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The last total lunar eclipse of the year is set to take place on Tuesday, when the Earth blocks the Sun’s rays from reaching the Moon. Also known as the Blood Moon, the lunar eclipse will take place almost a year after the last total lunar eclipse, and viewers in North America, Central America, most of South America, the Pacific Ocean, Australia, New Zealand, and Asia will see the Moon darken and acquire a reddish hue on Tuesday. This will be the last total lunar eclipse until March 14, 2025.

How to watch the lunar eclipse

The Moon will traverse the northern half of Earth’s shadow, with totality predicted to last 86 minutes. Mid-eclipse happens on November 8th at 10:59 Universal Time (UT) or 4:29pm IST, around six days before apogee, when the Moon is farthest from Earth in its orbit. The actual clock times of the eclipse depend on your time zone.

You don’t need any equipment to observe a Blood Moon, but binoculars or a telescope can help enhance the view and the red colour of Earth’s only natural satellite.

You can also watch the lunar eclipse from the video embedded below

What to expect from the lunar eclipse

As a result, during the eclipse, the Moon will appear 7 percent smaller than it does when it’s at perigee (closest to Earth), but the difference is imperceptible. The eclipse on Tuesday will be a bit brighter than the one that occurred in May — especially in the Moon’s northern half — since the Moon doesn’t glide as close to the dark center of Earth’s shadow.

There are several delightful extras viewers can look out for while admiring the eclipse. During totality, Earth’s shadow dims the Moon sufficiently for stars to be visible right up to its edge. In addition, Uranus reaches opposition just a day after the eclipse, when it’s directly opposite the Earth from the Sun and at its closest and brightest.

And on eclipse night the distant planet will be upper left of the red-hued Moon — binoculars will reveal the planet’s pale disk. The farther west you are, the smaller the gap between planet and Moon. Also, the Northern and Southern Taurid meteor showers peak around this time, so eclipse-watchers might be treated to a few meteors streaking across the night sky.

All stages of the eclipse occur simultaneously for everyone, but not everyone will see the full eclipse. Weather permitting, observers in western North America will witness the entirety of the event on the morning of November 8, with the partial eclipse phase beginning an hour or so after midnight. In Hawai’i, the eclipsed Moon will be directly overhead. Viewers in the central parts of the continent will see all of totality and most of the final partial phases, while those on the East Coast can watch the Sun rise as totality ends.

South America will witness the initial phases of the eclipse up to totality, while Central America can enjoy the show a bit longer and see it through the total phase. The eclipse is an early evening event in central and eastern Asia, Australia, and New Zealand, and the Moon rises either during the earlier partial phases or during totality.

What to observe during the lunar eclipse.

The Moon’s leading edge enters the pale outer fringe of Earth’s shadow: the penumbra. You are unlikely to notice anything until the Moon is about halfway across the penumbra.

  1. Watch for a slight darkening on the Moon’s left side as seen from North America. The penumbral shading becomes stronger as the Moon moves deeper in.
  2. The penumbra is the region where an astronaut standing on the Moon would see Earth covering only part of the Sun’s disc.
  3. The Moon’s leading edge enters the umbra, the cone of Earth’s shadow within which the Sun’s completely hidden. You should notice a dramatic darkening on the leading edge of the lunar disk. With a telescope, you can watch the edge of the umbra slowly engulfing one lunar feature after another, as the entire sky begins to grow darker.
  4. The trailing edge of the Moon slips into the umbra for the beginning of total eclipse. But the Moon won’t black out completely: It’s sure to glow some shade of intense orange or red.
  5. Why is this? The Earth’s atmosphere scatters and bends (refracts) sunlight that skims its edges, diverting some of it onto the eclipsed Moon. If you were on the Moon during a lunar eclipse, you’d see the Sun hidden by a dark Earth rimmed with the reddish light of all the sunrises and sunsets ringing the world at that moment.
  6. The red umbral glow can be quite different from one eclipse to the next. Two main factors affect its brightness and hue. The first is simply how deeply the Moon goes into the umbra as it passes through; the center of the umbra is darker than its edges. The other factor is the state of Earth’s atmosphere. If a major volcanic eruption has recently polluted the stratosphere with thin global haze, a lunar eclipse can be dark red, ashen brown, or occasionally almost black.
  7. In addition, blue light is refracted through Earth’s clear, ozone-rich upper atmosphere above the thicker layers that produce the red sunrise-sunset colors. This ozone-blue light tints the Moon also, especially near the umbra’s edge. You’ll need binoculars or a telescope to see this effect.
  8. As the Moon progresses along its orbit, events replay in reverse order. The Moon’s edge re-emerges into the sunlight, ending totality and beginning a partial eclipse again.
  9. When all of the Moon escapes the umbra, only the last, penumbral shading is left. Sometime later, nothing unusual remains.

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T Corona Borealis May Erupt Soon: Rare Nova Could Be Visible to Naked Eye

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T Corona Borealis May Erupt Soon: Rare Nova Could Be Visible to Naked Eye

T Corona Borealis is a binary star system in the Northern Crown constellation which is being monitored closely by astronomers worldwide for signs of a rare stellar eruption. The system consists of a white dwarf and a red giant orbiting each other with the white dwarf pulling material from its companion. The gradual accumulation of matter on the surface of dwarf white planet can lead to a thermonuclear explosion, known as a Nova. Scientists recorded the last erupted Nova in 1946. Now, there have been some indications that we might experience another nova outburst in the near future.

The researchers have recorded a brightening event in 2015 followed by a dimming in 2023, which has mirrored the pattern seen in the last eruption. This leads the experts to believe that there might be another nova outburt. If an eruption occurs T Corona Borealis could become visible to the naked eye and shine as brightly as the most prominent stars.

Accretion Activity and Expert Predictions

According to a study published in the Monthly Notices of the Royal Astronomical Society, the system has exhibited behaviour similar to the years leading up to its previous eruption. T Corona Borealis is one of only eleven recurrent novae observed in recorded history with eruptions noted in 1217, 1787, 1866 and 1946. As per the latest data available with the researchers, the accretion disc surrounding the white dwarf has became highly active and bright between 2015 and 2023. The study reveals that this heightened activity could trigger an eruption within a year or two.

There are multiple predictions from the scientists based on orbital analysis suggesting possible eruption dates. As per multiple reports, the Nova outburst might take place between March 27 or November 10 this year or June 25, 2026. The researchers has also suggested a theory regarding a potential third object influencing the binary system. Astronomers like Dr Léa Planquart of Université de Strasbourg and Dr Jeremy Shears of the British Astronomical Association have dismissed this theory citing the absence of supporting evidence. Both experts believe the activity of the accretion disc remains the most likely cause of an impending eruption.

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Scientists Spot a Key Difference in Matter and Antimatter Decay

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Scientists Spot a Key Difference in Matter and Antimatter Decay

A key difference has been observed in the behaviour of matter and antimatter particles by researchers working at a particle physics laboratory. A new measurement has been carried out that recorded the decay of a specific type of matter particle and its antimatter equivalent. This development is being seen as significant because it may explain why the universe is filled with matter while antimatter is nearly absent. The discovery has been described as a step towards solving one of physics’ biggest mysteries.

New Study Reveals Baryon Decay Difference

According to the research shared by the LHCb experiment at CERN and posted on the arXiv preprint server, a difference has been recorded in how a particle called the beauty-lambda baryon and its antimatter counterpart decay. These particles belong to the proton family and are classified as baryons. The report further added that the decay was observed into a proton and three mesons based on data collected between 2009 and 2018.

The evidence suggests that the decay of the beauty-lambda baryon differs from its antimatter twin. According to sources involved in the study the likelihood of this difference being a random occurrence is less than one in three million. Tim Gershon who is a particle physicist at the University of Warwick and part of the research team told Nature that this is the first time such a difference has been spotted in baryons.

Experts Say Findings Could Aid Understanding of Matter’s Prevalence

Tara Shears who is a particle physicist at the University of Liverpool stated to Nature that the observation could offer new insight into why matter is found in abundance while antimatter is not. She said that this imbalance is one of the major unresolved questions in physics.

Yuval Grossman a theoretical physicist from Cornell University mentioned to Nature that while the current measurement does not fully explain the imbalance it helps add a crucial piece to the puzzle.

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China Loses 26 Percent of Its Glaciers Due to Global Warming, Claims New Study

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China Loses 26 Percent of Its Glaciers Due to Global Warming, Claims New Study

China has reportedly witnessed a significant decline in glacier area over the last six decades. As per a new study published online,  the country has lost nearly 26 percent of its total glacier coverage since the 1960s. The study claims that the lost of such glacier area might be due to the rapid increase in global temperatures around the globe. Official data confirmed that close to 7000 small glaciers have entirely vanished from the landscape. The shrinking of glacier masses has been observed to accelerate over the past few years as warming trends continue to intensify.

Glacier Loss Confirmed by Chinese Academy of Sciences

According to a study released by the Northwest Institute of Eco-Environment and Resources under the Chinese Academy of Sciences it was recorded that China’s glacier area had reduced to nearly 46000 square kilometres by 2020. The total number of glaciers was stated to be around 69000 at that time. This marked a steep fall from an earlier figure of approximately 59000 square kilometres reported between 1960 and 1980 when glacier count stood at roughly 46000.

Impact of Glacier Retreat on Water Security and Environment

The melting of glaciers has raised concerns over freshwater availability across several regions. Environmental agencies have cautioned that the loss of glacier mass may result in higher competition for water resources in the years to come. The Tibetan Plateau which hosts a large portion of these glaciers has been referred to as the Third Pole owing to the vast ice reserves it holds.

Efforts to Slow Glacier Melting

Attempts have been made by Chinese authorities to slow the melting process through technological interventions. Artificial snow systems and snow blankets have been deployed as part of these initiatives.

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