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🎉 Craziest Goa Party Ever!
Get ready for unlimited fun as Jai, Vaibhav, and Premgi Amaren light up Goa with their unforgettable party moments in this hilarious scene. Packed with friendship, fun, and crazy vibes, this is one of the most entertaining sequences from the film!
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ove sparks unexpectedly when a chance meeting at a wedding changes everything in this heartwarming scene from Shokiwala. Watch Ajay Rao and Sanjana Anand share a memorable first encounter filled with emotions and charm.
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Get ready for an adrenaline-packed sequence from Dev. Watch Karthi in an epic non-stop car chase filled with action, thrill, and breathtaking moments. Featuring Rakul Preet Singh alongside Karthi, this exciting scene showcases the adventurous spirit and high-octane energy that make Dev a thrilling entertainer.
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Get ready to experience the exhilarating ride of 'Acham Enbathu Madamaiyada' as Simbu and Manjima traverse through roads of destiny, leading to the ultimate destination of love
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Instagram Subscription காசுகாக பண்றனா Reshma Pasupuleti open Interview @Reshmapasupuletiofficial
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Hello, my loves!
This was my first trip to Maldives and it was by far the most memorable holiday of my life. I talk about my time in this beautiful island nation, my love for yoga, scuba diving, food and life stuff.
Hope you enjoy. ♥️
Stayed at this gorgous property- @vvillasmaldivesatmirihi highly recommend it. ♥️
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Time stamps
1:18 - bangalore airport
1:36- Male airport
2:52- first night at the property
3:20- yoga on day 2
7:21- spa
7:53- meditation class
8:35- getting ready for sunset cocktail followed by dinner
9:00- woke up to a rainy day on day 3
9:14- scuba diving with philip
11:30- exploring the island
12:30- yoga on the beach
13:05- last day at the property
13:25- leaving male :(
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Welcome to my channel, travel, island, big city life, scuba diving, swimming, exploring the island, happy, YouTube, YouTube channel, yoga, meditation, spa, YouTube travel adventure , Bangalore airport, male, Maldives , what to do in Maldives
Part 1 : https://youtu.be/NCWBWYoxzkw
In this video we discussed the benefits of trees and their role in the world., we'll explore what would happen if the world didn't have any trees. We'll look at the environmental consequences of deforestation, the impact of deforestation on climate change, and the impact of deforestation on humanity.
So what would happen if the world lost all of its trees? Watch this video to find out! In this series, we're discussing some of the most important issues facing the world today, and we started with the question: what if there were no trees?
In the second part of this video, we talked about the importance of trees and the impact they have on our environment.
If you want to know what to do to help stop the deforestation of the world, be sure to watch part 1 and do you think Would the world be able to function without trees? What problems would arise?
Stay tuned for more videos on this topic!
#trees #benefitsoftrees #whatiftheworlddidn'thaveanytrees #theimpactofdeforestation #andtheimpactofdeforestationonhumanity #whatwouldhappeniftheworldlostallofitstrees #whatiftherewerenotrees #importanceoftrees #treetypes #tyesoftrees #treesage #tre #nationaltree #treename #christmasactivity #deforestation #chainsawman #treecuttingmachine #treecuttingmachine #humanextinction #vaanveli #tamil #treesintamil #gk #whatif #treehunt #shorts #earth
TOI 700 e is the latest planetary discovery in this solar system. In 2020, three other planets were also found orbiting the star TOI 700. Named TOI 700 b, TOI 700 c and TOI 700 d, they too are believed to orbit within the so-called optimistic habitable zone.
TOI 700 is a red dwarf 101.4 light-years away from Earth located in the Dorado constellation that hosts TOI 700 d, the first Earth-sized exoplanet in the habitable zone discovered by the Transiting Exoplanet Survey Satellite.
TOI-700 d is a super Earth exoplanet that orbits an M-type star. Its mass is 1.25 Earths, it takes 37.4 days to complete one orbit of its star, and is 0.1633 AU from its star. Its discovery was announced in 2020.
Regards,
Vaan Veli
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HI,
Composition: The Sun is primarily composed of hydrogen (about 74%) and helium (about 24%), with trace amounts of other elements.
Size: The Sun is an average-sized star, about 1.4 million kilometers (870,000 miles) in diameter. It's so large that about 1.3 million Earths could fit inside it.
Energy Source: The Sun generates energy through a process called nuclear fusion, where hydrogen atoms fuse to form helium. This process releases a tremendous amount of energy in the form of light and heat.
Temperature: The core of the Sun is incredibly hot, with temperatures reaching around 15 million degrees Celsius (27 million degrees Fahrenheit). The surface temperature, known as the photosphere, is cooler at about 5,500 degrees Celsius (9,932 degrees Fahrenheit).
Energy Output: The Sun emits an estimated 3.8 x 10^26 watts of energy, which is equivalent to the energy produced by about 100 billion nuclear bombs exploding every second.
Light Speed: It takes about 8 minutes and 20 seconds for sunlight to travel from the Sun's surface to Earth.
Life Cycle: The Sun is currently in the middle of its main sequence phase, where it has been shining for about 4.6 billion years. It's expected to continue this phase for another 5 billion years or so.
Solar Flares: The Sun occasionally experiences solar flares, which are intense bursts of radiation and energy. These flares can cause disruptions to communication systems and power grids on Earth.
Sunspots: Sunspots are cooler, darker areas on the Sun's surface caused by magnetic activity. They often occur in cycles, with the number of sunspots waxing and waning over an 11-year period.
Solar Wind: The Sun emits a stream of charged particles called solar wind, which constantly flows outward in all directions. This solar wind interacts with Earth's magnetosphere and can create phenomena like the auroras (northern and southern lights).
Gravity: The Sun's enormous mass creates a strong gravitational pull that keeps all the planets in our solar system, including Earth, in orbit around it.
Eclipses: Solar eclipses occur when the Moon passes between the Earth and the Sun, blocking out some or all of the Sun's light. Total solar eclipses, where the Sun is completely obscured, are rare and awe-inspiring events.
Regards,
VaanVeli
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Hi,
Star Classification: The Sun is a G-type main-sequence star, often referred to as a G-dwarf star or a yellow dwarf.
Size and Mass: The Sun is about 109 times the diameter of Earth and approximately 333,000 times its mass. It accounts for about 99.86% of the total mass of the entire Solar System.
Energy Source: The Sun's energy comes from nuclear fusion reactions occurring in its core, where hydrogen nuclei fuse to form helium, releasing a tremendous amount of energy in the process.
Light Travel Time: The sunlight we see from the Sun actually left its surface about 8 minutes and 20 seconds ago. This is because light takes time to travel the distance between the Sun and Earth.
Surface Temperature: The Sun's surface, known as the photosphere, has an average temperature of around 5,500 degrees Celsius (9,932 degrees Fahrenheit). However, the Sun's core temperature reaches millions of degrees Celsius due to the fusion reactions taking place there.
Solar Flares and Sunspots: The Sun's surface is not uniformly smooth. It has dark spots called sunspots, caused by the Sun's magnetic activity. Solar flares, which are bursts of energy and radiation, can also occur due to this magnetic activity.
Solar Wind: The Sun constantly emits a stream of charged particles called solar wind. This solar wind affects the space environment of the entire Solar System and interacts with the planets' magnetospheres.
Life Cycle: The Sun is approximately 4.6 billion years old and is roughly middle-aged in terms of its life cycle. It's currently in the phase where it's fusing hydrogen into helium in its core.
Future Evolution: In about 5 billion years, the Sun will exhaust its hydrogen fuel and enter a phase where it expands into a red giant, swallowing up Mercury, Venus, and possibly Earth. Eventually, it will shed its outer layers and become a white dwarf.
Solar Eclipses: Solar eclipses occur when the Moon passes between the Earth and the Sun, blocking out the Sun's light. Total solar eclipses happen when the apparent size of the Moon matches that of the Sun, creating a stunning visual effect.
Composition: The Sun is primarily composed of hydrogen (about 74%) and helium (about 24%). Other elements, such as oxygen, carbon, neon, and iron, make up the remaining percentage of its composition.
Size: The Sun is an average-sized star, classified as a G-type main-sequence star (G2V). Its diameter is about 109 times that of Earth, and it could fit more than 1.3 million Earths inside it.
Energy Source: The Sun generates energy through a process called nuclear fusion, where hydrogen nuclei combine to form helium, releasing an immense amount of energy in the form of light and heat.
Temperature: The temperature at the Sun's core is estimated to be around 15 million degrees Celsius (27 million degrees Fahrenheit). The surface temperature, known as the photosphere, is about 5,500 degrees Celsius (9,932 degrees Fahrenheit).
Light Travel Time: It takes about 8 minutes and 20 seconds for light from the Sun to reach Earth. This means that when we look at the Sun, we are actually seeing it as it appeared over 8 minutes ago.
Sunspots: Sunspots are temporary dark spots that appear on the Sun's surface due to magnetic activity. They are cooler regions compared to the surrounding areas and can vary in size.
Solar Flares and Coronal Mass Ejections (CMEs): The Sun occasionally experiences explosive events known as solar flares and CMEs, releasing bursts of energy and charged particles into space. These phenomena can affect Earth's space environment and cause geomagnetic storms.
Solar Wind: The Sun constantly emits a stream of charged particles called solar wind, which flows outward into space and influences the heliosphere, the region dominated by the Sun's magnetic field.
Lifecycle: The Sun is currently about 4.6 billion years old and is estimated to have a total lifecycle of around 10 billion years. It is currently in the middle stage of its life, where it fuses hydrogen into helium in its core.
Importance to Earth: The Sun is essential for life on Earth. It provides light and heat necessary for maintaining suitable conditions for life. It also drives the Earth's climate, weather, and various natural processes.
Sun's Magnetic Field: The Sun has a complex and dynamic magnetic field that gives rise to various solar phenomena, including sunspots, flares, and CMEs.
Regards,
VaanVeli
Santhosh
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Top Five Extinctions
Ordovician-silurian Extinction: 440 million years ago.
Devonian Extinction: 365 million years ago.
Permian-triassic Extinction: 250 million years ago.
Triassic-jurassic Extinction: 210 million years ago.
Cretaceous-tertiary Extinction: 65 million Years Ago.
Hi,
செத்து பொழச்ச பூமி JUST MISS | Dark Side of the Earth | பூமியின் வரலாறு
நம் பூமி உருவானபோ பல பேரழிவுகளை சந்தித்துள்ளது அதே போல் உயிரினங்கள் எப்படி உருவானது மற்றும் ஏற்பட்ட பேரழிவுகளால் உயிரினங்கள் எப்படி அழிந்தது , அனைத்தையும் நாம் இந்த பதிவில் தெரிந்துகொள்ளலாம்
Approximately 485.4 million to 443.8 million years ago. Here are some key points about the Ordovician period:
Sea Life: The Ordovician is known for the diversification of marine life. It saw the proliferation of various marine organisms, including trilobites, brachiopods, cephalopods, and early fish. Some of the first jawed fish appeared during this period.
Mass Extinction: Toward the end of the Ordovician period, there was a significant mass extinction event known as the Ordovician-Silurian extinction event. It is considered one of the Big Five mass extinctions in Earth's history
Continental Drift: During the Ordovician, the continents were positioned differently than they are today due to the process of plate tectonics.
Devonian extinction:
Timing: The Late Devonian extinction occurred over several million years, spanning the later part of the Devonian period. It's not a single, sudden event like some other mass extinctions.
Affected Organisms: The Devonian extinction primarily affected marine life. It had a particularly significant impact on marine organisms like corals, trilobites, brachiopods, and various types of jawless fish. Some groups, however, such as ammonoids, bony fish, and certain types of sharks, survived the extinction relatively unscathed.
Volcanic Activity: Intense volcanic activity could have released greenhouse gases into the atmosphere, leading to global warming and changes in ocean chemistry.
The Permian-Triassic extinction event, also known as the "Great Dying," is one of the most devastating mass extinctions in Earth's history. It occurred approximately 252 million years ago, marking the boundary between the Permian and Triassic periods. Here are key details about this catastrophic event:
Extent of Extinction: The Permian-Triassic extinction event is considered the most severe mass extinction event in Earth's history. It resulted in the loss of an estimated 90-96% of marine species and around 70% of terrestrial vertebrate species. It affected life on both land and in the oceans.
Volcanic Activity: One leading hypothesis is that extensive volcanic eruptions in an area now known as the Siberian Traps released massive amounts of lava and greenhouse gases. This led to significant global warming, acid rain, and changes in ocean chemistry, contributing to the environmental stress.
The Triassic-Jurassic extinction event is one of the five major mass extinctions in Earth's history, occurring approximately 201 million years ago, at the boundary between the Triassic and Jurassic periods. Here are key details about this extinction event:
Causes: The exact causes of the Triassic-Jurassic extinction are still debated among scientists, but several contributing factors have been proposed:
Volcanic Activity: Intense volcanic activity, particularly the eruption of the Central Atlantic Magmatic Province (CAMP), released large volumes of lava and greenhouse gases into the atmosphere. This led to global warming, ocean acidification, and changes in climate patterns.
Cretaceous-tertiary Extinction:
It occurred approximately 66 million years ago at the boundary between the Cretaceous and Tertiary (now known as the Paleogene) periods. Here are key details about this extinction event:
Extent of Extinction: The K-T extinction event resulted in the extinction of an estimated 75% of Earth's species, including many marine and terrestrial organisms. It is perhaps most famously known for causing the extinction of the non-avian dinosaurs.
Effects on Marine Life: Marine ecosystems experienced significant losses during the K-T extinction. Many marine reptiles, ammonites, and other marine species went extinct. Some groups, such as mammals, crocodiles, and some types of fish, survived the event.
நன்றி
Regards,
Vaan Veli
Santhosh
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What would earth be like without humans? Do you believe we could live without earth and do you believe the earth could exist peacefully without human ? Let's see what happens if there are no humans on the planet earth.
மனிதனின் கடைசி நொடிகளும் மனிதன் இல்லாத பூமியும்
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Vaan Veli
Santhosh
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Disclaimer:
This channel does not offer financial advice. All information on this channel is offered solely for educational and informational reasons. This channel does not guarantee that you will be able to generate money online using the method presented in the video. Your level of success in achieving the outcomes indicated in the video will involve hard work, aptitude, learning and experience. Before investing or joining any such site, this channel strongly suggested you to conduct thorough investigation.
In this video, we'll be discussing all the important Io Moon facts! From its name to its characteristics, this video is packed with information about the Io Moon.
If you're curious about the Io Moon, or want to know more about it, then this video is for you! We'll discuss everything you need to know about this fascinating moon, from its name to its characteristics. Be sure to watch until the end to learn about the amazing things that happen during the Io Moon!
IO Moon of Jupiter, IO Moon in tamil, IO Moon volcano eruption, IO Moon Surface, what is io mooon, IO moon temprature
Discovery: Io was discovered by Galileo Galilei on January 8, 1610, along with three other large moons of Jupiter.
Size: It is the fourth-largest moon of Jupiter and has a diameter of about 3,643 kilometers (2,263 miles).
Composition: Io is primarily composed of silicate rock and iron, similar to the terrestrial planets Mercury, Venus, Earth, and Mars.
Surface: Io has a diverse and geologically active surface, featuring numerous volcanic calderas, mountains, and plains.
Volcanic Activity: Io is the most volcanically active body in the solar system, with hundreds of active volcanoes spewing sulfur and other materials.
Lava Lakes: Some of Io's volcanic eruptions result in lava lakes, large molten pools of lava on its surface.
Ionian Name: Io is named after a priestess of Hera in Greek mythology who became one of Zeus's mortal lovers.
Orbit: Io orbits Jupiter at an average distance of about 422,000 kilometers (262,000 miles).
Orbital Period: It takes approximately 1.77 Earth days for Io to complete one orbit around Jupiter.
Tidal Heating: Io experiences intense tidal heating due to its elliptical orbit, caused by gravitational interactions with Jupiter and the other Galilean moons.
Surface Temperature: Io's surface temperatures can vary widely, with some regions reaching up to 1,600 degrees Celsius (2,900 degrees Fahrenheit).
Atmosphere: Io has a thin atmosphere composed mainly of sulfur dioxide, which freezes onto its surface when the moon is in shadow.
Surface Coloration: The surface of Io displays a variety of colors, including red, orange, yellow, and white, due to different types of materials and their oxidation states.
High Radiation Levels: Io is exposed to high levels of radiation from Jupiter's powerful magnetosphere, making it a challenging environment for spacecraft exploration.
Surface Changes: Observations over time have revealed significant changes in Io's surface features, indicating ongoing geological activity.
Peaks: Some of Io's mountains reach impressive heights, with several exceeding 10 kilometers (6 miles) in height.
Loki Patera: Loki Patera is a massive volcanic depression on Io, possibly a large lava lake or a complex system of interconnected lava lakes.
Surt Volcano: Surt is one of Io's prominent volcanoes, named after a fire giant in Norse mythology.
Prometheus: Prometheus is a large, elongated volcanic feature on Io with a distinctive shape, likely caused by repeated volcanic eruptions.
Voyager Missions: Io was first studied up close by NASA's Voyager 1 and Voyager 2 spacecraft in 1979.
Galileo Orbiter: The Galileo spacecraft, which orbited Jupiter from 1995 to
Regards,
Vaan Veli
Santhosh
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Disclaimer:
This channel does not offer financial advice. All information on this channel is offered solely for educational and informational reasons. This channel does not guarantee that you will be able to generate money online using the method presented in the video. Your level of success in achieving the outcomes indicated in the video will involve hard work, aptitude, learning and experience. Before investing or joining any such site, this channel strongly suggested you to conduct thorough investigation.
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The Chernobyl disaster happened on April 26 1986, at the Chernobyl Nuclear Power Plant in Pripyat, Ukrainian SSR, which was part of the Soviet Union at the time. It is often regarded as the worst nuclear disaster in history.
The incident occurred during a late-night safety test in Chernobyl's fourth reactor. A sudden power surge caused a large explosion and the discharge of a significant amount of radioactive elements into the atmosphere due to a combination of design defects and operator errors. Large amounts of radioactive particles, including iodine-131, cesium-137, and strontium-90, were discharged as a result of the explosion and ensuing fires.
The direct impact of the explosion killed two plant workers, and 29 more perished in the days that followed from acute radiation illness. The long-term effects of the Chernobyl tragedy were severe, with an increase in malignancies, particularly thyroid cancer, among people exposed to the radiation. To minimize future exposure, the affected area was evacuated and a huge exclusion zone was constructed.
Chernobyl had far-reaching consequences for nuclear energy policies, safety standards, and public opinion of nuclear power. It also contributed to the eventual breakup of the Soviet Union by highlighting the government's secrecy and reluctance to divulge information about the catastrophe. Significant changes resulted from the accident.
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Jupiter is the most largest planet in our solarsystem, Jupiter facts,
with a diameter of about 139,820 kilometers (86,881 miles).
It has a mass that is approximately 318 times that of Earth, making it more massive than all the other planets in the solar system combined.
Jupiter is primarily composed of hydrogen and helium, similar to the composition of the sun.
It doesn't have a solid surface; instead, its atmosphere gradually transitions into its dense, gaseous interior.
Jupiter has a thick atmosphere with bands of clouds and high winds.
Prominent features in its atmosphere include the Great Red Spot, a giant storm that has been raging for at least 350 years.
Jupiter has a very strong magnetic field, much stronger than Earth's.
Its magnetic field is responsible for intense radiation belts around the planet.
Jupiter has a large number of moons, with over 80 known as of my last update in January 2022.
The four largest moons, known as the Galilean moons, are Io, Europa, Ganymede, and Callisto.
Jupiter is the fifth planet from the Sun and has an average orbital distance of about 484 million miles (778 million kilometers).
It takes approximately 11.86 Earth years to complete one orbit around the Sun.
Jupiter's rotation is very fast; it completes one rotation on its axis in just under 10 hours.
Jupiter has a faint ring system composed of small, dark particles.
Its ring system is much less prominent than Saturn's.
Several spacecraft have visited Jupiter, including Pioneer 10, Pioneer 11, Voyager 1, Voyager 2, Galileo, and Juno.
Jupiter is often referred to as the "king" of the planets and plays a crucial role in the dynamics of the solar system.
Its immense gravity has helped shape the orbits of other planets and objects in the solar system.
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Watch this video to learn about the different types of asteroid impacts that have occurred on Earth. We'll compare some of the major hits and their effects on our planet. This fascinating look at asteroid impacts is brought to you by Vaan Veli. #asteroidhitcomparison #asteroidimpacts #vaanveli
Chicxulub Impact (Cretaceous-Paleogene Extinction Event): This impact occurred approximately 66 million years ago and is believed to have caused the mass extinction of dinosaurs.
Tunguska Event (1908): Although not caused by an asteroid, this event involved the explosion of a large airburst, likely a comet or asteroid, over Siberia. It flattened an estimated 80 million trees over an area of 2,150 square kilometers.
Barringer Crater (Meteor Crater): Formed around 50,000 years ago in Arizona, USA, this impact crater was created by an iron-nickel meteorite approximately 50 meters in diameter.
Chelyabinsk Meteor (2013): While not an impact, this was a significant event where a meteor exploded in the atmosphere over Russia, causing widespread damage and injuring thousands of people.
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Asteroids
Asteroid Comparison
Asteroid size comparison
The History of first life on our planet,
The earliest life on Earth is thought to have arisen around 3.5 to 4 billion years ago. The exact timeframe is difficult to pinpoint exactly due to the scarcity of geological and fossil data from that far period. The fossilized remnants of microbes such as bacteria and archaea provide the oldest evidence of life.
These early life forms were single-celled creatures that most likely lived in hydrothermal vents or shallow, warm oceans. The early Earth's atmosphere was significantly different from today's, with high amounts of gases such as methane, ammonia, and water vapor. Life is supposed to have originated when these basic creatures discovered the capacity to gather energy from their surroundings and reproduce.
Earth history, Human history, Earth History in tamil, History of earth, History of our life, Human evoluation
#earthhistory #historyofourearth #humanhistory #humanevolution
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Alpha Centauri is a triple star system in the southern constellation Centaurus. It has three stars: Rigil Kentaurus, Toliman, and Proxima Centauri. Proxima Centauri is the Sun's nearest star, at 4.2465 light-years.
Proxima A
Proxima B
Proxima C
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The Largest Galaxy In The Universe IC1101 பிரபஞ்சத்தின் மிகப்பெரிய Galaxy | IC 1101 is a supergiant elliptical galaxy in the constellation of Virgo, around 1.04 billion light-years from Earth. It is one of the biggest known galaxies in the visible universe, having a diameter of around 6 million light-years.
IC 1101 is categorized as a cD galaxy, which indicates it contains a large halo of stars around its main core. These galaxies are frequently observed near the cores of galaxy clusters and are thought to have evolved via the mergers of numerous smaller galaxies over billions of years.
The mass of IC 1101 is believed to be around 100 trillion times that of the Sun, making it one of the most massive galaxies known. Its immense size and mass indicate that it has been involved in countless galaxy mergers over its history, acquiring stars and other galactic material in the process.
IC 1101 was discovered in 1790 by the British astronomer Frederick William Herschel. Since then, astronomers have examined it extensively with various telescopes and technologies to better understand its structure, creation, and evolution.
#ic1101 #galaxy #universe #largestgalaxyintheuniverse #ic1101intamil
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The supermassive blackhole Sagittarius A is located at the heart of the Milky Way galaxy. சூரியனை விட 40 லட்சம் மடங்கு பெரிய கருந்துளை ,
Sagittarius A, also known as Sgr A*, is a supermassive black hole situated in the heart of the Milky Way galaxy. It is one among the most widely studied objects in astronomy. Sagittarius A* is predicted to have 4.1 million times the mass of our Sun, although it is concentrated in an area smaller than our solar system.
Sagittarius A*, despite its tremendous mass, does not produce light. Instead, it is detected indirectly by its influence on neighboring stars and gas clouds. Scientists have been able to establish the presence and mass of Sagittarius A* by studying the orbits of stars surrounding it.
Sagittarius A* also produces radio waves, which are thought to originate from the accretion disk of gas and dust swirling into the black hole. In recent years, astronomers have utilized more advanced techniques, like as very-long baseline interferometry (VLBI), to study Sagittarius A* with excellent accuracy.
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