The Longest Eclipse of The 21st Century Happens Next Week, And Earth Will Colour The Moon Blood Red

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According to ScienceAlert (This article and its images were originally posted on ScienceAlert July 17, 2018 at 09:20PM.)

Huge swaths of Earth are in for a special astronomical treat in late July: the longest total lunar eclipse in roughly 100 years.

During the early morning of July 28, Earth will pass between the sun and the moon to cast a shadow on our 4.5-billion-year-old satellite.

Earth’s shadow isn’t a dull grey, though.

It ranges from orange to an eerie blood-red hue if you’re right in the middle, which is precisely where the moon will be this time around.

Here’s that works.

How a total lunar eclipse colours the moon red

A total lunar eclipse and a total solar eclipse are similar, if not the reverse of one another, but their appearances are significantly different.

During a solar eclipse, the moon passes between Earth and the sun to cast its shadow on our planet. The shadow is colorless because the moon has no atmosphere to scatter or refract any sunlight.

Earth, of course, is a different story.

Our planet’s nitrogen-rich atmosphere takes white sunlight, a mix of all colours of the spectrum, and scatters around the blue colours. This makes the sky appear blue during the day and the sun yellow.

Around sunset and sunrise, the light reaching our eyes has been more throughly scattered, so much that blues are nearly absent. This makes the sun and its light appear more orange or even red.

Roughly 386,200 kilometres (240,000 miles) away at the moon, the Earth would look quite stunning as the same air, like a big lens, refracts that tinged light toward the full moon.

“If you were standing on the moon’s surface during a lunar eclipse, you would see the sun setting and rising behind the Earth,” David Diner, a planetary scientist at NASA’s Jet Propulsion Laboratory, wrote in a blog post.

“You’d observe the refracted and scattered solar rays as they pass through the atmosphere surrounding our planet.”

what lunar eclipse blood moon looks like The Earth, Moon, and Sun during a total lunar eclipse. (Shayanne Gal/Business Insider)

This is why lunar eclipses are orange-red: All of that coloured light is focused on the moon in a cone-shaped shadow called the umbra.

The moon is also covered in ultra-fine, glass-like rock dust called regolith, which has a special property called “backscatter“.

This bounces a lot of light back the same way it came from, in this case toward Earth (Backscattering also explains why full moons are far brighter than during other lunar phase.)

So, when we’re looking at the moon during a total lunar eclipse, we’re seeing Earth’s refracted sunset-sunrise light being bounced right back at us.

The red colour is never quite the same from one lunar eclipse to the next due to natural and human activities that affect Earth’s atmosphere.

“Pollution and dust in the lower atmosphere tends to subdue the colour of the rising or setting sun, whereas fine smoke particles or tiny aerosols lofted to high altitudes during a major volcanic eruption can deepen the colour to an intense shade of red,” Diner said.

Where and when to see the total lunar eclipse

If the weather cooperates, most of eastern Africa, the Middle East, and central Asia should see the full and total lunar eclipse. Scientists in Antarctica should also have a great view.

Europe, eastern Asia, Australia, Indonesia, and other regions will also enjoy a partial lunar eclipse, where the moon passes partly through Earth’s shadow.

Western Australia will be the only Australian state to catch the entire eclipse.

Here’s when to catch it in Australia (times in AEST):

  • 3:14am: The penumbral eclipse begins when the Earth’s penumbra starts to touch the moon.
  • 5:30am: The total eclipse can be seen when the moon is fully red.
  • 6:21am: Maximum eclipse.
  • 7:13am: Total eclipse ends and moon will set in the west-southwest.

where you can see blood eclipse july 2018Where the total lunar eclipse will be visible. (Fred Espenak/NASA Goddard Space Flight Center)

You can still watch on a live webcast, though, if you’re located elsewhere.

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This article and its images were originally posted on [ScienceAlert] July 17, 2018 at 09:20PM. All credit to both the author DAVE MOSHER & SHAYANNE GAL and ScienceAlert | ESIST.T>G>S Recommended Articles Of The Day.

 

 

 

Look Up Friday! Green Comet and Snow Moon Eclipse Team Up for Skywatchers

Look Up Friday! Green Comet and Snow Moon Eclipse Team Up for Skywatchers

Skywatchers this weekend will get two special, subtle treats: a penumbral lunar eclipse on Friday (Feb. 10) and a strange green comet reaching its peak viewing time the following morning.

First, February’s full moon — the “snow moon” — will pass through the edge of the Earth’s shadow, which is called the penumbra. During this “full snow moon eclipse,” the moon will be completely shaded, making the change easier to see, although it won’t stand out as much as a typical lunar eclipse when the moon passes deep into the heart of Earth’s shadow, called the umbra, and turns a ruddy color.

Meanwhile, Comet 45P/Honda-Mrkos-Pajdusakova will be visible in the predawn hours by skywatchers using binoculars or small telescopes between Thursday and Sunday, in the constellation Hercules in the eastern sky. The comet’s closest approach will come on Saturday, when the object will pass just 7.4 million miles (12 million kilometers) from Earth.

While that’s 20 times the distance to the moon, the comet’s approach is close by celestial standards. Comet 45P will appear blueish-green due to vaporizing diatomic carbon, which appears green in space’s near-vacuum conditions.

Astronomy broadcasting service Slooh will have two shows related to the eclipse and the comet. “The Full Snow Moon Eclipse” will broadcast on Feb. 10 at 5:30 p.m. EST (2030 GMT), and “Cruise the Galaxy with Comet 45P” will broadcast the same night at 10:30 p.m. EST (0330 GMT Feb. 11).

You can also watch both of the broadcasts here on Space.com, courtesy of Slooh.

The penumbral lunar eclipse is visible nearly worldwide, except for in Hawaii, Australia, New Zealand and countries along the coast of the Pacific in east Asia. The moon will enter Earth’s shadow at 5:32 p.m. EST (2232 GMT) and leave at 9:55 p.m. EST (0255 GMT on Feb. 11); the peak eclipse takes place at 7:43 p.m. EST (0034 GMT on Feb. 11).

The moon will be harder to see in most of North America, because the full moon will still be rising at that time, while East Asian viewers will have a setting moon during the eclipse. It will be best visible in areas with little light pollution and a horizon unobstructed by buildings, mountains or trees.

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This article was posted on livescience.com

By Elizabeth Howell, Live Science Contributor

 

 

 

 

 

 

HOW TO WATCH TOMORROW MORNING’S SOLAR ECLIPSE

See a ‘Ring of Fire’ Annular Solar Eclipse Thursday Via Slooh Webcast :  You can watch the webcast at Slooh.com, beginning at 2:45 a.m. EDT Thursday (0645 GMT).

ccssc-annular-solar-eclipse-ring

A spectacular “ring of fire” solar eclipse will darken skies over Africa early Thursday morning (Sept. 1), and people anywhere in the world can watch the event live during a free webcast by the Slooh Community Observatory.

The show will feature live telescope shots from Slooh’s flagship observatory in the Canary Islands off the west coast of Africa, as well as views from South Africa, Tanzania, Madagascar and tiny Réunion Island. You can watch the webcast at Slooh.com, beginning at 2:45 a.m. EDT Thursday (0645 GMT).

You can also watch the solar eclipse webcast on Space.com, courtesy of Slooh. Thursday’s eclipse will begin a little after 2 a.m. EDT (0600 GMT), reach its maximum extent three hours later and wrap up at about 8 a.m. EDT (1200 GMT). [Solar Eclipse 2016 Guide: Where, When & How to See It]

Map showing the path of the Sept. 1, 2016 annular solar eclipse across parts of Africa.

Credit: NASA/Fred Espenak

In “ring of fire” (also known as “annular”) solar eclipses, the moon doesn’t quite blot out the sun, leaving a thin ring blazing around the edge of the solar disk. Such events occur when the moon is relatively far from Earth in its elliptical orbit. (Total solar eclipses occur when the moon is closer to Earth, and therefore big enough in our sky to block the sun completely.)

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By Samantha Cole

 

 

Source: See a ‘Ring of Fire’ Annular Solar Eclipse Thursday Via Slooh Webcast

Space scientists observe Io’s atmospheric collapse during eclipse| ESIST

An artist’s rendering depicts Io’s volcanic plumes creating the atmosphere in sunlight.
Credit: Image courtesy of Southwest Research Institute
 A Southwest Research Institute-led team has documented atmospheric changes on Io, Jupiter’s volcanically active satellite, as the giant planet casts its shadow over the moon’s surface during daily eclipses.

A study led by SwRI’s Constantine Tsang concluded that Io’s thin atmosphere, which consists primarily of sulfur dioxide (SO2) gas emitted from volcanoes, collapses as the SO2 freezes onto the surface as ice when Io is shaded by Jupiter. When the moon moves out of eclipse and ice warms, the atmosphere reforms through sublimation, where ice converts directly to gas.

“This research is the first time scientists have observed this phenomenon directly, improving our understanding of this geologically active moon,” said Tsang, a senior research scientist in SwRI’s Space Science and Engineering Division.

The findings were published in a study titled “The Collapse of Io’s Primary Atmosphere in Jupiter Eclipse” in the Journal of Geophysical Research. The team used the eight-meter Gemini North telescope in Hawaii and the Texas Echelon Cross Echelle Spectrograph (TEXES) for this research.

Data showed that Io’s atmosphere begins to “deflate” when the temperatures drop from -235 degrees Fahrenheit in sunlight to -270 degrees Fahrenheit during eclipse. Eclipse occurs 2 hours of every Io day (1.7 Earth days). In full eclipse, the atmosphere effectively collapses as most of the SO2 gas settles as frost on the moon’s surface. The atmosphere redevelops as the surface warms once the moon returns to full sunlight.

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Source: Southwest Research Institute

 

Source: ScienceDaily