Connect with us

Published

on

The first solar eclipse of 2024 is all set to darken the skies on April 8. This particular event will be a total solar eclipse, a rare occurrence on Earth. After this event, the next total solar eclipse in the same region will not be seen for two more decades. A total solar eclipse of similar impact is expected in 2044. This event will mainly be visible in North America, including Mexico, the US, and Canada. While a few more territories will observe it partially, the rest of the world cannot see it directly. Here’s everything you need to know about the latest solar eclipse, along with a list of all upcoming solar eclipses and more.

 

Total Solar Eclipse 2024: Date, Time, and Place

The total solar eclipse of 2024 will occur on April 8. The total darkening of the sky, also known as totality, will be visible across a 185-kilometre stretch between Mexico, the US, and Canada. It will start on Mexico’s Pacific coast at 11:07am PDT, and the eclipse will end on the Atlantic coast of Newfoundland, Canada, at 5:16pm NDT. As many as 18 different US States will also get to see it.

The total solar eclipse will not be visible from India. It will begin at 9:12 pm IST, a few hours after the Sun is set. Totality will start at 10:08pm IST, and the eclipse will end at 2:22am IST on April 9.

Total Solar Eclipse 2024: How to Watch it Live Online

While people in India and other countries, excluding North America, cannot physically witness the total solar eclipse, astronomy enthusiasts can still follow it online. There will be multiple live streams covering this rare celestial event. NASA will start its live stream on April 8 at 5:00pm GMT (10:30pm IST) and continue until 8:00pm GMT (1:30am IST). You can watch the stream here.

Skywatching website timeanddate.com will also live stream the total solar eclipse on its YouTube channel starting at 4:30pm GMT (10:00pm IST) on April 8. The stream will provide real-time updates and background information as well.

Finally, the University of Maine will send a high-altitude science balloon into the sky and live stream a view of the total solar eclipse from the stratosphere. It can be watched here on April 8, starting at noon GMT (5:30pm IST).

Total Solar Eclipse 2024: List of Countries to Watch the Celestial Event

The total solar eclipse of 2024 will only be visible in some parts of Mexico, the US, and Canada.

List of Upcoming Solar Eclipse

According to data from timeanddate.com, the following solar eclipses are expected to be observed from the Earth.

Date Type Location
April 8, 2024 Total North America
October 2, 2024 Annular North and South America
March 29, 2025 Partial Europe, North Asia, North and West Africa
September 29, 2025 Partial South Australia
February 17, 2026 Annular Southern Africa, South America
August 12, 2026 Total Europe, North Asia
February 6, 2027 Annular Africa, South America
August 2, 2027 Total Europe, South Asia

What is a Solar Eclipse?

A solar eclipse is an astronomical phenomenon where the Moon passes between the Earth and the Sun and blocks the Sun’s light either entirely or partially. These events are infrequent and occasional since the Moon needs to be in the same plane as the Sun and the Earth, which does not always happen. Even when an alignment does occur, it is more likely to be partial than full. This is the reason why total solar eclipses are so rare.

On average, the Earth can get between two to five solar eclipses in a year. However, most of these are partial eclipses and are not very noticeable. Total eclipses are dramatic and turn the sky dark, but they are only visible from a few locations. This is why the opportunity to experience an eclipse is often called a once-in-a-lifetime opportunity.

Different Types of Solar Eclipses

There are three types of solar eclipses. A solar eclipse can be defined as partial, total, or annular, depending on the Moon’s position. Here are the full details:

Partial solar eclipse: A partial solar eclipse occurs when the Moon partially covers the Sun, but some of the Sun’s light can still reach the Earth. When a partial solar eclipse occurs, a portion of the Sun appears to have vanished. It can be observed in a larger area.

Total solar eclipse: A total solar eclipse occurs when the Moon and the Sun are on the same plane, and the Moon is at such a distance from the Earth that it covers the Sun for a brief period. Unlike a partial solar eclipse, it is usually visible from a smaller strip of land.

Annular solar eclipse: Finally, during an annular solar eclipse, the Moon is placed far away from the Earth and is unable to cover the Sun entirely. At the peak of this solar eclipse, the Moon covers the central portion of the Sun, and only a ring of light can be seen from the Earth.

Things to Remember to View Upcoming Solar Eclipse Safely

While it is never recommended to look directly at the Sun since its intense brightness and harmful ultraviolet radiation can cause permanent damage to the unaided eye, this becomes even more important during a solar eclipse. Darkened skies can create a false impression that the Sun’s intensity is reduced and that it is safe to look at it; however, any escaping sunlight will cause the same amount of damage to the eye. This is why precautions must always be taken before viewing a solar eclipse event.

1. People should use safe solar viewing glasses when watching a solar eclipse directly.

2. Regular sunglasses, no matter how dark, are not safe to look at the Sun directly.

3. Binoculars, camera lenses, telescopes, or any other optical devices should not be used with solar viewing glasses, as concentrated solar rays can burn through the filter.

4. Proper solar filters should be added to optical devices before viewing the Sun through them.

5. If solar glasses are unavailable, people can opt for indirect viewing of the solar eclipse. NASA highlighted the pinhole projector method, where a small hole punched into an index card can project an image of the Sun on a surface through which the eclipse can be seen.

Frequently Asked Questions (FAQs) 

What is so special about the solar eclipse 2024?

The 2024 total solar eclipse is one of the rare celestial events that occur across the globe. It will be the most watched solar eclipse as it passes through various large cities. Moreover, it is also the last total solar eclipse across the United States for 20 years.  

How long will the 2024 eclipses last?

According to official NASA data, the total solar eclipse will last 4 minutes and 28 seconds. In most places, it will be visible for approximately 3.5 and 4 minutes. 

What is the timing of solar eclipse on 8 April 2024?

As per the Indian Standard Time (IST), the total solar eclipse will start at 9:12 pm, while the totality will begin at 10:08 pm. The eclipse will end on April 9, 2024, at 2:22 am. 

Is the April 8th solar eclipse visible in India?

Sadly, the total solar eclipse will only be visible in the United States and not in India. 
 

Continue Reading

Science

Hubble finds missing globular cluster in Milky Way’s crowded stellar halo

Published

on

By

Hubble finds missing globular cluster in Milky Way’s crowded stellar halo

A striking new image captured by NASA’s Hubble Space Telescope has shed light on an underexplored gatekeeper of our galactic neighbours’ achievements and tragedies. Adorned with multi-hued stars, the spherical cluster glitters amid the expanse of stars in our Milky Way galaxy. This type of globular cluster is a very dense grouping of stars — about the same mass as 100,000 suns — that orbit all around the centre of their galaxy. Stars in a cluster are typically roughly the same age, as they formed from the same collapsing gas cloud. In this new view, stars show up in temperatures indicated in red and blue colours: red for colder and blue for hotter stars.

Hubble Maps Forgotten Star Cluster ESO 591-12 to Uncover Milky Way’s Ancient Stellar Secrets

As per a report from NASA’s Hubble team, ESO 591-12 was imaged during the Hubble Missing Globular Clusters Survey—an initiative targeting 34 Milky Way globular clusters that had never been observed by the space telescope. The aim is to construct a comprehensive database of the ages, distances, and stellar populations of all the galaxy’s known globular clusters and star formations. However, it has always been tough for telescopes on Earth to pick out individual stars in these densely populated regions, so Hubble’s high resolution has done much to finally be able to track the movements of stars to unlock their histories and formation.

The ESO 591-12 data are part of an ongoing study to improve knowledge of the formation and evolution of globular clusters in the galaxy’s bulge and halo. These star clusters are cosmic fossils that have preserved cosmic conditions from the primordial universe. Their work helps build a fuller narrative of the evolution of the Milky Way and how it has changed over billions of years.

This new image is a further example of how advanced space-based observing facilities are helping astronomers to excavate the contents of the dark and dusty skeleton cloaking the Milky Way and sculpt a better understanding of not only the universe’s evolution but also that of our cosmic home.
Each one tells part of the astronomical story, and Hubble is digging out new chapters to enrich the tale, such as probing data for clusters as much as ESO 591-12, which have been mostly neglected until now. This finding adds to our knowledge of the early universe by shining a spotlight on something that was in plain sight.

For the latest tech news and reviews, follow Gadgets 360 on X, Facebook, WhatsApp, Threads and Google News. For the latest videos on gadgets and tech, subscribe to our YouTube channel. If you want to know everything about top influencers, follow our in-house Who’sThat360 on Instagram and YouTube.


Very Massive Stars Blow Away Outer Layers in Powerful Winds Before Black Hole Collapse

Continue Reading

Science

Massive stars shed extreme mass before collapsing into black holes

Published

on

By

Massive stars shed extreme mass before collapsing into black holes

New research indicates that the most monstrously huge stars — those more than 100 times as massive as the sun — shed at least 20 times more matter before they collapse than previously thought to do so as they cool off to become black holes. These stars blow off a significant portion of their outer layers in quite powerful stellar winds over the brief but intense course of their lives, leaving behind low masses at the end. One benefit of this extreme mass loss is that it can account for observed strangeness in stars such as those in the Tarantula Nebula, providing new information on stellar evolution, black hole formation, and sources of gravitational waves.

Hurricane-like Stellar Winds Explain Extreme Mass Loss in Universe’s Most Massive Stars

As per a report from Space.com, researchers used sophisticated models and observations to learn that very massive stars give off winds so powerful they act more like hurricanes than gentle solar breezes. Their results agree very well with observations of WNh-type Wolf-Rayet stars in the Tarantula Nebula, which are hotter and more compact than would be expected by standard models. The improved models explain the very high temperatures at the surface and the stability of hydrogen, which address previous challenges.

One key subject in this study is R136a1 — the most massive known star — with a mass up to 230 times that of the sun. The researchers suggested that it either formed as a single star of around 200 solar masses or as a binary star system where the two stars had a combined mass of about 200 solar masses. In both such cases, the star must have lost a huge amount of mass early in its life, so the findings would call into question how it is that massive stars can live long enough to leave such a wreckage in the Large Magellanic Cloud.

The implications extend to black hole formation as well. More massive stellar winds erode more mass, resulting in the production of smaller black holes and decreasing the chances of creating elusive intermediate-mass black holes. This revision also enhances the matches of the model with the observed gravitational wave signal of a coalescing black hole binary.

Although the models are restricted to stars in the Tarantula Nebula, the researchers stress that in order for their findings to be considered universal, it is important to understand stars in different chemical environments as well. The results not only reshape predictions of black hole populations but may also adjust our understanding of how the most massive stars in the universe live — and die.

For the latest tech news and reviews, follow Gadgets 360 on X, Facebook, WhatsApp, Threads and Google News. For the latest videos on gadgets and tech, subscribe to our YouTube channel. If you want to know everything about top influencers, follow our in-house Who’sThat360 on Instagram and YouTube.


New Interstellar Comet 3I/ATLAS Speeds Through Solar System

Continue Reading

Science

Astronomers Capture First-Ever Image of a Dead Star That Exploded Twice in Rare Supernova Event

Published

on

By

Astronomers Capture First-Ever Image of a Dead Star That Exploded Twice in Rare Supernova Event

For the first time, a team of astronomers has captured a clear image of a white dwarf star that exploded not just once, but twice, as a Type Ia supernova — a “double-detonation” that scientists hadn’t thought possible until now. The extraordinary observation could revise our long-held notions of how stars die, suggesting that some stars can explode as supernovas without ever crossing the Chandrasekhar limit, the minimum mass normally thought necessary for such an explosion. The astronomers employed the Very Large Telescope’s MUSE instrument to zoom in on the four-century-old supernova remnant SNR 0509-67.5, which sits 60,000 light-years away in the constellation Dorado, revealing evidence of two separate blasting catastrophes in its construction.

First Visual Proof Shows White Dwarfs Can Explode Twice Without Reaching Chandrasekhar Limit

As the researchers report on July 2 in Nature Astronomy, the team found a distinctive “fingerprint” in the debris of SNR 0509-67.5 in the Large Magellanic Cloud that the models predicted. White dwarfs—which are the dead stage of sun-like stars—usually blow up into Type Ia supernovas after they hit the Chandrasekhar limit by stealing matter from a neighbouring star.

However, this finding shows that the detonation can be launched at an earlier time. The explosion is likely to have a two-step origin, the team argues, with the initial blast being generated when an unstable layer of helium that the star had acquired exploded on its surface; the resulting shock wave then drove a second and main detonation.

“This physical proof of a double-detonation not only helps solve a long-standing mystery of what causes these explosions, but it represents the most visually compelling evidence for this origin.” Priyam Das, University of New South Wales, team leader and author.

Something is happening to Type Ia supernovas, the “standard candles” used to measure cosmic distances, because their brightness doesn’t fluctuate. But they have long mystified scientists with how they explode. Until this discovery, an explosion white dwarf that didn’t surpass the Chandrasekhar limit was only considered in theory.

This fresh visual evidence for the double detonation model further informs our knowledge of stellar evolution and also informs how we should interpret light from distant supernovas. More than its scientific implications, its discovery adds a colourful new page to the story of dying stars — stars that, as it now appears, will not go gently into that night but will light up the sky twice over in fantastic fireworks before vanishing from the cosmos.

Continue Reading

Trending