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‘Strongest meteor storm in generations could light up skies above North America early next week

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The ‘strongest meteor storm in generations’ could light up skies above North America next week.

Fragments of dying comet SW3 are predicted to be visible from america and parts of Canada when the Earth crosses through its orbital path on Tuesday.

The SW3 comet, full name 73P/Schwassmann-Wachmann 3, is answerable for the fragments of dust that causes meteor shower Tau Herculids. 

SW3 split into large fragments in 1995, and has continued to fragment further since. 

Next week the Earth could have a direct interaction with the debris from the comet for the very first time.

Nevertheless, NASA is uncertain whether the debris will make it to us this 12 months and has cautioned the Tau Herculids might be ‘all or nothing’.  

Images of 48 comet fragments from SW3 recorded in May 2006 by the Infrared Array Camera (IRAC) on board the Spitzer Space Telescope. Emission from the dust particles warmed by sunlight appears to fill the space along the cometary orbit

A meteor shower occurs when the Earth passes through the trail of debris left by a comet or asteroid

A meteor shower occurs when the Earth passes through the trail of debris left by a comet or asteroid 

Explained: The difference between an asteroid, meteorite and other space rocks 

  An asteroid is a big chunk of rock left over from collisions or the early solar system. Most are positioned between Mars and Jupiter within the Principal Belt.

A comet is a rock covered in ice, methane and other compounds. Their orbits take them much further out of the solar system.

A meteor is what astronomers call a flash of sunshine within the atmosphere when debris burns up.

This debris itself is often known as a meteoroid. Most are so small they’re vapourised within the atmosphere.

If any of this meteoroid makes it to Earth, it is known as a meteorite.

Meteors, meteoroids and meteorites normally originate from asteroids and comets.

For instance, if Earth passes through the tail of a comet, much of the debris burns up within the atmosphere, forming a meteor shower.

A meteor shower occurs when the Earth passes through the trail of debris left by a comet or asteroid.

Most meteor showers are predictable, recurring annually when the Earth traverses a specific trail of debris.

Nevertheless, occasionally the Earth passes through a very narrow and dense clump of space dust which turns into hundreds of fast-moving shooting stars.

That is often known as a meteor storm, and provides a blinding spectacle for stargazers.

The starry pattern related to the Tau Herculids is the Hercules constellation, the fifth largest constellation within the sky, and the shower appears to radiate from a degree about ten degrees from the star Arcturus.

SW3 was first spotted in 1930 by German observers Arnold Schwassmann and Arno Arthur Wachmann, who determined it to have a 5.4 12 months orbit.

Over time it became very faint, but in 1995 it unexpectedly became nearly 400 times brighter and was even visible from the naked eye.

The comet’s icy core had split into 4, releasing huge amounts of gas and debris, which continued because it orbited the Sun.

By 2006, the shattered comet was in 68 pieces, and is more likely to have broken down much more since. 

Computer modelling suggests that fragments of SW3 have been spreading out of its orbit like tentacles. 

Nevertheless, these fragments usually are not visible until the Earth ploughs into them.

This 12 months, our planet is as a consequence of cross its path on May 31, although the comet itself is not speculated to pass by until a couple of months later.

The brightness of the meteor storm will depend upon how much debris SW3 has thrown in front of it, if any. 

This might be the primary time the Earth and the numerous comet debris shed in 1995 have come together for the reason that fragmentation event.

If we go through a heavy concentration of the debris, then there’s a possibility of a dramatic meteor storm.

Bill Cooke, who leads NASA’s Meteoroid Environment Office on the Marshall Space Flight Center, describes it as ‘an all or nothing event’.

He said: ‘If the debris from SW3 was travelling greater than 220 mph (354 km/h) when it separated from the comet, we’d see a pleasant meteor shower. 

‘If the debris had slower ejection speeds, then nothing will make it to Earth and there might be no meteors from this comet,

‘It’s an ideal opportunity for space enthusiasts to get out and experience considered one of nature’s most vivid light shows.’

Some models suggest that there might be a powerful display from the meteor shower while others predict the cosmic fragments will just fall in need of the Earth’s path.

Positions of Earth, SW3 ('1995') and presumed train of meteoroids on May 31 2022 using orbital simulator, assuming meteoroids are trailing behind the parent comet. In this situation no interaction with Earth can take place. Positions of Earth, SW3 ('1995') and presumed train of meteoroids on May 31 2022 using orbital simulator, assuming meteoroids are moving ahead of the parent comet. Interaction with the Earth takes place between comet samples #12 and #13

Positions of Earth, SW3 (‘1995’) and presumed train of meteoroids on May 31 2022 using orbital simulator. Left – Assuming meteoroids are trailing behind the parent comet. In this case no interaction with Earth can happen. Right – Assuming meteoroids are moving ahead of the parent comet. Interaction with the Earth takes place between comet samples #12 and #13

Map of the geographic visibility of the potential meteor outburst. Radiant elevations are presented as concentric circles at 10◦ intervals. The radiant of a meteor shower is the celestial point in the sky from which the paths of meteors appear to originate to a terrestrial viewer

Map of the geographic visibility of the potential meteor outburst. Radiant elevations are presented as concentric circles at 10◦ intervals. The radiant of a meteor shower is the celestial point within the sky from which the paths of meteors appear to originate to a terrestrial viewer

The Earth should cross the debris stream that SW3 left in 1995 between 00:45 and 01:17 am ET early Tuesday morning, and is predicted to last as long as two hours if visible.

The phenomenon ought to be visible from North and South America because it is as a consequence of be a recent moon, so the very dark sky will allow for max brightness. 

The most effective view might be from the southwest of the USA and Mexico, while it is also seen from the southeastern provinces of Canada.

Nevertheless it won’t be seen from Alaska, Washington and the north and western provinces of Canada as it is going to be twilight on the time of the shower.

In Australia the storm will even be over before it’s dark enough to be seen, and it’s unlikely to be visible within the UK.

The Earth will even cross SW3’s orbit that it made in 1892 on Monday May 30 at about 2 pm ET, after which through its 1897 passage at about Tuesday May 31 at 6 am ET.

Unfortunately the debris left from these orbits can have unfolded over time, so only a couple of meteors might be expected.

REMAINING METEOR SHOWERS IN 2022 

Delta Aquarids: July 30 – 25 per hour – Regular stream over days

Alpha Capricornids: July 30 – 5 per hour – Yellow slow fireballs

Perseids: August 12-13 – 100 per hour – Shiny, fast meteors with trains

Draconids: October 8-9 – 10 per hour – From comet Giacobini-Zimmer

Orionids: October 21-22 – 25 per hour – Fast with nice trains

Taurids: October 10-11 (Southern), November 12-13 (Northern) – 5 per hour – Very slow

Leonids: November 17-18 – 10 per hour – Fast and vibrant

Geminids: December 14-15 – 150 per hour – Shiny and plentiful, few trains

Ursids: December 22-23 – 10 per hour – Sparse shower 

Note: Dates seek advice from each shower’s peak 

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