Tomorrow morning will be three-and-a-half hours. Some parts of the planet will experience the most dramatic colour changes. The moon’s light is reddened as it moves through Earth’s shadow.

This will be the longest partial lunar eclipse of the century, according to NASA, with the peak at 09:02 GMT (04:02 ET), when 97 per cent of the moon will be covered in shadow. 

You can see it best from North America. Hawaii will receive 97% coverage and the rest of North America is able to witness the whole event. 

This is due to the Earth’s atmosphere filtering light from the sun, which causes it to take on a reddish or rusty colour. 

Skywatchers in the UK won’t get much of a show, with a small slither of the moon turning red from the start of the eclipse at 06:02 GMT until moonset at 07:24 GMT.  

According to Greenwich’s Royal Observatory Greenwich, a partial eclipse is ‘barely noticeable in the UK’ if it happens when the moon passes close to the horizon. 

Because it occurs at the furthest point of Earth, this full moon is also known as “beaver-blood micro moon”. 

The longest partial lunar eclipse of the century will take place on Friday morning, according to NASA, making the moon appear red for up to 3.5 hours. This is a lunar eclipse seen in China in May 2021

NASA has announced that Friday will be the longest partial lunar eclipse in history. The moon appears red for as long as 3.5 hours. In May 2021, this lunar eclipse was seen in China.

What is a LUNAR ECLIPSE? 

An eclipse occurs any time a planet or moon passes between another planet, moon or the sun.

They may be partial or total depending on how they orbit the earth.

Moonrise is an event that occurs when Earth aligns directly with the sun and moon.

Earth’s shadow blocks light from the sun onto the moon when this occurs. The shadow of Earth falls onto the moon.

During a lunar eclipse, we can see Earth’s shadow on the moon.

Although they can last up to an hour, it’s rare that a total eclipse lasts more than 100 minutes.  

Each year there are at least two moon eclipses.

Because it is dependent on moonset and sunrise, your location will affect how visible the eclipse.

The early stages will not be missed by those living in Australia, New Zealand and western Asia. However, the latter stages will be missed by people from South America and Western Europe. 

Meanwhile, it won’t be visible at all in Africa or the Middle East. 

The eclipse’s first phases will start at 06:02 GMT on November 19 (01:02 ET).

The moon will then gradually become more obscured from 07:18 GMT (02:18 ET), ending at 10:47 GMT (05:47 ET), although the peak point is at 09:02 GMT (04:02 ET).

The UK moon sets on Friday at 07:24 GMT (2:24 ET). This is well ahead of the peak eclipse.

The reddish moon will start to appear in the southern part of England at 07:18 ET (02:18 ET). However, it will only be visible just above the horizon.  

Dhara Patel (Royal Observatory Greenwich) told MailOnline that the partial lunar eclipse of Friday morning would be difficult to view for UK residents. 

It will not be easy to see the Moon setting if viewers don’t have clear vision of the northern horizon.

‘The Moon will however begin to pass into the outer part of the Earth’s shadow just after 6:00am – early risers will be able to see the full Moon over the north western horizon, but the penumbra (outer part of the Earth’s shadow) is weaker and it’s unlikely to create a visible change.’ 

When the Earth crosses the line between the sun and moon, it is called a lunar eclipse. Our natural satellite’s shadow will be eclipsed by the Earth’s orbit.

Skywatchers in the UK won't get much of a show, with a small slither of the moon turning red from the start of the eclipse at 06:02 GMT until moonset at 07:24 GMT

The UK Skywatchers won’t see much, as there will be a small red sludge of the moon changing color from 06:02 GMT to 07:24 GMT.

It will darken the moon for most of the planet on November 19, with up to 97 per cent of the moon slipping into Earth's shadow. This is a near full moon in New York last night

On November 19, it will make the moon darker for the majority of Earth, with 97% of the moon falling into Earth’s shadow. New York’s last night saw a nearly full moon.

DURATIONS OF PARTIAL LUNAR LUNAR ECLIPSE 

The  umbral eclipse, the part covered by Earth’s full shadow, will last for 3 hours and 28 minutes on November 19, 2021 — the longest of the century.

It is 6 hours 1 minute long, and the penumbral shadow (when the moon passes through both the inner and outer portions of Earth shadow) will be the longest lasting in six centuries. 

In July 2019, the partial lunar eclipse lasted less than three hours. The one that occurred in June 2010 took two hours and 43 seconds.

There was a partial moonrise in November 1974 that lasted 3 hours 14 minutes. In May 1979, it lasted 3 hours 18 minutes.

NASA reports that the May 1956 partial eclipse lasted just four minutes longer than the Friday one. 

A partial lunar eclipse in 1892 was three hours 26 minutes long, while one in 1511 lasted three hour and 27 minutes. NASA data reveal that one which lasts longer than three hours 28 minutes can be found back at 1440. 

Partial eclipses are when most of the sunlight from the sun is blocked by the Earth. This causes the moon to appear reddish.

The Earth’s shadow blocks sunlight, but it still bends around the Earth, travels through the atmosphere and filters out the bluer wavelengths.

This filtered starlight is reflected as orange and red onto the moon. It causes the moon to look redder during an eclipse.

‘During a lunar eclipse, the Moon turns red because the only sunlight reaching the Moon passes through Earth’s atmosphere,’ according to NASA.

‘The more dust or clouds in Earth’s atmosphere during the eclipse, the redder the Moon will appear. 

‘It’s as if all the world’s sunrises and sunsets are projected onto the Moon.’

A number of factors affect how long the eclipse lasts, including the position of the moon in the Earth’s orbit.

It all depends on the position of Earth in relation to the sun.

From the moment that the Earth’s shadow starts to cover the moon it will eclipse for six hours and twenty-two minutes. This is the longest time since February 18th, 1440. 

Three factors determine the duration: how far the moon is away from Earth, how far the Earth from the sun and how close the sun, Earth, and moon are to each other at this point. 

Friday’s alignment of Earth and moon is perfect.

At 06:00 the moon is seen entering Earth’s pre-shadow (or penumbra) and departing penumbra at 12 :03 GMT (07 :03 ET). 

For three and a half hours tomorrow some parts of the world will see most of the moon change colour, turning red as it passed through the Earth's shadow

Tomorrow, for three-and-a-half hours, some areas of the globe will witness the majority of the moon’s colour change. It turns red when it passes through Earth’s shadow.

The duration is based on three things - how far away the moon is from the Earth, how far away the Earth is from the sun, and how closely aligned the sun, Earth and moon are at that point. This shows the moon entering the earth's shadow next to Sydney tower on July 27, 2018

It is determined by three factors: the distance between the Earth and the moon, the Earth’s distance from the sun, as well as how aligned Earth, sun, and moon at this point. On July 27, 2018, the moon entered the earth’s shadow near Sydney Tower.

According to the Royal Observatory, Greenwich, the partial eclipse will be 'barely visible in the UK' as it occurs when the moon is close to or below the horizon

The partial eclipse, according to Greenwich’s Royal Observatory, will not be visible in the UK if the moon passes close to or below it.

WHY IS THE MOON RAISED RED 

This same phenomenon, which makes the sky blue and sunsets red, also turns the Moon red when there is a lunar eclipse. 

It’s called Rayleigh scattering. 

Waves of light travel through the air, so different colors have unique physical properties. 

Blue light has a shorter wavelength and is scattered more easily by particles in Earth’s atmosphere than red light, which has a longer wavelength. 

The atmosphere is more direct for red light to travel. 

Blue light is visible when the Sun shines overhead. However, when the Sun goes down, light must travel through more atmosphere before it reaches our eyes. 

The Sun’s visible blue light is scattered away and the longer-wavelength yellow, orange and red light continues to pass through.

During a lunar eclipse, the Moon turns red because the only sunlight reaching the Moon passes through Earth’s atmosphere. 

The more dust or clouds in Earth’s atmosphere during the eclipse, the redder the Moon will appear. It’s as if all the world’s sunrises and sunsets are projected onto the Moon.

NASA.

The umbral eclipse, the part covered by Earth’s full shadow, will last for 3 hours and 28 minutes — the longest of the century.

It is 6 hours 1 minute long, and the penumbral shadow (when the moon passes through both the inner and outer portions of Earth shadow) will be the longest lasting in six centuries. 

In July 2019, the partial lunar eclipse lasted less than three hours. The one that occurred in June 2010 took two hours and 43 seconds.

There was a partial moonrise in November 1974 that lasted 3 hours 14 minutes. In May 1979, it lasted 3 hours 18 minutes.

NASA reports that the May 1956 partial eclipse lasted just four minutes longer than Friday’s due. 

A partial lunar eclipse in 1892 was three hours 26 minutes long, while one in 1511 lasted three hour and 27 minutes. NASA data reveal that one which lasts longer than three hours 28 minutes can be found back at 1440. 

Earth won’t see another of this duration until February 8, 2669, however there is a total lunar eclipse in May 2022, that should be visible from most of the UK.

The Royal Observatory Greenwich Astronomers stated that while the UK may not see every aspect of the solar eclipse in May 2022 they can still see totality (when the Moon turns red) when it occurs.

Dhara Patel recommends to anyone who still wants to attempt to spot Friday’s eclipse from the UK that they ‘find as clear a view of northwestern horizon possible’ and head north to areas of the UK where moonset is slightly later.

This gives ‘viewers the opportunity to catch the start of the Moon’s passing into the central part of the Earth’s shadow before it sets below the horizon. 

“Viewers will notice a difference in the Moon’s north-west limb as the shadow edge begins to rise, darkening it.

WHAT YOU’LL SEE AFTER THE MOON ENTERS EARTH’S SHADE 

TABLE TITLE
GMT EST PHASE DESCRIPTION
6:02 1.02 AM Beginning of the penumbral eclipse The Moon passes through the Earth’s shadow penumbra. Although the Moon starts to dimming, it is subtle.
7:19 2:19 AM Partially eclipse starts As the Moon enters Earth’s umbra, the partial eclipse starts. It looks as though the Moon is taking a bite out of its lunar disk when it moves into the umbra. You will see the dark side of the Moon within the umbra.
8:45 3:45 am It becomes obvious that red colour is visible The umbra covers more than 95% the Moon’s disc and will make it appear red. It might be more easy to spot the colour with binoculars, or even a telescope. With exposures lasting several seconds, a camera attached to a tripod will capture the colours. This can help expose only the illuminated part of the Moon.
9:03 4.03 AM Eclipse peak Peak of the eclipse is at 9:03 UTC This is when you can see the most intense red hue.
9:20 4.20 AM It is not possible to see red color anymore Redness diminishes when less than 95% are in Earth’s umbra. The Moon’s opposite side appears to have been bitten.
10:47 5:47 AM Partial eclipse ends Although the entire Moon lies in Earth’s penumbra (the dimming of which is also subtle),
12:04 7.04 am End of penumbral eclipse It is now over.

 SOURCENASA