted as a barrier, disturbing the dust disk (debris disk) surrounding the young sun. This created an overdensity – a greater than normal density – within the dust disk, trapping pebbles outside its orbit.

As a result, material from farther out could not mix with other material closer in to the sun, at least not until Jupiter grew enough to scatter those pebbles inward with its gravity.

Stunning close-up view of cloud systems on Jupiter, from Juno’s Perijove 14 orbit in July, 2018. View more images from Perijove 14. Image via NASA/SwRI/MSSS/Gerald Eichstädt/Seán Doran.

Beyond Jupiter, the researchers also say that their new results can also be used to help solve some long-running puzzles about the formation of Uranus and Neptune, as well as some similar exoplanets. This could be especially relevant to the so-called hot Jupiters, which are gas giant planets the size of Jupiter or larger that orbit much closer to their stars – and other gas giants found in other solar systems.

How did those planets grow even larger than Jupiter and why do many of them orbit so much closer to their stars (i.e. the hot Jupiters)? Maybe this new research will help shed some light.

Bottom line: Scientists have found that Jupiter, the largest planet in our solar system, went through “growing pains” as it was forming, with a period of time where its growth had slowed down considerably. Scientists involved in the new study now think they understand why.

Source: The formation of Jupiter by hybrid pebble–planetesimal accretion

Via University of Bern



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Spectacular view of Jupiter from the Juno spacecraft, acquired April 1, 2018. Image via NASA/JPL-Caltech/SwRI/MSSS. Citizen scientists Gerald Eichstädt and Seán Doran created this image using data from the spacecraft’s JunoCam imager.

Jupiter is sometimes called the king of the planets in our solar system, due to its enormous size. It has some 300 times Earth’s mass. Jupiter is thought to have become the largest planet early in our solar system’s history. Still, questions remained about how quickly (or not) Jupiter kept growing, with earlier evidence suggesting Jupiter’s growth was delayed for about two million years. The reason for this delay was unknown. Now, astrophysicists in Switzerland think they have an answer. Their work was published August 27, 2018, in the peer-reviewed journal Nature Astronomy.

The researchers are affiliated with two organizations, NCCR PlanetS and ETHzürich. Co-author Julia Venturini explained in a statement:

We … show that Jupiter grew in different, distinct phases.

Lead author Yann Alibert added:

Especially interesting is that it is not the same kind of bodies that bring mass and energy [to Jupiter].

In other words, these scientists used computer modeling to show that – billions of years ago, early in our solar system’s history – Jupiter underwent a delayed growth phase as material of varying sizes and types accreted onto it.

Artist’s concept of a very young Jupiter. Scientists think that Jupiter, Earth and the other planets in our solar system formed from a disk of gas and dust surrounding the young sun. Image via Lawrence Livermore National Laboratory.

Planets – like Earth or Jupiter – are thought to grow by accretion from the gas-and-dust clouds, or nebulae, surrounding young stars. That is, they grow as small bits of material in the cloud collide, stick together, and become increasingly bigger. Once the planets themselves get big enough, they begin to sweep up even more material from the solar nebula, via the power of their gravitational pull.

So what happened during these different phases of Jupiter’s growth? It’s thought that, during the first million years or so, Jupiter’s planetary core was built rather quickly from small, centimeter-sized pebbles of rocky material. During the next two million years, there was a slower accretion of larger, kilometer-sized rocks called planetesimals. A lot of heat was released during this period as the planetesimals collided with the young, growing planet. As explained by Alibert:

During the first stage the pebbles brought the mass. In the second phase, the planetesimals also added a bit of mass, but what is more important, they brought energy.

Jupiter continued to grow after this, reaching 50 Earth masses after about 3 million years. This led to the beginning of the third phase, where runaway concretion of gas fueled the continued growth of Jupiter, until the planet reached a staggering 300 Earth masses. This is the Jupiter we know and love today.

But why exactly was there the period of slowed growth? First, the researchers found that the period where Jupiter was between 15-50 Earth masses lasted longer than previously thought. The collisions with the larger planetesimals were intense enough that the atmosphere was heated sufficiently to prevent rapid cooling, contraction and further gas accretion. The growth process was therefore delayed. As noted in the new paper:

Pebbles are important in the first stages to build a core quickly, but the heat provided by planetesimals is crucial to delay gas accretion so that it matches the timescale given by the meteorite data.

Scientists now think they know why Jupiter’s growth went through 3 distinct stages. This diagram depicts the 3 stages of Jupiter’s growth, in millions of years. Image via Nature Astronomy/Yann Alibert (Universität Bern) et al.

Below are the three stages of Jupiter’s growth, in brief. Note that they relate to the image above:

Stage 1: until 1 million years: Jupiter grows by accretion of pebbles (blue dots). Large primordial planetesimals (big red dots) show high collision velocities (red arrows) leading to destructive collisions (yellow) and producing small, second generation planetesimals (small red dots).

Stage 2: 1-3 million years: The energy resulting from the accretion of small planetesimals prevents rapid gas accumulation and thus rapid growth (gray arrows).

Stage 3: beyond 3 million years: Jupiter is massive enough to accrete large amounts of gas.

The new formation scenario described by Alibert and team also fits nicely with previous data taken from meteorites. Based on analysis of the meteorites, scientists had concluded that the solar nebula in the primordial early solar system had somehow been divided into two different regions over two million years. When Jupiter had grown to 20-50 Earth masses, it acted as a barrier, disturbing the dust disk (debris disk) surrounding the young sun. This created an overdensity – a greater than normal density – within the dust disk, trapping pebbles outside its orbit.

As a result, material from farther out could not mix with other material closer in to the sun, at least not until Jupiter grew enough to scatter those pebbles inward with its gravity.

Stunning close-up view of cloud systems on Jupiter, from Juno’s Perijove 14 orbit in July, 2018. View more images from Perijove 14. Image via NASA/SwRI/MSSS/Gerald Eichstädt/Seán Doran.

Beyond Jupiter, the researchers also say that their new results can also be used to help solve some long-running puzzles about the formation of Uranus and Neptune, as well as some similar exoplanets. This could be especially relevant to the so-called hot Jupiters, which are gas giant planets the size of Jupiter or larger that orbit much closer to their stars – and other gas giants found in other solar systems.

How did those planets grow even larger than Jupiter and why do many of them orbit so much closer to their stars (i.e. the hot Jupiters)? Maybe this new research will help shed some light.

Bottom line: Scientists have found that Jupiter, the largest planet in our solar system, went through “growing pains” as it was forming, with a period of time where its growth had slowed down considerably. Scientists involved in the new study now think they understand why.

Source: The formation of Jupiter by hybrid pebble–planetesimal accretion

Via University of Bern



from EarthSky https://ift.tt/2wK4S3J

Use Big Dipper to find North Star

Tonight’s chart shows Polaris and the Big and Little Dippers for a September evening. You can use the Big Dipper to find Polaris, which is also known as the North Star. Notice that a line from the two outermost stars in the bowl of the Big Dipper points to Polaris. And notice that Polaris marks the tip of the handle of the Little Dipper.

The northern sky is a large clock, with Polaris at its center. The hour hand is a line drawn through Dubhe and Merak, the two pointer stars of the Big Dipper. Because the stars make a full circle in 23 hours 56 minutes instead of exactly 24 hours, this star clock is not exactly the same as the one on the wall, but with a little practice you can learn to read it well.

The Big and Little Dippers: All you need to know

EarthSky astronomy kits are perfect for beginners. Order today from the EarthSky store

View larger. Keith Breazeal's photo of a meteor streaking past the Big Dipper. Perseid Meteor Shower 12-13 Aug 2015. One of the many captured last night at the Bear River Dam in the California Sierra Nevada mountains. This one was at 10:32 Canon 5D Mark III Rokinon 14mm f2.8 25 seconds ISO 5000. Thank you Keith!

View larger. | Keith Breazeal’s photo of a meteor streaking past the Big Dipper during the 2015 Perseid meteor shower. Captured at the Bear River Dam in the California Sierra Nevada mountains. Can you find Polaris in this photo?

The Big Dipper swings full circle – 360 degrees – around Polaris in about 23 hours and 56 minutes. In 24 hours, the Big Dipper actually swings more than full circle, or 361 degrees. Does that make a difference? Yes! It means that – if you look at the same time each evening – the Big Dipper will appear just a little bit lower in the northwestern evening sky.

If you’re in the northern U.S., Canada or at a similar latitude, the Big Dipper is circumpolar for you – always above the horizon. Image via burro.astr.cwru.edu

A month from now at mid-evening, the Big Dipper will be noticeably lower in the northwest. It’ll actually beneath the horizon as seen from the southern latitudes in the United States – although it’s circumpolar, or always above the northern horizon, as seen from the northern U.S., Canada and similarly northern latitudes.

The constant motion from night to night of these stars circling Polaris is a bit like a bear circling its prey, looking for a way to attack. Several ancient cultures from the Greeks and Romans to the Micmac Indians likened these stars to a bear.

In Greek mythology, the Big Dipper asterism represents the hindquarters and tail of the constellation Ursa Major, the Great Bear. The Micmacs saw the three stars of the Big Dipper handle as hunters chasing the bear.

Watch the Big and Little Dippers circle around Polaris tonight! To locate Polaris, the North Star, just draw a line between the two outer stars in the bowl of the Big Dipper.

Enjoying EarthSky so far? Sign up for our free daily newsletter today!



from EarthSky https://ift.tt/1L3HkUk

Tonight’s chart shows Polaris and the Big and Little Dippers for a September evening. You can use the Big Dipper to find Polaris, which is also known as the North Star. Notice that a line from the two outermost stars in the bowl of the Big Dipper points to Polaris. And notice that Polaris marks the tip of the handle of the Little Dipper.

The northern sky is a large clock, with Polaris at its center. The hour hand is a line drawn through Dubhe and Merak, the two pointer stars of the Big Dipper. Because the stars make a full circle in 23 hours 56 minutes instead of exactly 24 hours, this star clock is not exactly the same as the one on the wall, but with a little practice you can learn to read it well.

The Big and Little Dippers: All you need to know

EarthSky astronomy kits are perfect for beginners. Order today from the EarthSky store

View larger. Keith Breazeal's photo of a meteor streaking past the Big Dipper. Perseid Meteor Shower 12-13 Aug 2015. One of the many captured last night at the Bear River Dam in the California Sierra Nevada mountains. This one was at 10:32 Canon 5D Mark III Rokinon 14mm f2.8 25 seconds ISO 5000. Thank you Keith!

View larger. | Keith Breazeal’s photo of a meteor streaking past the Big Dipper during the 2015 Perseid meteor shower. Captured at the Bear River Dam in the California Sierra Nevada mountains. Can you find Polaris in this photo?

The Big Dipper swings full circle – 360 degrees – around Polaris in about 23 hours and 56 minutes. In 24 hours, the Big Dipper actually swings more than full circle, or 361 degrees. Does that make a difference? Yes! It means that – if you look at the same time each evening – the Big Dipper will appear just a little bit lower in the northwestern evening sky.

If you’re in the northern U.S., Canada or at a similar latitude, the Big Dipper is circumpolar for you – always above the horizon. Image via burro.astr.cwru.edu

A month from now at mid-evening, the Big Dipper will be noticeably lower in the northwest. It’ll actually beneath the horizon as seen from the southern latitudes in the United States – although it’s circumpolar, or always above the northern horizon, as seen from the northern U.S., Canada and similarly northern latitudes.

The constant motion from night to night of these stars circling Polaris is a bit like a bear circling its prey, looking for a way to attack. Several ancient cultures from the Greeks and Romans to the Micmac Indians likened these stars to a bear.

In Greek mythology, the Big Dipper asterism represents the hindquarters and tail of the constellation Ursa Major, the Great Bear. The Micmacs saw the three stars of the Big Dipper handle as hunters chasing the bear.

Watch the Big and Little Dippers circle around Polaris tonight! To locate Polaris, the North Star, just draw a line between the two outer stars in the bowl of the Big Dipper.

Enjoying EarthSky so far? Sign up for our free daily newsletter today!



from EarthSky https://ift.tt/1L3HkUk

2018 SkS Weekly Climate Change & Global Warming Digest #35

Calls to Action... Story of the Week... Editorial of the Week... El Niño/La Niña Update... Toon of the Week... Coming Soon on SkS... Climate Feedback Reviews... SkS Week in Review... Poster of the Week...

Calls to Action*...

Looking ahead...

Sat Sep 8 is an extremely important day for climate activists because they will be gathering in cities throughout the world to Rise Up for Climate. If you re not already plugged into an event in your area, you can easily do so by going to the official Rise Up for Climate website. From the global campaign's website:

On September 8, we’re planning thousands of rallies in cities and towns around the world to demand our local leaders commit to building a fossil free world that puts people and justice before profits.

No more stalling, no more delays: it’s time for a fast and fair transition to 100% renewable energy for all.

Real climate leadership rises from below. It means power in the hands of people not corporations. It means economic opportunity for workers and justice and dignity for frontline communities that are the hardest hit by the impacts of the fossil fuel industry and a warming world. 

Looking inside... 

Be sure to check out the next two sections of this digest — Story of the Week and Opinion of the Week. They address two inter-related issue re the hum race's ability to come to grips with the reality of man-made climate change and the need to effectively mitigate it srtarting now.

Looking behind...

Something that flew under my radar screen when it was released earlier this year...

Narrated by Danny Glover, A documentary special reveals how climate change science has been under systematic attack; the multi-million dollar campaign allowed a climate change denier to be elected president (a new version with updated content and music)

TRNN Documentary: Trump, The Koch Brothers and Their War on Climate Science, May 23, 2018

TRNN = The Real News Network, Baltimore, MD


*The views expressed in this section are those of John Hartz and do not necessarily reflect  consensus views of the SkS author team — it's nearly impossible to achieve consensus within a herd of cats.  


Story of the Week...

The Swedish 15-year-old who's cutting class to fight the climate crisis

Following Sweden’s hottest summer ever, Greta Thunberg decided to go on school strike at the parliament to get politicians to act

Greta Thurnberg Stockholm Sweden Aug 2018 

Greta Thunberg leads a school strike and sits outside of the Swedish Parliament, in an effort to force politicians to act on climate change. Photograph: Michael Campanella for the Guardian 

Why bother to learn anything in school if politicians won’t pay attention to the facts?

This simple realisation prompted Greta Thunberg, 15, to protest in the most effective way she knew. She is on strike, refusing to go to school until Sweden’s general election on 9 September to draw attention to the climate crisis.

Her protest has captured the imagination of a country that has been struck by heatwaves and wildfires in its hottest summer since records began 262 years ago.

Every day for two weeks, Thunberg has been sitting quietly on the cobblestones outside parliament in central Stockholm, handing out leaflets that declare: “I am doing this because you adults are shitting on my future.”

Thunberg herself is a diminutive girl with pigtails and a fleeting smile – not the stereotypical leader of a climate revolution.

“I am doing this because nobody else is doing anything. It is my moral responsibility to do what I can,” she says. “I want the politicians to prioritise the climate question, focus on the climate and treat it like a crisis.”

When people tell her she should be at school, she points to the textbooks in her satchel.

“I have my books here,” she says in flawless English. “But also I am thinking: what am I missing? What am I going to learn in school? Facts don’t matter any more, politicians aren’t listening to the scientists, so why should I learn?”

The Swedish 15-year-old who's cutting class to fight the climate crisis by David Crouch, Science, Guardian, Sep 1, 2018 


Opinion of the Week...

Would you put your child or grandchild on a plane that has a one chance in 20 of a disastrous crash?

It’s hard imagining anyone doing that, but it is essentially what we are doing to our kids and grandkids by not raising our voices about climate change and the 1-in-20 chance that disaster lies ahead for them. It is bad enough that we are likely on the path to exceed the 3.6 degree Fahrenheit goal stated in the Paris Agreement, which will result in dire consequences such as increasing droughts and wildfires and inundation of low lying coastal areas because of sea level rise.

If we continue on that path without taking the necessary actions to reduce greenhouse gas emissions, there is a 5 percent chance of catastrophic consequences — even an existential threat to humanity by mid-century, according to experts at the Scripps Institute. 

Uncontrolled climate change could result in disaster for our kids. Will we do something?, Opinion by Mike Hoffman, USA Today, Aug 1, 2018 


El Niño/La Niña Update...

With all signs highlighting a switch, from the La Nina to the forecast El Nino (formally called El Nino Southern Oscillation or ENSO) climate pattern for this fall 2018, and winter too, meteorologists and climatologists expect to have a better idea of how strong this El Nino event will become by late October into November.

"Looking at the latest 30-day and 90-day maps generated (for this Autumn 2018 which the Climate Prediction Center issued Aug. 16, 2018) it appears we're witnessing the incorporation of an El Nino event into the outlooks," said Allen Dutcher, associate state climatologist, Nebraska State Climate Office-Lincoln. "During the past four weeks, there's been a subtle shift toward a wetter pattern across the southern Plains, while the northern Plains has slipped towards the dry side."

Most weather signs are pointing to an El Nino weather pattern this fall and winter by Amy G. Hadachek, The Fence Post, Aug 31, 2018 


Toon of the Week...

2018 Toon 35 


Coming Soon on SkS...

 [To be added.] 


Climate Feedback Reviews...

[To be added.] 


SkS Week in Review... 

 [To be added.] 


Poster of the Week...

2018 Poster of the Week 

 

 



from Skeptical Science https://ift.tt/2NLVbIw

Calls to Action... Story of the Week... Editorial of the Week... El Niño/La Niña Update... Toon of the Week... Coming Soon on SkS... Climate Feedback Reviews... SkS Week in Review... Poster of the Week...

Calls to Action*...

Looking ahead...

Sat Sep 8 is an extremely important day for climate activists because they will be gathering in cities throughout the world to Rise Up for Climate. If you re not already plugged into an event in your area, you can easily do so by going to the official Rise Up for Climate website. From the global campaign's website:

On September 8, we’re planning thousands of rallies in cities and towns around the world to demand our local leaders commit to building a fossil free world that puts people and justice before profits.

No more stalling, no more delays: it’s time for a fast and fair transition to 100% renewable energy for all.

Real climate leadership rises from below. It means power in the hands of people not corporations. It means economic opportunity for workers and justice and dignity for frontline communities that are the hardest hit by the impacts of the fossil fuel industry and a warming world. 

Looking inside... 

Be sure to check out the next two sections of this digest — Story of the Week and Opinion of the Week. They address two inter-related issue re the hum race's ability to come to grips with the reality of man-made climate change and the need to effectively mitigate it srtarting now.

Looking behind...

Something that flew under my radar screen when it was released earlier this year...

Narrated by Danny Glover, A documentary special reveals how climate change science has been under systematic attack; the multi-million dollar campaign allowed a climate change denier to be elected president (a new version with updated content and music)

TRNN Documentary: Trump, The Koch Brothers and Their War on Climate Science, May 23, 2018

TRNN = The Real News Network, Baltimore, MD


*The views expressed in this section are those of John Hartz and do not necessarily reflect  consensus views of the SkS author team — it's nearly impossible to achieve consensus within a herd of cats.  


Story of the Week...

The Swedish 15-year-old who's cutting class to fight the climate crisis

Following Sweden’s hottest summer ever, Greta Thunberg decided to go on school strike at the parliament to get politicians to act

Greta Thurnberg Stockholm Sweden Aug 2018 

Greta Thunberg leads a school strike and sits outside of the Swedish Parliament, in an effort to force politicians to act on climate change. Photograph: Michael Campanella for the Guardian 

Why bother to learn anything in school if politicians won’t pay attention to the facts?

This simple realisation prompted Greta Thunberg, 15, to protest in the most effective way she knew. She is on strike, refusing to go to school until Sweden’s general election on 9 September to draw attention to the climate crisis.

Her protest has captured the imagination of a country that has been struck by heatwaves and wildfires in its hottest summer since records began 262 years ago.

Every day for two weeks, Thunberg has been sitting quietly on the cobblestones outside parliament in central Stockholm, handing out leaflets that declare: “I am doing this because you adults are shitting on my future.”

Thunberg herself is a diminutive girl with pigtails and a fleeting smile – not the stereotypical leader of a climate revolution.

“I am doing this because nobody else is doing anything. It is my moral responsibility to do what I can,” she says. “I want the politicians to prioritise the climate question, focus on the climate and treat it like a crisis.”

When people tell her she should be at school, she points to the textbooks in her satchel.

“I have my books here,” she says in flawless English. “But also I am thinking: what am I missing? What am I going to learn in school? Facts don’t matter any more, politicians aren’t listening to the scientists, so why should I learn?”

The Swedish 15-year-old who's cutting class to fight the climate crisis by David Crouch, Science, Guardian, Sep 1, 2018 


Opinion of the Week...

Would you put your child or grandchild on a plane that has a one chance in 20 of a disastrous crash?

It’s hard imagining anyone doing that, but it is essentially what we are doing to our kids and grandkids by not raising our voices about climate change and the 1-in-20 chance that disaster lies ahead for them. It is bad enough that we are likely on the path to exceed the 3.6 degree Fahrenheit goal stated in the Paris Agreement, which will result in dire consequences such as increasing droughts and wildfires and inundation of low lying coastal areas because of sea level rise.

If we continue on that path without taking the necessary actions to reduce greenhouse gas emissions, there is a 5 percent chance of catastrophic consequences — even an existential threat to humanity by mid-century, according to experts at the Scripps Institute. 

Uncontrolled climate change could result in disaster for our kids. Will we do something?, Opinion by Mike Hoffman, USA Today, Aug 1, 2018 


El Niño/La Niña Update...

With all signs highlighting a switch, from the La Nina to the forecast El Nino (formally called El Nino Southern Oscillation or ENSO) climate pattern for this fall 2018, and winter too, meteorologists and climatologists expect to have a better idea of how strong this El Nino event will become by late October into November.

"Looking at the latest 30-day and 90-day maps generated (for this Autumn 2018 which the Climate Prediction Center issued Aug. 16, 2018) it appears we're witnessing the incorporation of an El Nino event into the outlooks," said Allen Dutcher, associate state climatologist, Nebraska State Climate Office-Lincoln. "During the past four weeks, there's been a subtle shift toward a wetter pattern across the southern Plains, while the northern Plains has slipped towards the dry side."

Most weather signs are pointing to an El Nino weather pattern this fall and winter by Amy G. Hadachek, The Fence Post, Aug 31, 2018 


Toon of the Week...

2018 Toon 35 


Coming Soon on SkS...

 [To be added.] 


Climate Feedback Reviews...

[To be added.] 


SkS Week in Review... 

 [To be added.] 


Poster of the Week...

2018 Poster of the Week 

 

 



from Skeptical Science https://ift.tt/2NLVbIw