The universe is everything that exists, including all space, time, matter, and energy. It can be described as all existing matter and space taken as a whole, also called the cosmos. The observable universe is about 93 billion light-years in diameter and contains hundreds of billions of galaxies. The universe has been expanding since the Big Bang, which occurred approximately 13.8 billion years ago.
Galaxies are large systems bound by gravity that contain stars, gas, dust, and dark matter. They range in size from dwarf galaxies with a few million to several billion stars to giant galaxies with up to about one hundred trillion stars. The word galaxy comes from the Greek galaxias (γαλαξίας), meaning “milky,” referring to the Milky Way. Most stars in a galaxy move in orbits around its central region under the influence of gravity.
Galaxies are commonly classified into four main types based on their shape and structure: elliptical, spiral, lenticular, and irregular.
Elliptical galaxies are smooth, round to elongated systems with little internal structure. They contain very small amounts of gas and dust and show little or no ongoing star formation. Most of their stars are old, typically several billion years in age, and are mainly low-mass, reddish stars. Blue, young stars are rare. Their brightness is highest at the center and gradually decreases toward the edges. Elliptical galaxies are supported mainly by random stellar motions rather than strong rotation, although some do rotate slowly.
Spiral galaxies, including the Milky Way, are disk-shaped systems with a bright central bulge and spiral arms that extend outward. They are classified into two main types: normal (unbarred) spiral galaxies and barred spiral galaxies, which have a bar-shaped structure across the center. The spiral arms contain large amounts of gas and dust and are regions where new stars are actively forming, making them appear bright and prominent. While stars orbit the galactic center, the spiral arms themselves are patterns of higher density rather than fixed structures.
Lenticular galaxies (also called S0 galaxies) are an intermediate type between spiral and elliptical galaxies. They have a disk and a central bulge like spiral galaxies, but lack prominent spiral arms. They contain very little gas and dust, so there is little or no new star formation. Most of their stars are old, similar to those in elliptical galaxies. Visually, they appear as smooth, lens-shaped systems with a bright center and a faint disk.
Irregular galaxies are a class of galaxies that lack a definite shape such as spiral or elliptical forms. They have no clear symmetry or organized structure. Many irregular galaxies contain large amounts of gas and dust and show active star formation, which is why they often appear bright and blue due to the presence of young, massive stars. Their unusual shapes are commonly the result of gravitational interactions or past collisions with other galaxies. Unlike spirals and ellipticals, their stars do not follow well-defined orbital patterns, though the galaxies as a whole still rotate.
Galaxies are vast systems of stars, gas, dust, and dark matter bound together by gravity. Astronomers estimate that the observable universe contains hundreds of billions of galaxies.
The Milky Way galaxy began forming more than 13 billion years ago and continues to evolve through star formation and mergers with smaller galaxies. It produces several new stars each year from clouds of gas and dust.
The Milky Way is part of a collection of galaxies known as the Local Group, which contains over 50 known galaxies, including the Andromeda Galaxy and the Magellanic Clouds. The Local Group itself is part of a much larger structure called the Virgo Supercluster.
Relative to the cosmic microwave background radiation, the Milky Way is moving through space at about 600 kilometers per second (around 370 miles per second).
Galaxies come in different shapes and sizes. About one-third of known galaxies are elliptical, while most of the rest are spiral or irregular in form. Dwarf galaxies are the most common type and usually contain only a few billion stars, making them much smaller than large spiral galaxies like the Milky Way.
Typical galaxies range from about 1,000 to 100,000 parsecs in diameter. One parsec equals about 3.26 light-years or roughly 31 trillion kilometers.
Some of the most distant known galaxies formed only a few hundred million years after the Big Bang. One such example, GN-z11, is observed as it appeared about 13.4 billion years ago, making it one of the earliest galaxies ever detected.
Studies of galaxy rotation, especially in the Andromeda Galaxy, provided key evidence for the existence of dark matter. These observations were pioneered by astronomer Vera Rubin, who showed that visible matter alone could not explain galactic motion.
The idea that galaxies are separate “island universes” was suggested in the 18th century by philosopher Immanuel Kant, long before telescopes could confirm it.
Lenticular galaxies are considered transitional forms between spiral and elliptical galaxies. They have disk-like shapes but lack visible spiral arms and contain little gas for new star formation.
Most large galaxies are believed to host a supermassive black hole at their centers. The Milky Way contains one known as Sagittarius A*, which has a mass millions of times that of the Sun.
Black holes themselves do not create galaxies, but they influence the motion of nearby stars and gas and play an important role in galaxy evolution. The term “black hole” was introduced in 1967 by physicist John Archibald Wheeler.
The Andromeda Galaxy (also called Messier 31) is a spiral galaxy located about 2.5 million light-years from Earth and is the largest member of the Local Group. It is moving toward the Milky Way, and the two galaxies are expected to merge in about 4–5 billion years.
Some galaxies experience bursts of intense star formation and are known as starburst galaxies. One example is the so-called Fireworks Galaxy, which has produced many observed supernovae in recent decades.
Flocculent spiral galaxies lack clearly defined spiral arms and instead appear patchy and fragmented. The Sunflower Galaxy (M63) is an example of this type.
The Milky Way alone likely contains hundreds of billions of stars and potentially billions of planetary systems.
Galaxy classification was first systematized by astronomer Edwin Hubble, who grouped galaxies into spirals, ellipticals, lenticulars, and irregulars based on their appearance.
The Coma Cluster is a massive collection of thousands of galaxies located about 320 million light-years from Earth.
A light-year is the distance light travels in one year, about 9.46 trillion kilometers. The Milky Way has a diameter of roughly 100,000 light-years.
From Earth, several galaxies can be seen without a telescope under dark skies, including the Andromeda Galaxy, the Magellanic Clouds, and the Triangulum Galaxy.
Some galaxies contain trillions of stars, making them among the largest known structures in the universe. The largest known galaxies are giant elliptical galaxies found at the centers of galaxy clusters.
Galaxies can collide and merge without stars directly crashing into each other because the distances between stars are extremely large compared to their sizes.
When galaxies merge, they often trigger intense periods of star formation called starbursts due to the compression of gas clouds.
The shape of a galaxy can change over time through gravitational interactions with neighboring galaxies.
Spiral galaxies rotate in an organized disk, while elliptical galaxies are supported mainly by random stellar motions rather than rotation.
Some galaxies are almost entirely made of dark matter, with very little visible matter. These are called dark galaxies and are difficult to detect.
Galaxies often exist in long chains and sheets known as cosmic filaments, forming a vast structure called the cosmic web.
The space between galaxies is not empty; it contains hot gas, dust, and dark matter.
Active galaxies contain extremely bright central regions powered by supermassive black holes. These are called active galactic nuclei (AGN).
Quasars are among the brightest objects in the universe and are powered by supermassive black holes in young galaxies.
Some galaxies stop forming stars entirely and become quiescent galaxies.
Galaxies can eject gas into intergalactic space through powerful winds caused by supernovae and black hole activity.
The first galaxies formed only a few hundred million years after the Big Bang.
Galaxies are surrounded by large invisible regions of dark matter called dark matter halos.
Most of a galaxy’s mass is actually in its dark matter halo rather than in its stars.
Some galaxies are isolated, while others belong to clusters containing thousands of galaxies.
The color of a galaxy reveals its age: blue galaxies are rich in young stars, while red galaxies are dominated by older stars.
Radio galaxies emit powerful radio waves from jets launched by their central black holes.
Galaxies can steal stars from one another through gravitational tidal forces.
There are galaxies with almost no stars, composed mostly of gas.
Some dwarf galaxies orbit larger galaxies like satellites, such as the Magellanic Clouds orbiting the Milky Way.
Galaxies do not have sharp edges; their outer regions gradually fade into intergalactic space.
A solar system is formed when a star and the group of celestial bodies bound to it by gravity come together. These bodies, which include planets, moons, asteroids, and comets, revolve around the star. Our solar system formed about 4.6 billion years ago from a cloud of gas and dust, with the Sun at its center.
The solar system consists of the Sun, eight planets (Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune), along with dwarf planets, moons, asteroids, comets, and other small bodies held together by gravity.
About 1.3 million Earth-sized planets could fit inside the Sun by volume.
The solar system formed around 4.6 billion years ago from a cloud of gas and dust known as the solar nebula. Its collapse may have been triggered by a shock wave from a nearby supernova explosion.
Thousands of planetary systems have been discovered around other stars in our galaxy, showing that solar systems are common in the universe.
Sunlight takes about 8 minutes and 20 seconds to reach Earth.
Venus is the hottest planet, with an average surface temperature of about 460°C, while Uranus has the coldest recorded atmospheric temperatures, reaching about –224°C. Earth’s average surface temperature is about 15°C.
Jupiter has the largest number of known moons in the solar system, with over 90 confirmed moons, while Saturn also has more than 80 known moons.
After the Moon, Venus is the brightest natural object in the night sky.
Venus is often called the morning star or evening star because it is visible near sunrise and sunset. It is covered by thick clouds of sulfuric acid that strongly reflect sunlight.
Jupiter is the largest planet in the solar system, with a radius of about 69,900 kilometers and a surface area of roughly 61 billion square kilometers.
Mercury is the smallest planet, with a radius of about 2,440 kilometers and a surface area of about 75 million square kilometers.
There are five officially recognized dwarf planets in the solar system: Ceres, Pluto, Haumea, Makemake, and Eris. These bodies orbit the Sun but do not clear their orbital paths of other debris.
Neptune has the fastest winds in the solar system, reaching speeds of over 2,000 kilometers per hour, and its massive storms can be large enough to rival the size of Earth.
The Sun contains about 99.86% of the total mass of the entire solar system.
The asteroid belt between Mars and Jupiter is not empty space; it contains millions of rocky bodies, including the dwarf planet Ceres.
Saturn’s density is so low that it would float in water if a bathtub large enough could exist.
Mars has the largest volcano in the solar system, Olympus Mons, which is about three times taller than Mount Everest.
Jupiter’s Great Red Spot is a giant storm that has been raging for at least 300 years.
Uranus rotates on its side, with an axial tilt of about 98 degrees, causing extreme seasonal changes.
Neptune was the first planet discovered by mathematical prediction before it was observed through a telescope.
The Kuiper Belt is a region beyond Neptune filled with icy bodies and is the source of many comets.
The Oort Cloud is a distant, spherical shell of icy objects thought to surround the solar system and may extend up to one light-year away.
Comets develop glowing tails when they approach the Sun because heat causes their ice to turn directly into gas.
The Moon is slowly moving away from Earth at a rate of about 3.8 centimeters per year.
Earth is the only known planet with liquid surface water and confirmed life.
Venus rotates in the opposite direction to most planets, meaning the Sun would rise in the west and set in the east there.
Mercury experiences the greatest temperature range of any planet, from about –180°C at night to over 430°C during the day.
Jupiter’s magnetic field is the strongest of any planet in the solar system.
Saturn’s rings are made mostly of ice particles, ranging in size from grains of sand to mountains.
Mars has seasons similar to Earth because it has a tilted axis.
Solar wind from the Sun creates a vast bubble in space called the heliosphere, which surrounds the entire solar system.
Voyager 1 is the most distant human-made object and has entered interstellar space.
Some moons, such as Europa and Enceladus, are believed to have subsurface oceans beneath their icy crusts.
A star is a massive, luminous sphere of plasma held together by gravity and powered by nuclear fusion in its core. The nearest star to Earth is the Sun. Many other stars are visible to the naked eye at night, but because they are extremely far away, they appear as tiny, fixed points of light in the sky.
The Milky Way galaxy contains an estimated 100 to 400 billion stars, and possibly more.
Under perfectly dark skies with no Moon and no light pollution, a person with excellent eyesight can see about 2,000 to 3,000 stars at one time with the naked eye.
Star color is linked to temperature. Red stars are the coolest, while blue stars are the hottest.
Stars behave approximately like blackbody radiators, meaning they emit light across a range of wavelengths depending on their temperature, though they are not perfect black bodies.
There are no truly green stars because stars emit light across many wavelengths, and green light is mixed with other colors, making stars appear white or slightly tinted.
The surface temperature of the Sun is about 5,800 kelvin (roughly 5,500°C).
The Sun is classified as a yellow dwarf (G-type main-sequence star).
Stars do not actually twinkle. Twinkling is caused by turbulence in Earth’s atmosphere, which bends starlight as it passes through moving air layers.
One of the largest known stars in the Milky Way is Stephenson 2-18, with an estimated diameter of about 2 to 3 billion kilometers, though its exact size is uncertain.
The Sun has a diameter of about 1.39 million kilometers and a radius of about 696,000 kilometers.
UY Scuti is one of the largest known stars, with a radius roughly 1,700 times that of the Sun, meaning it could contain several billion Suns by volume.
One of the smallest known stars is EBLM J0555–57Ab, which is only slightly larger than Saturn and lies near the minimum size required for hydrogen fusion.
Sirius is the brightest star in Earth’s night sky, but it is not the brightest star in the universe.
Astronomers have observed extremely old stars formed less than a billion years after the Big Bang. One such star observed by the Hubble Space Telescope appears as it was about 12.9 billion years ago, making it among the oldest known stars.
In about 5 billion years, the Sun will exhaust the hydrogen fuel in its core and evolve into a red giant before ending its life as a white dwarf.
The nearest star system to Earth after the Sun is Proxima Centauri, about 4.24 light-years away. With current spacecraft technology, a journey there would take tens of thousands of years.
Some neutron stars spin extremely rapidly. The fastest known neutron stars rotate at over 700 times per second.
Stars are born inside vast clouds of gas and dust called nebulae, where gravity pulls material together until nuclear fusion begins.
A star’s lifetime depends mainly on its mass. Massive stars live fast and die young, sometimes in only a few million years, while small stars can live for trillions of years.
Most stars in the universe are red dwarfs, which are smaller and cooler than the Sun but far more numerous.
Binary and multiple star systems are common; many stars exist in pairs or groups, orbiting a shared center of gravity.
When massive stars explode as supernovae, they create and spread heavy elements such as iron, gold, and uranium into space.
All elements heavier than hydrogen and helium in your body were formed inside stars or during supernova explosions.
White dwarf stars are so dense that one teaspoon of their material would weigh several tons on Earth.
Neutron stars are even denser; a sugar-cube-sized piece of neutron star matter would weigh billions of tons.
Some stars vary in brightness over time and are called variable stars. Their changes help astronomers measure distances in space.
Stars move through space at high speeds, but because of their vast distances, their motion is usually not noticeable to the human eye.
The energy released by the Sun every second comes from converting about 4 million tons of mass into energy, according to Einstein’s equation E = mc².
Brown dwarfs are objects too small to sustain hydrogen fusion and are sometimes called failed stars.
The light we see from distant stars is actually light from the past, because it takes years, centuries, or millennia to reach Earth.
Some stars are surrounded by disks of gas and dust called protoplanetary disks, where planets can form.
The brightest stars in the sky are not always the biggest; many appear bright simply because they are close to Earth.
Stars can form clusters containing thousands to millions of stars, held together by gravity.
There are stars with powerful magnetic fields that produce intense bursts of radiation known as magnetars.
The Sun completes one orbit around the center of the Milky Way in about 225–250 million years, a period called a galactic year.
According to International Astronomical Union, a planet has three qualities or must to three things: i) Must Orbit a Star, ii) Must be large enough to have gravity that forces into spherical shape, iii) Must be large enough to clear its orbit as it revolves around its star.
Planets are formed by pieces of rock and ice that travel through the galaxy until they become entangled in the gravitational pull of a sun.
Kepler 22b, discovered in the Kepler 22 system in 2011, was deemed habitable, similar to Earth 2.0. However, at 600 light-years away, it remains unclear whether this exoplanet can support life.
ROXs 42Bb, the largest planet in the universe, is thought to have a radius up to 2.5 times that of Jupiter.
Jupiter has a radius of 43,441 miles, which equals 1 RJ .
HD 100546 b, a celestial body with a radius of 6.9RJ, is an exoplanet. However, the mass of this planet and other factors appear to indicate that it is a brown dwarf.
A brown dwarf is a type of object that exists between a planet and a star.
Jupiter has a mass that is approximately 317 times that of Earth.
We've been exploring space for over 60 years and have captured close-up images of dozens of celestial objects. We've sent spacecraft to all of our solar system's planets, including Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune, as well as two dwarf planets, Pluto and Ceres.
On Venus, it snows metal and rains acid.
On Mars, the sunset is blue.
There is no atmosphere on Mercury. Mercury is not the hottest planet, despite being closest to the sun, because it has no weather or wind.
Neptune emits more heat than it receives from the sun.
Uranus is the only planet in the solar system that spins on its axis sideways. According to scientists, a collision realigned its orientation.
Mars' largest volcano is three times the size of Mount Everest.
Jupiter is the solar system's garbage dump. Jupiter attracts the majority of the solar system's asteroids. Many potentially hazardous asteroids are sucked up by Jupiter's gravity field.
Saturn is the Milky Way's second-largest and lightest planet. Because it is mostly gas, its low density causes it to float in water.
Mercury is our solar system's fastest planet. It travels at a speed of 65,000 kilometers per hour (40,000 miles per hour) faster than Earth. A year on Mercury lasts only 88 days.
On Mars, a day lasts 24 hours, 39 minutes, and 35 seconds. Mars orbits the sun slower than Earth, so one Martian year has 687 Earth days.
One day on Venus is equivalent to 243 Earth days. One orbit of Venus around the sun takes only 225 Earth days, implying that one day on Venus is 18 Earth days longer.
Mars has the world's longest valley. The Valles Marineris is nearly the length of the United States. It is 4,000 kilometers long, which is more than ten times the length of the Grand Canyon.
A planet made of diamonds twice the size of Earth exists. 55 Cancri e is a so-called "super-Earth" made of diamonds discovered in 2004 in the Milky Way around a nearby star.
In 2013, Mercury was completely mapped. In 2013, the Messenger finished mapping Mercury's surface.
Our solar system contains 181 moons. Both Jupiter and Saturn currently have 53 confirmed moons.
Every year, the moon moves 4 cm away from Earth.
The Earth is 81 times heavier than the moon.
The Moon is roughly 27% the size of Earth.
The moon used to be a part of the Earth.
One moon orbits Neptune in reverse. Triton orbits Neptune in reverse, making it the only large moon in the solar system to do so.
Io, Jupiter's moon, is the most active moon in the solar system, with hundreds of volcanoes. It emits plumes that can travel up to 250 miles into the atmosphere.
The craters on the moon may be the coldest places in the solar system. The temperatures in the moon's craters in the southern hemisphere never rise above -238°C.
Saturn has a moon in the shape of a UFO. Pan is another oddly shaped celestial body in space. The sweeping up of ring material from the Encke gap gives it a walnut-like appearance.
Our Solar System contains 552,894 asteroids and 3,083 comets.
Halley's Comet will not be visible again until 2061. Edmond Halley's 1705 discovery was last seen in 1986. This comet appears only once every 75 to 76 years.
In 240 B.C., the Chinese began to record Halley's Comet. Following its discovery in 240 B.C., Chinese astronomers began to record its passage after 164 B.C.
An asteroid the size of a car enters Earth's atmosphere about once a year. Fortunately, it burns up in the atmosphere before it reaches us.
The largest asteroid in the solar system has a diameter of 329 miles. Vesta is 25 times the size of Manhattan.
Scientists believe that celestial phenomena will destroy the Earth within the next billion years.
The universe is composed of approximately 68% dark energy, 27% dark matter, and 5% ordinary matter.
A modern spacecraft would take 450 million years to reach the centre of our galaxy.
The sun accounts for more than 99% of the mass in our galaxy.
At 75 mph, driving around one of Saturn's rings would take 258 Earth days.
Saturn's rings are made of ice and rock and range in size from 175,000 miles long to 3,200 feet thick.
A radio signal from 5 billion light-years away was detected in space by scientists.
The Earth did not exist at the time the source transmitted it because it was 5 billion light-years away!
The first soft drink consumed in space was Coca-Cola.
Sputnik was the first artificial satellite to orbit the Earth. The Soviet Union launched it with a single shot on October 4, 1957.
The astronaut stool must be returned to Earth via spacecraft.
The gravitational pull of a planet is used by scientists to calculate its weight.
If two pieces of the same metal come into contact in space, they will permanently bond. Due to the absence of water and air molecules in space, two pieces of the same metal will merge during the cold welding process.
Astronomers discovered a massive water vapour cloud about 10 billion light-years away that contains 140 trillion times the mass of water in the Earth's oceans.
The International Space Station (ISS) is valued at one billion dollars. It is also the largest manned spacecraft ever launched.
The International Space Station recycles 93% of the liquids it receives. Recycling takes 8 days, and a lengthy purification process makes it cleaner than the water people drink at home.
It takes 45 minutes to put on a spacesuit. This lengthy procedure will ensure the astronaut's maximum safety, and any mistakes could be fatal.
A typical NASA spacesuit costs $12 million. In 2017, NASA faced a suit shortage. Only 11 suits are currently in use, with others constructed years ago.
In space, your face would puff up. Our bodily fluids are redistributed in space, resulting in "shrinking" legs and a "puffy" face.
There are 88 known constellations. These star patterns can be seen from both the southern and northern hemispheres.
In space, you can't use a regular pen. Normal pens use gravity to draw ink to the nib, allowing you to write. Astronauts and scientists, on the other hand, must use a zero-gravity pen.
The universe contains more stars than grains of sand on Earth.
Diamonds are raining down on Jupiter and Saturn. Both Jupiter and Saturn have high levels of methane in their atmospheres, which results in diamond hailstones. Lightning storms convert methane to soot (carbon), which hardens into graphite chunks and, eventually, diamond.
Mars currently has six spacecraft. Mars' only known inhabitants are space rovers and spacecraft.
Between Earth and the moon, all of the planets in the solar system could fit.
When exposed to space, you could double your size.
The first photographed black hole is 3 million times the size of the Earth. It was first photographed in April of this year.
Being in space is comparable to catching a cold. Different space conditions would congest your nose and impair your sense of taste.
Astronauts will gain 2 inches in space. The absence of gravity causes the discs between the vertebrae to expand, resulting in a slight increase in height. When astronauts return to Earth, gravity compresses their spine and returns them to their normal height.