Science 101

It is hypothesized to be the driving factor behind the accelerated expansion of the universe, a phenomenon first observed in the late 1990s by two independent research teams studying distant supernovae. Despite its significant presence, dark energy's exact nature remains one of the most profound mysteries in modern cosmology and physics.

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These remnants from the early solar system offer crucial insights into its formation and evolution. They vary widely in size, ranging from tiny pebbles to objects spanning hundreds of kilometers. The largest known asteroid, Ceres, is about 940 kilometers in diameter and is also classified as a dwarf planet. 

The Food 101 Foundation is dedicated to combating food insecurity and promoting nutritional well-being in underserved communities. Our primary goals include alleviating hunger by providing access to nutritious meals, educating communities on healthy eating habits, and supporting local food systems to ensure sustainable sources of nourishment. We advocate for policies that address the root causes of food insecurity, empower communities through initiatives like community gardens, and work to reduce food waste by redirecting surplus food to those in need. Additionally, we aim to enhance school meal programs to support children's development and raise public awareness to mobilize community support and volunteerism. Through these efforts, the Food 101 Foundation strives to create lasting change and build healthier, more resilient communities.

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One of Jupiter's most captivating features is its atmosphere, characterized by colorful bands and zones created by strong winds that blow in opposite directions. These bands, composed of ammonia clouds, vary in color from white and yellow to shades of red and brown. The interplay of these clouds creates a mesmerizing pattern that has intrigued astronomers for centuries. The planet's fast rotation, completing one spin in just under 10 hours, contributes to the dynamic and turbulent atmosphere.

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We are excited to announce a special fundraiser hosted by Book 101 Review podcast in support of less fortunate children around the world. Our goal is to foster a love for reading and provide essential educational resources to children who need them the most. By participating in this fundraiser, you can help us supply books, school supplies, and other learning materials to underprivileged communities. Every donation, no matter the size, will make a significant difference in a child's education and future. Join us in this noble cause and help us spread the joy of reading to every corner of the globe.

At its core, gravity is the attractive force that exists between all objects with mass. This force is what keeps planets in orbit around stars, holds galaxies together, and causes objects to fall to the ground on Earth. It was first mathematically described by Sir Isaac Newton in the 17th century, who formulated the law of universal gravitation. According to Newton, every mass exerts an attractive force on every other mass, with the force being directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers.

The event horizon of a black hole is one of the most captivating and enigmatic concepts in astrophysics. It represents the boundary surrounding a black hole, beyond which no information or matter can escape the gravitational pull. This invisible surface marks a point of no return, where the escape velocity exceeds the speed of light. The event horizon, therefore, creates a stark divide between the observable universe and the hidden singularity at the black hole's core. Understanding the event horizon is crucial for grasping the fundamental nature of black holes and the limits of our observable universe.

Its gravity holds the Solar System together, influencing the orbits of planets, moons, comets, and asteroids. This stellar giant is primarily composed of hydrogen and helium, undergoing nuclear fusion in its core, where hydrogen atoms combine to form helium, releasing a tremendous amount of energy. This process is the source of the Sun's light and heat, essential for life on Earth.

Predicted by Albert Einstein in 1916 as a consequence of his General Theory of Relativity, these waves propagate at the speed of light, carrying with them information about their cataclysmic origins and about the nature of gravity. Unlike electromagnetic waves, which travel through space, gravitational waves actually travel through spacetime itself, making them a unique messenger in the realm of astrophysics.