For centuries, humanity has looked up at the night sky and wondered: Are we alone in the universe? Do Aliens exist? With advances in space exploration, astrobiology, and technology, the search for alien life has never been more intense. While we have yet to find definitive proof of extraterrestrial beings, multiple scientific discoveries suggest that life beyond Earth may be more than just a possibility, it might be an eventual certainty.
Existing Evidence Supporting Alien Life
1. The Discovery of Exoplanets in the Habitable Zone
Thanks to telescopes like Kepler and James Webb Space Telescope (JWST), astronomers have discovered thousands of exoplanets (planets outside our solar system). Many of these planets, such as those in the TRAPPIST-1 system, exist within their star’s “habitable zone,” where conditions might be right for liquid water which is one of the essential ingredients for life as we know it.
2. Organic Molecules Found Beyond Earth
Scientists have found organic molecules, the building blocks of life, on Mars, Saturn’s moon Enceladus, and even in interstellar space. In 2018, NASA’s Curiosity rover detected complex organic compounds on Mars, suggesting that the planet might have once supported microbial life. Additionally, water plumes on Enceladus contain organic materials, hinting at a potentially habitable environment beneath its icy crust.
3. The Mysterious Case of Venus’ Atmosphere
In 2020, researchers discovered phosphine gas in the atmosphere of Venus. On Earth, phosphine is primarily produced by microbial life in oxygen-free environments. While this does not confirm alien life on Venus, it raises questions about unknown biological or chemical processes occurring on the planet.
4. The Fermi Paradox and the Great Silence
One of the biggest mysteries in the search for extraterrestrial life is the Fermi Paradox: If the universe is so vast, why haven’t we found alien civilizations yet? Some theories suggest that intelligent life is incredibly rare, while others propose that advanced civilizations may be avoiding us or are simply too far away to communicate.
Are We Close to a Breakthrough?
With upcoming missions like the Europa Clipper (to explore Jupiter’s moon Europa, which has a subsurface ocean) and the continued search for biosignatures in exoplanet atmospheres, scientists believe we are closer than ever to answering the age-old question.
While we haven’t found direct evidence of extraterrestrial life yet, the discoveries of exoplanets, organic molecules, and potential biosignatures suggest that at least in microbial form, alien life could exist somewhere in the vast universe. It does not matter if we will find life, but when.
Conclusion
The search for alien life continues to be one of the most exciting fields of scientific exploration. As technology advances and space missions become more ambitious, the possibility of discovering life beyond Earth grows stronger. Whether we find microbes on Mars, complex organisms on an exoplanet, or intelligent civilizations through radio signals, the answer may come sooner than we think.
Until then, we keep looking to the stars with curiosity and hope.
In the ever-evolving landscape of space exploration, the notion of humans living on Mars has shifted from science fiction to a tantalizing possibility. With technological advancements, ambitious missions, and some of the brightest minds working toward this goal, the dream of establishing a human presence on the Red Planet is closer than ever. But how realistic is it, and what challenges remain for making life there?
The Vision of Mars Colonization
For decades, the red planet has captured humanity’s imagination. The idea of sending humans to Mars is not new. Science fiction writers like H.G. Wells and Arthur C. Clarke envisioned Martian civilizations, while more recent films and books like The Martian and Red Mars have only amplified our collective curiosity.
The red planet has a day that lasts 24.6 hours, polar ice caps, and a surface area comparable to Earth’s dry land. These features make it seem like a potential “second home” for humanity if we can overcome the hurdles involved in reaching and surviving on its surface.
The Space Agencies and Private Enterprises Leading the Charge
NASA has been at the forefront of Mars exploration for years. The space agency’s Mars rover missions, like Curiosity and Perseverance, have been vital in uncovering the planet’s secrets, revealing that it once had conditions suitable for life. NASA’s Artemis program aims to return astronauts to the Moon by the late 2020s, a stepping stone toward future Mars missions.
In parallel, private companies like SpaceX are pushing the boundaries of space technology. Elon Musk’s ambitious goal to establish a self-sustaining city on Mars by the mid-21st century has caught the public’s imagination. SpaceX’s Starship, currently under development, is designed to carry large payloads and passengers to Mars, showcasing the potential for mass space travel.
Challenges: The Harsh Realities of the Red Planet
While the idea is appealing, the journey and long-term survival are fraught with challenges. Solar System facts you never knew make this task even more daunting. Some of the most significant hurdles include:
1. Distance and Travel Time
On average, it is about 225 million kilometers (140 million miles) from Earth. This vast distance depends on the relative positions of Earth and Mars in their orbits. Prolonged space travel poses serious risks, including radiation exposure, muscle atrophy, and psychological stress from isolation.
2. Life Support and Sustainability
Mars has a thin atmosphere composed mostly of carbon dioxide, with very little oxygen, and surface temperatures can dip as low as -125°C (-195°F). In addition, the planet has no liquid water on its surface (except for trace amounts in polar ice caps). This means future settlers would need to rely on advanced life support systems, technologies to produce oxygen, water, and food, and habitats capable of shielding them from harsh radiation.
One promising technology is the use of in-situ resource utilization (ISRU), which focuses on extracting and utilizing local resources—such as harvesting carbon dioxide to produce oxygen or water from ice deposits—rather than relying on constant shipments from Earth.
3. Radiation Exposure
Mars lacks a magnetic field and a thick atmosphere to protect against harmful cosmic and solar radiation. Without Earth’s protective layers, any humans living on Mars would be exposed to radiation levels that could significantly increase the risk of cancer, genetic mutations, and other health problems. Developing reliable radiation shielding for habitats and spacesuits is a critical component of any Mars mission.
4. Psychological and Social Challenges
Spending extended periods on the red planet presents psychological challenges. The isolation, distance from Earth, and confinement in small, enclosed spaces could lead to mental health issues such as depression, anxiety, and interpersonal conflicts. Solving these problems might involve rigorous training, creating systems to ensure psychological well-being, and designing habitats that promote social interaction and relaxation.
What the Future Holds
In the next few decades, we will likely see human missions to the red planet, though they will probably be short-term exploratory missions rather than permanent colonization. But the groundwork being laid today is crucial for the future. If successful, Mars could become humanity’s first off-world settlement, a crucial stepping stone for future space exploration.
Some experts believe that Mars could be terraformed in the long term to support human life more easily. But this process, if feasible, would likely take centuries or even millennia, and it remains highly speculative.
The Hubble Space Telescope (HST) is one of the most important astronomical instruments ever created, revolutionizing our understanding of the universe. Launched in 1990, it has provided invaluable data and images that have reshaped science across multiple fields, from cosmology to stellar evolution. Below is an in-depth exploration of the Hubble Space Telescope, detailing its importance, capabilities, and impact on modern astronomy.
What Is the Hubble Space Telescope?
The Hubble Space Telescope is a large, space-based observatory that orbits Earth. Unlike ground-based telescopes, it is positioned beyond the Earth’s atmosphere, which allows it to capture clear, unobstructed images of distant objects in the universe. Among some cool facts about the universe, the Hubble telescope is a joint project involving NASA, the European Space Agency (ESA), and the Canadian Space Agency (CSA). It is named after the American astronomer Edwin Hubble, whose work in the 1920s led to the discovery of the expanding universe.
The telescope is equipped with a 2.4-meter (7.9-foot) diameter primary mirror and a suite of scientific instruments, including cameras, spectrometers, and other sensors designed to collect a wide range of data from visible, ultraviolet, and near-infrared wavelengths. This broad range of capabilities makes Hubble an incredibly versatile tool for studying different types of celestial objects, from nearby planets to far-off galaxies.
The Significance of Hubble
Hubble’s importance lies in its ability to provide images and data that are unobstructed by Earth’s atmosphere, which distorts and absorbs light. Ground-based telescopes, while powerful, suffer from these atmospheric limitations, which can blur observations. In contrast, the Hubble Space Telescope has provided astronomers with incredibly sharp images and accurate data that have advanced our knowledge of the universe in several significant ways.
Cosmology and the Expansion of the Universe
One of the most groundbreaking contributions of Hubble has been its role in helping refine our understanding of the age and size of the universe. In 1998, Hubble’s observations provided crucial evidence that the universe’s expansion was accelerating, a discovery that led to the concept of dark energy, a mysterious force driving this acceleration. Hubble’s precise measurements of distant galaxies and their redshifts were essential in determining the expansion rate, offering critical insights into cosmology.
Deep Field Observations
In 1995, Hubble captured the “Hubble Deep Field,” an image of a seemingly empty patch of sky that revealed thousands of distant galaxies. This observation provided an unprecedented look at the universe’s distant past, offering insights into galaxy formation and evolution. Subsequent deep field observations, such as the Hubble Ultra Deep Field, have further expanded our understanding of the universe’s origins.
Stellar and Planetary Formation
Hubble has also provided detailed images of nebulae, star clusters, and other cosmic phenomena that have enhanced our knowledge of stellar birth and evolution. The telescope’s ability to observe in ultraviolet and near-infrared wavelengths has been particularly useful for studying young stars and planetary systems. Its images of regions like the Eagle Nebula, where new stars are forming, have offered spectacular views of the processes that shape stars and planets.
Exoplanet Discovery and Atmospheric Studies
In recent years, Hubble has been instrumental in the study of exoplanets, or planets outside our solar system. By observing the way starlight filters through an exoplanet’s atmosphere, Hubble has helped scientists detect the chemical composition of these distant worlds. This has paved the way for further exploration into the possibility of life on planets beyond Earth.
Hubble’s Design and Operation
The Hubble Space Telescope is positioned in a low Earth orbit, about 547 kilometers (340 miles) above the planet’s surface. Its orbit allows it to avoid the distortion caused by Earth’s atmosphere, which is crucial for capturing high-resolution images. The telescope’s primary mirror, which is 2.4 meters in diameter, collects light from astronomical objects, and its scientific instruments analyze the light to gather information about the objects’ composition, motion, and other properties.
Hubble’s instruments include:
Wide Field Camera 3 (WFC3)
A versatile camera that can capture images in ultraviolet, visible, and near-infrared wavelengths.
Advanced Camera for Surveys (ACS)
A camera is used for studying distant galaxies, star clusters, and large-scale structures in the universe.
Cosmic Origins Spectrograph (COS)
An instrument designed to analyze light from distant objects and study the composition of intergalactic gas.
Space Telescope Imaging Spectrograph (STIS)
A tool that measures the light spectrum of astronomical objects, providing detailed information about their properties.
Hubble was designed for servicing missions, meaning that astronauts could visit the telescope in space to repair, maintain, and upgrade its instruments. This ability was crucial in keeping the telescope at the forefront of technological advancements, and several servicing missions were conducted between 1993 and 2009. These missions helped repair flaws in Hubble’s optics, replace aging equipment, and install more advanced instruments.
Conclusion
The Hubble Space Telescope has been an essential tool for astronomers and scientists, offering insights that have deepened our understanding of the cosmos. Its contributions to cosmology, stellar and planetary science, and the study of exoplanets are unmatched, and its legacy will continue to shape the future of space exploration.
In 2019, astronomers unveiled the first-ever image of a black hole. Captured by the Event Horizon Telescope (EHT), this image marked a monumental achievement in our understanding of the universe. It wasn’t just a snapshot of a black hole but a glimpse into space’s mysterious and enigmatic heart. But what does this remarkable image tell us about black holes, space, and the nature of our cosmos? Let’s dive in and explore.
The First-Ever Image of a Black Hole: A Historic Milestone
Before the first-ever image of a black hole was captured, black holes were purely theoretical objects. Their existence was supported by mathematics and our understanding of general relativity, but no one had ever “seen” one. For years, black holes were thought to be invisible to telescopes because of their gravitational pull, which is so strong that not even light can escape. The idea of photographing something that couldn’t even emit light seemed impossible. However, scientists were determined to make the impossible possible.
In April 2019, the EHT collaboration revealed an image of the black hole at the center of the galaxy M87. This was an astounding achievement, marking a scientific breakthrough that captured the imagination of people all over the world. The image showed a glowing, orange ring of light surrounding a dark central region — the shadow of the black hole itself. It was a visual confirmation of Einstein’s theory of general relativity in action.
The Technical Feats Behind the First-Ever Image of a Black Hole
You may be wondering how scientists were able to capture such an elusive and distant object. The first-ever image of a black hole was not taken using a regular telescope but rather a global network of radio telescopes, a technique called Very Long Baseline Interferometry (VLBI). By combining data from radio telescopes spread across the globe including locations in the Arctic, Hawaii, and Spain, scientists created an image with a resolution sharp enough to capture the event horizon of a black hole nearly 55 million light-years away.
The data collected was vast, amounting to petabytes of information, far exceeding what typical telescopes gather. This massive volume of data came from a global network of radio telescopes, each contributing a piece to the puzzle. The process of stitching this immense dataset together into a single, coherent image took years of computational effort.The result was nothing short of extraordinary. The first-ever image of a black hole was the product of collaboration between thousands of scientists, engineers, and mathematicians worldwide.
What Does This Discovery Mean for the Future?
The first-ever image of a black hole is just the beginning. With more advanced technology and more powerful telescopes, astronomers are now equipped to study black holes with even greater precision. In the future, we may be able to capture more detailed images of black holes, study their magnetic fields, and gain deeper insights into their role in the formation of galaxies.
This discovery also opens new doors in our understanding of the universe, allowing us to explore more about our mysterious cosmos. Black holes are not just cosmic oddities; they could hold the key to answering some of the most fundamental questions about space, time, and the nature of reality. The Event Horizon Telescope team is already working on new projects to capture images of other black holes, including one at the center of our own Milky Way galaxy, known as Sagittarius A*.
The first-ever image of a black hole is a monumental achievement in science, providing a window into a previously invisible and mysterious part of the universe. It confirms some of our long-held theories while raising new questions and possibilities. With future advances in technology and more global collaborations, we can look forward to even more discoveries about these fascinating objects.
The solar system is a fascinating and complex part of our universe, full of incredible wonders and hidden secrets. While most of us are familiar with the basic planets and the Sun, many surprising facts might just blow your mind. Here are five solar system facts that you may have never known about the solar system.
There Are More Than 200 Moons Orbiting Planets in Our Solar System
Most people are familiar with Earth’s Moon, but did you know that there are over 200 moons orbiting planets in our solar system? Jupiter alone has 92 moons, including the massive Ganymede, which is even larger than the planet Mercury! Saturn follows closely behind with 83 moons. These moons vary greatly in size and composition, and some, like Europa and Enceladus, might even have the potential to support life.
Venus Has a Day Longer Than Its Year
Venus is known for its extreme temperatures and thick atmosphere, but one of its most unusual characteristics is that its day lasts longer than its year. A day on Venus equals 243 Earth days, while a year (the time it takes to orbit the Sun) only lasts about 225 Earth days. This means a day on Venus is longer than its year by almost 20 days!
The Largest Volcano in the Solar System Is on Mars
Olympus Mons, located on Mars, is the largest volcano in the solar system. It stands about 13.6 miles (22 kilometers) high—almost three times the height of Mount Everest! It’s also about 370 miles (600 kilometers) in diameter, making it roughly the size of the state of New Mexico. Scientists believe that the lack of tectonic plate movement on Mars allowed Olympus Mons to grow to such an enormous size.
There’s a “Dwarf Planet” in the Outer Solar System
Pluto may be the most famous dwarf planet, but it’s not the only one. The solar system contains several other dwarf planets, most of which lie beyond Neptune in a region called the Kuiper Belt. Eris, which is slightly smaller than Pluto, is one of the most notable dwarf planets. These objects are just as fascinating as the larger planets, with many still holding secrets about the early days of the solar system.
The Sun Makes Up 99.86% of the Solar System’s Mass
The Sun is by far the largest object in our solar system, holding nearly all of the system’s mass. In fact, it contains about 99.86% of the total mass of the entire solar system. If you could fit the Sun inside a ball, over 1.3 million Earths could fit within it! The Sun’s gravity also keeps all the planets, moons, and other objects in orbit around it.
The Solar System facts are Full of Surprises
While the solar system may seem familiar with its eight planets and the Sun, it’s full of fascinating and surprising facts. From the extreme length of a Venusian day to the massive Olympus Mons on Mars, the solar system is a place of wonder. As we continue to explore and learn more about our cosmic neighborhood, there’s no telling what other secrets we’ll uncover.
Is the Earth Really Flat? For centuries, people believed the Earth was flat, but modern science has thoroughly debunked this myth. The Earth is an oblate spheroid, slightly flattened at the poles and bulging at the equator due to its rotation. Astronauts have captured stunning images of the round Earth from space, and scientists have long known that the curvature can be observed through various phenomena, such as the way ships disappear over the horizon or the changing position of the stars as you travel north or south.
The Flat Earth Theory: A Historical Perspective
For centuries, many believed that the Earth was flat, and this idea was widely accepted by ancient civilizations. However, as human understanding of science advanced, so did our knowledge of the Earth’s true shape.
Modern Science Debunks the Myth
Today, scientists know that the Earth is an oblate spheroid, meaning it is slightly flattened at the poles and bulges at the equator. This has been confirmed through space missions, satellite imagery, and careful observation.
Evidence from Space and Astronomy
One of the most convincing proofs of a round Earth comes from space exploration. Astronauts aboard the International Space Station (ISS) have captured clear images showing the Earth as a sphere. Additionally, during lunar eclipse and total solar eclipse, the Earth’s shadow cast on the Moon is always round, further supporting the idea of Earth’s spherical shape. The way the Earth’s shadow moves across the Moon during these events also provides strong evidence of its roundness.
Everyday Observations That Prove the Earth Is Round
You don’t need to go to space to see evidence of Earth’s curvature. The way ships disappear over the horizon, or how the stars change position as you travel north or south, are simple, everyday examples of how the Earth’s round shape affects our world.
The Bottom Line, Is the Earth really flat? No, it is not.
While the flat Earth theory persists among a small group of believers, overwhelming evidence from astronomy, physics, and our own observations proves that the Earth is round. The myth of a flat Earth has been thoroughly debunked, and the science is clear—our planet is a sphere.
On March 18, 1965, history was made when Soviet cosmonaut Alexei Leonov became the first human to walk in space. This remarkable achievement marked a major milestone in the space race and the advancement of human space exploration. In this article, we will take a closer look at Alexei Leonov’s life, his groundbreaking spacewalk, and its impact on the future of space exploration.
The Early Life of Alexei Leonov
The Early Life of Alexei Leonov
Born on May 30, 1934, in the small town of Listvyanka, Soviet Union, Alexei Arkhipovich Leonov’s journey to becoming a cosmonaut began with his early fascination with aviation. He graduated from the Kachinsk Air Force Pilot School and later joined the Soviet Air Force, where he became a skilled pilot. His aviation expertise and remarkable physical endurance made him an ideal candidate for the Soviet space program.
Selection for the Soviet Space Program
In 1960, the Soviet Union began its search for cosmonauts to join its space program, and Alexei Leonov was selected as one of the initial candidates. After undergoing extensive training, including rigorous physical and psychological tests, Leonov was chosen to be part of the Voskhod 2 mission. His training would prepare him for one of the most challenging and dangerous feats in the history of space exploration: a spacewalk.
The Historic Spacewalk: Voskhod 2 Mission
The Voskhod 2 mission, launched on March 18, 1965, was the first time a human would leave the confines of their spacecraft to float freely in space. As part of the mission, Leonov’s primary objective was to conduct an extravehicular activity (EVA), or spacewalk. Equipped with a specially designed space suit and tethered to the spacecraft, Leonov opened the airlock and stepped out into the vacuum of space.
The spacewalk lasted 12 minutes and 9 seconds, during which Leonov floated freely in space, becoming the first person to do so. This momentous event was a significant achievement for both the Soviet space program and humanity’s understanding of space. However, the spacewalk was not without challenges.
The Challenges of Spacewalking
Leonov faced numerous difficulties during his spacewalk. One of the most significant challenges he faced as the first human to walk in space was the expansion of his spacesuit in the vacuum of space. As Leonov floated outside the spacecraft, the lack of atmospheric pressure caused his suit to inflate, making it difficult for him to move and return to the spaceship. At one point, he found himself unable to get back into the airlock due to the suit’s rigidity.
In a moment of desperation, Leonov was forced to release some of the pressure in his suit to fit back into the airlock. This decision, though risky, allowed him to re-enter the spacecraft safely. Despite the challenges, Leonov’s spacewalk was a triumph and demonstrated the potential for future human exploration beyond the spacecraft.
Aftermath and Legacy
Following his historic spacewalk, Leonov continued his career as a cosmonaut and later became a prominent figure in the space industry. His achievement in 1965 paved the way for future space missions, including the Apollo moon landings and the development of space stations such as the International Space Station (ISS).
Leonov’s spacewalk was a key turning point in the space race between the United States and the Soviet Union. It demonstrated that human space exploration was possible and laid the groundwork for future missions to the Moon, Mars, and beyond.
Alexei Leonov’s spacewalk on March 18, 1965, was a groundbreaking achievement that changed the course of space exploration. His courage, determination, and resourcefulness during the mission helped to advance human space travel and inspire future generations of astronauts. As the first human to walk in space, Leonov’s legacy continues to live on in the history of space exploration, reminding us of the incredible possibilities that await beyond our planet.
The moon is the natural satellite of the earth. You may have noticed that the moon is slightly different every other day. This is because the moon is going through phases.
What is a moon phase?
To understand the reason for the different phases of the moon, you need to understand what a moon cycle is.
Firstly, the moon does not have its light. It reflects the light of the sun. The sun’s rays hit the moon and this is why we can see the moon shine at night.
Secondly, the moon orbits the Earth. It orbits the Earth. Because it is constantly in motion, not all of the moon receives sunlight. This is why we see only a part of the moonshine. The part of the moon that receives the sunlight is the part of the moon you can see from the earth.
What are the different phases of the moon?
Phases of the moon
New moon: This is when the unilluminated face of the moon faces the earth. This is when you see no moon in the sky.
Waxing Crescent: This is when you see the silver of the moon in the sky. When the day-part of the moon is mostly facing away from the earth. This is called a crescent moon and looks like a ‘C’.
First Quarter: The first quarter moon is also known as the half-moon. You can see more of the moon than just a crescent. It rises at noon and sets at midnight.
Waxing Gibbous: The waxing gibbous moon phase is more illuminated than a ‘half-moon’. It is not a complete full moon, but it is not a half moon either.
Full moon: During the full moon phase, the illuminated side of the moon faces the earth and we see a full, circular moon. It tends to light up the night with its silver light.
Waning Gibbous: This is when the moon is turning away again. The moon decreases in size and this phase comes after the full-moon phase.
Third Quarter: The third quarter is also known as the last quarter. The half-illuminated portion of the moon faces the Earth, making the moon look half.
Waning Crescent: During the waning crescent moon phase, you can see only silver or white. This is because only a small portion of the moon faces the earth, making a small crescent illuminated and visible.
What are moon cycles and moon phases?
The moon cycle is the cycle of the moon around the sun.
It takes about 28 days for the moon to orbit the Earth. As the moon orbits the Earth, the moon tends to change its phases. There are 8 different phases of the moon; four primary phases and four secondary phases.
The moon does not have its light. It reflects the light of the sun. And because it is continuously orbiting the Earth, only part of the moon receives the sunlight. The moon absorbs the sunlight and reflects a portion of it. It is this portion of the reflected sunlight that we see from Earth.
Conclusion
It takes 29.5 days for a moon to orbit the Earth. During this moon cycle, the moon goes through 8 different phases. The earth is interesting in itself but, even the heavenly body outside is equally amazing.
FAQs
1. What are the 8 moon cycles?
The 8 moon cycles are waxing crescent, first quarter, waxing gibbous, full moon, waning gibbous, third quarter, and waning crescent.
2. Are all the moon cycles 28 days?
It usually takes 29.5 days for a moon to cycle the Earth. During the sidereal month, it takes 27 days, 7 hours, and 43 minutes to orbit the earth and complete a cycle.
3. How long is a 12-moon cycle?
A lunar year or 12-moon cycle takes about 354 days.
4. Are moon cycles monthly?
Yes, moon cycles complete in a month.
5. What is a full moon cycle?
It is the time interval between a full moon and the repetition of the same phase. It lasts about 29.53 days.
Our universe is so big and many events are constantly taking place. We may not be able to experience all of them because of how vast the universe is. Watching a total solar eclipse is one such celestial event.
People have always been fascinated by this for many years and this year is no different. The total solar eclipse of 2024 is said to last twice the normal eclipse so, here are some precautions you should take before watching the eclipse.
What is a total solar eclipse?
A total solar eclipse occurs when the moon comes in between the earth and the moon. This causes the shadow of the moon to be cast on a portion of the earth. A rare total eclipse is going to take place on April 8, 2024. Parts of the world will be able to experience this celestial event.
What makes it so unique and different from the rest of the eclipse is the length of the eclipse. This eclipse is said to be twice as long as a normal eclipse. But before going out to see this eclipse, you need to keep a few things in mind. Here are a few things you need to make sure are in check.
Things you need to know before watching a total solar eclipse
Glasses with solar filters
It is advised that you get glasses with a solar filter. You may think you could use any of your goggles to watch the eclipse, but that is not the case. All the glasses cannot filter the radiation of the sun that would permanently or temporarily damage your eyesight.
Solar eclipse needs special glasses to safely watch. And even though 3D glasses look similar to eclipse glasses, you should not use them.
Time of the total eclipse
Keep track of the time of the eclipse. They do not last very long so double-check the time of the eclipse so that you don’t miss out. This is a very rare event; if you have the chance, you should make sure you experience this surreal celestial event. It is said to begin at 11:07 am, starting at Mexico’s Pacific coast.
If you live in the United States, make sure you get your eclipse glasses ready before noon. And if you’re in Canada, you will be experiencing the eclipse from around 2 pm which will end in the evening. Keep yourself updated with the eclipse news so you don’t miss out.
The 2024 total solar eclipse can be seen in many cities across North America. Here are some important places and the times when the eclipse will happen there.
The data information is sourced from the NASA website.
USA total eclipse time:
Location
Partial Begins
Totality Begins
Maximum
Totality Ends
Partial Ends
Dallas, Texas
12:23 p.m. CDT
1:40 p.m. CDT
1:42 p.m. CDT
1:44 p.m. CDT
3:02 p.m. CDT
Idabel, Oklahoma
12:28 p.m. CDT
1:45 p.m. CDT
1:47 p.m. CDT
1:49 p.m. CDT
3:06 p.m. CDT
Little Rock, Arkansas
12:33 p.m. CDT
1:51 p.m. CDT
1:52 p.m. CDT
1:54 p.m. CDT
3:11 p.m. CDT
Poplar Bluff, Missouri
12:39 p.m. CDT
1:56 p.m. CDT
1:56 p.m. CDT
2:00 p.m. CDT
3:15 p.m. CDT
Paducah, Kentucky
12:42 p.m. CDT
2:00 p.m. CDT
2:01 p.m. CDT
2:02 p.m. CDT
3:18 p.m. CDT
Carbondale, Illinois
12:42 p.m. CDT
1:59 p.m. CDT
2:01 p.m. CDT
2:03 p.m. CDT
3:18 p.m. CDT
Evansville, Indiana
12:45 p.m. CDT
2:02 p.m. CDT
2:04 p.m. CDT
2:05 p.m. CDT
3:20 p.m. CDT
Cleveland, Ohio
1:59 p.m. EDT
3:13 p.m. EDT
3:15 p.m. EDT
3:17 p.m. EDT
4:29 p.m. EDT
Erie, Pennsylvania
2:02 p.m. EDT
3:16 p.m. EDT
3:18 p.m. EDT
3:20 p.m. EDT
4:30 p.m. EDT
Buffalo, New York
2:04 p.m. EDT
3:18 p.m. EDT
3:20 p.m. EDT
3:22 p.m. EDT
4:32 p.m. EDT
Burlington, Vermont
2:14 p.m. EDT
3:26 p.m. EDT
3:27 p.m. EDT
3:29 p.m. EDT
4:37 p.m. EDT
Lancaster, New Hampshire
2:16 p.m. EDT
3:27 p.m. EDT
3:29 p.m. EDT
3:30 p.m. EDT
4:38 p.m. EDT
Caribou, Maine
2:22 p.m. EDT
3:32 p.m. EDT
3:33 p.m. EDT
3:34 p.m. EDT
4:40 p.m. EDT
Canada total eclipse time:
Location
Partial Begins
Total Begins
Maximum
Total Ends
Partial Ends
New Brunswick, Fredericton
2:21 PM ADT
4:32 PM ADT
4:38 PM ADT
4:38 PM ADT
5:43 PM ADT
Ontario, Sault Ste. Marie
12:54 PM EDT
3:12 PM EDT
3:27 PM EDT
3:27 PM EDT
4:36 PM EDT
Quebec, Montreal
2:08 PM EDT
3:24 PM EDT
3:24 PM EDT
3:24 PM EDT
5:44 PM ADT
Nova Scotia, Halifax
3:23 PM ADT
4:39 PM ADT
4:41 PM ADT
4:41 PM ADT
5:46 PM ADT
Prince Edward Island, Charlottetown
3:26 PM ADT
4:35 PM ADT
4:38 PM ADT
4:38 PM ADT
5:44 PM ADT
Newfoundland, St. John’s
2:25 PM EDT
5:09 PM NDT
5:16 PM NDT
5:16 PM NDT
6:18 PM NDT
Mexico total eclipse time:
Location
Partial Begins
Total Begins
Maximum
Total Ends
Partial Ends
Mazatlán, Sinaloa
10:28 AM MDT
12:28 PM MDT
12:30 PM MDT
12:32 PM MDT
2:00 PM MDT
Durango, Durango
10:51 AM MDT
12:08 PM CST
12:23 PM CST
12:23 PM CST
1:43 PM CST
Torreón, Coahuila
10:58 AM CST
12:16 PM CST
12:32 PM CST
12:32 PM CST
1:51 PM CST
Please keep in mind that these times are close estimates and might differ a bit depending on where you are in the city. Make sure to watch the eclipse safely by using suitable eye protection!
Making an eclipse projector
You can also have fun in the eclipse and do a little science project and make an eclipse projector. To make this, you need to cover a small hole in a cardboard box and cover it with aluminum foil. Create a small hole in the foil and hold it against the sun so light can pass through it.
This will project an image of the sun on the second piece of cardboard. You may have to adjust the distance between the two pieces to get a clear image. Now you can see the eclipse safely.
Protect your skin
If you’re in the Southwest region, then you could be in the sun for a while. So, keep your sunscreen ready and keep an umbrella close by. You will be grateful for the shade you have. If you don’t, you could get sunburnt and they are not fun.
Keep your camera on standby
The total eclipse will last for a time less than you expect it to last. So, keep all of your equipment ready. The eclipse of April 8 2024 is supposed to last for twice as long as a normal eclipse.
Which parts of the world will experience the total solar eclipse of 2024?
Mexico’s Pacific coast is going to experience a total solar eclipse at around 11:07 a.m. PDT. Then the eclipse will go across the United States, touching down in Texas, and journeying through Oklahoma, Arkansas, Missouri, Illinois, Kentucky, Indiana, Ohio, Pennsylvania, New York, Vermont, New Hampshire, and Maine.
The eclipse will then make its way into Canada, gracing Southern Ontario, and continuing through Quebec, New Brunswick, Prince Edward Island, and Cape Breton. Finally, as the sun sets, the eclipse will end on continental North America on the Atlantic coast of Newfoundland, Canada, at 5:16 p.m. NDT.
It is a remarkable event that you cannot miss out on. Mark the date on the calendar, and make a checklist of things you need to keep in mind before looking at the total solar eclipse. Let your close friends and family know about it too!
Make sure you are well-equipped to see the solar eclipse. You will need solar-filter eclipse glasses, sunscreen, and an umbrella to have a pleasant experience.
What should we not do during the solar eclipse?
You should not look directly at the sun during the solar eclipse. It can blind you partially or fully(temporarily or permanently).
Is it safe to look at a total solar eclipse?
Even if it is dark, it is not safe to look at a total solar eclipse without specialized protection.
What happens during a total eclipse?
During a total solar eclipse, the moon comes in between the earth and the sun which casts a shadow on the earth.
Should I look at the eclipse?
You can watch the eclipse with eclipse-safe equipment, even your camera needs protection.
How rare is a total eclipse?
An eclipse occurs every 1.5 years.
Should I not go out during the solar eclipse?
You can go out during the solar eclipse but do not look at the eclipse with naked eyes.
Being an astronaut is such an amazing thing, you get to explore the world outside of the one we reside in. It is natural to want to know more about them. This article will walk you through 10 surprising facts about astronauts that are sure to blow your mind.
1. The oldest man in Space
John Glenn was the oldest man to be in outer space. He was 77 years old when he took off in Space Shuttle Discovery. There truly is no age limit for things you are passionate about.
2. First meal on the moon
Neil Armstrong and Buzz Aldrin were the first astronauts on the moon. They landed on the moon on July 20, 1996. They had bacon cubes, peaches, 3 sugar cookies, a pineapple grapefruit drink, and coffee for their first meal.
3. The time machine effect
According to Einstein’s theory of relativity, astronauts in space go back 10 million seconds in time, but they get back to normal when they enter the Earth’s atmosphere. Every time an astronaut circles the earth’s orbit, they return a few seconds.
4. Skin peeling off of astronauts
This may not be a popular news but, the skin of the astronauts in space tends to peel. This is because they do not walk like on Earth, making their soles feel soft and flakey. This does not usually smell or irritate, but they keep this in check using steroid cream.
5. Weightlessness in space
The astronauts feel intensely weightless because the fluids in the body get distributed. The blood and lymph in the legs get redistributed by the pressure. This makes them feel nauseous and sick. This weightlessness is not the best sensation and causes severe disorientation. It takes time for the astronauts to get used to it.
6. Chocolatier in Space
Helen Sharman worked at Mars, a chocolate bar company. He was a chemist there. When she heard of the opening for applicants to be the first British explorer, she applied and was selected out of 13,000 applicants. She was only 26 years old and went out into the space more than just once.
7. Valentina Tereshkova’s whereabouts
When Valentina left for training to become an astronaut, she told her mother that she was in camp training to be a pro skydiver. It was later when the entire landing was what Tereshkova was training for. She was shocked when she saw her daughter in space when the shuttle orbited the Earth.
8. Height requirement
Not every passionate person can be an astronaut. There are several checklists that they need to clear before they are considered to be a part of the space team. Height is one such requirement. The astronauts need to be taller than 5’2 feet. But not every tall person gets a pass. You cannot be an astronaut if you are taller than 6’3 feet.
9. Astronauts from the first moon landing were in quarantine
People did not know much about space, so naturally the first astronauts who landed on the moon on Apollo 11 were quarantined when they returned from space. This was to ensure that the astronauts were not infected with any deadly virus or radiation. They continued doing this till Apollo 14, after which they declared that the moon did not affect the astronaut’s health in a contagious way.
10. Coming back to earth is very overwhelming
Space is an empty vacuum and you don’t have much sound in the rocket too. So when astronauts come back home, it is not just the sense of being back that feels overwhelming but it is the noise and all the other earthly sounds. It is not just the physical body that needs time to adjust, it is the mental health that needs time for adjustments too.
These were some of the surprising facts about astronauts. You probably learned something new. Being an astronomer is a very cool job, but it comes with a lot of work. Some people are driven like Valentina and John Glenn, but their gender or age did not stop them from pursuing what their hearts desired.