The Wizard Nebula (NGC 7380) is a young open cluster of stars in the Cepheus constellation. Caroline Herschel discovered the nebula in 1787. The nebula spans 25 arcminutes and measures 100 light-years across. Stars within NGC 7380 are 2-4 million years old. The nebula lies 7,000 light-years from Earth and forms new stars. NGC 7380…
The Trifid Nebula, cataloged as Messier 20 and NGC 6514, is a star-forming region within the Milky Way galaxy. It lies 9,000 light-years from Earth in the constellation Sagittarius. The nebula spans 40 light-years in diameter and is estimated to be 300,000 years old. The nebula’s three-lobed appearance is created by obscuring dust bands that…
The Pelican Nebula (IC 5070) is an H II region associated with the North America Nebula in the Cygnus constellation. The Pelican Nebula spans 30 light-years and is located 1,800 light-years from Earth. The nebula’s contortions resemble a pelican, giving rise to its name. Radiation from stars ionizes surrounding gas, creating an emission nebula. Star…
The Pacman Nebula (NGC 281) is an emission nebula located 9,500 light-years in the constellation Cassiopeia. It spans a radius of 48 light-years and resembles a mouth with a Pacman-like shape. NGC 281 consists of vast interstellar clouds of gas and dust illuminated by stars at its center, including the cluster IC 1590. The nebula’s…
The Cat’s Eye Nebula (NGC 6543) is a planetary nebula located in the constellation Draco, 3,000 light-years from Earth. William Herschel discovered the nebula on February 15, 1786. The nebula measures 0.65 light-years in diameter and consists of shells, filaments, and knots formed by a dying star shedding its outer layers. The nebula’s star has…
The Veil Nebula (NGC 6992) is a supernova remnant in the Cygnus constellation. The nebula formed from a star’s explosion 8,000 years ago and spans 3 by 2 degrees of sky. The nebula is expanding at 100 km/s (62 miles/s) and contains 100 solar masses of ionized gas and dust. Located 2,100 light-years from Earth,…
The Lagoon Nebula, known as Messier 8, is a giant interstellar cloud located in the constellation Sagittarius. It spans 110 light-years across and 50 light-years wide and contains 2,000 solar masses. Giovanni Hodierna discovered the nebula in 1654, and Charles Messier cataloged it as M8 in 1764. The Lagoon Nebula features dust lanes and is…
The Heart Nebula (IC 1805) is an emission nebula located 7,500 light-years away in the Perseus arm of the Milky Way galaxy. William Herschel discovered the Heart nebula on November 3, 1787. The nebula spans 150 light-years in diameter and displays glowing ionized hydrogen gas in the constellation Cassiopeia. Its shape resembles a heart, measuring…
The Crab Nebula is a supernova remnant located in the constellation Taurus. The nebula formed from a star explosion observed in 1054 AD and exemplifies a pulsar wind nebula. William Parsons named it in 1842 due to its crab-like appearance. The nebula measures 10 light-years in diameter and expands at a rate of 1,500 kilometers…
The Carina Nebula is a star-forming region located in the southern constellation Carina. NGC 3372 spans over 300 light-years across and contains a keel-shaped cloud of gas and dust. Stellar winds and radiation sculpt the surrounding interstellar medium, creating an environment for star birth and death. Dust particles in the nebula consist of carbon, silicates,…
The Horsehead Nebula is a dark cloud in the Orion constellation. It appears as a feature against IC 434 and functions as a nursery for young stars. The nebula lies 1,500 light-years away from Earth and measures 3.5 light-years across. It is part of the Orion Molecular Cloud Complex, a star-forming region. The Horsehead Nebula…
The Helix Nebula is a planetary nebula located 650 light-years away in the constellation Aquarius. It consists of a star’s shell resembling a doughnut shape, glowing due to intense radiation from the central star. The nebula formed around 10,000 years ago when a Sun star exhausted its fuel and shed its outer layers. A hot…
The Eagle Nebula is a young open cluster of stars in the constellation Serpens, discovered by Jean-Philippe Loys de Cheseaux in 1745-1746. The Eagle Nebula measures 70 light-years across and 55 light-years long, covering an area of 50 square degrees in the night sky. The nebula contains thousands of forming stars, including the “Pillars of…
Asteroids are small, rocky objects orbiting the Sun, primarily found in the asteroid belt between Mars and Jupiter. The asteroid belt contains over 1 million asteroids, with an estimated 1.1-1.9 million larger than 1 km (0.6 miles) in diameter. Asteroid sizes range from tiny 4-meter boulders to massive bodies like Ceres, measuring 946 kilometers (588…
Kepler-452b is a potentially habitable exoplanet discovered in 2015. The planet orbits a Sun-like star every 385 days within its habitable zone. Kepler-452b measures 60% larger than Earth and could potentially support liquid water on its surface. The exoplanet is located approximately 1,400 light-years away from Earth. This distance translates to roughly 8.4 quadrillion miles…
Ceres is a dwarf planet located in the main asteroid belt between Mars and Jupiter. Giuseppe Piazzi discovered Ceres on January 1, 1801, at the Palermo Astronomical Observatory in Sicily. Ceres has a diameter of 946 km and orbits the Sun at 413 million kilometers. Ceres was initially classified as a planet, then an asteroid,…
Makemake is a dwarf planet located in the Kuiper Belt beyond Neptune’s orbit. It ranks as the third largest dwarf planet in the solar system with a diameter of 1,430 kilometers. Makemake’s surface consists primarily of methane and ethane ices, giving it a reflective and reddish appearance. The dwarf planet was discovered on March 31,…
Mimas is Saturn’s 20th largest moon, orbiting at 185,520 km from the planet. It measures 486.3 km in diameter and consists primarily of water ice and organic material. Mimas features a prominent Herschel crater and potentially harbors a subsurface ocean. William Herschel discovered Mimas in 1781, and it has been studied by Voyager 1, 2,…
Natural satellites are celestial bodies orbiting larger astronomical objects in space. Planets, dwarf planets, and smaller bodies can have natural satellites, commonly referred to as moons. Earth’s Moon orbits at an average distance of 384,400 kilometers from our planet. Jupiter has 79 known natural satellites, while Mercury has none. Saturn holds the record for the…
Meteors are streaks of light in the sky caused by space rocks entering Earth’s atmosphere. Space rocks heat up and burn due to friction with air molecules at speeds of 11 to 72 kilometers per second. Meteor showers occur when Earth passes through debris trails left by comets or asteroids. The Perseid meteor shower in…
Comets are small, icy celestial bodies orbiting the Sun in highly eccentric paths. These “dirty snowballs” consist primarily of dust and frozen gases like water, methane, and ammonia. Comet diameters range from a few to tens of kilometers. The Sun’s radiation causes a comet’s ices to vaporize as it approaches, creating a bright tail visible…
The asteroid belt is a torus-shaped region of space between Mars and Jupiter. It spans approximately 140 million miles (225 million kilometers) in our solar system. The belt contains millions of asteroids and minor planets, ranging from small boulders to objects hundreds of miles across. The main asteroid belt measures about 100 million miles (160…
The Oort Cloud is a theoretical spherical distribution of icy bodies surrounding our solar system. It contains trillions of objects ranging from small boulders to large planetesimals. Jan Oort proposed this concept in 1950 to explain the origins of long-period comets. The Oort Cloud is located in the outermost region of the solar system, extending…
Nebulae are vast interstellar clouds of gas and dust spanning tens of light-years in space. These cosmic structures consist primarily of hydrogen and helium, with traces of heavier elements and dust particles. Nebulae play a crucial role as stellar nurseries, forming new stars through gravitational collapse of dense regions. Powerful telescopes allow astronomers to study…
Haumea is a dwarf planet located in the Kuiper Belt beyond Neptune’s orbit. It was discovered in 2004 by a team led by Mike Brown at Caltech’s Palomar Observatory. Haumea measures 1,960 km in length and has two known moons, Namaka and Hi’iaka. Its rotation causes an elongated shape, completing one rotation every 3.9 hours….
Quaoar is a dwarf planet candidate located in the Kuiper Belt beyond Neptune. American astronomers Chad Trujillo and Michael Brown discovered Quaoar on June 4, 2002, at the Palomar Observatory. Quaoar has a diameter of approximately 1,090 kilometers (680 miles), making it one of the largest known Kuiper Belt objects. Quaoar’s surface contains crystalline water…
Phobos is one of Mars’ two natural satellites, discovered by American astronomer Asaph Hall in 1877. The moon measures approximately 22 kilometers in diameter and is believed to be a captured asteroid composed of carbonaceous chondrite material. Phobos orbits Mars at a distance of 6,000 kilometers above the planet’s surface, closer than any other moon…
Deimos is one of Mars’ two moons, discovered by American astronomer Asaph Hall in 1877. The smaller outer moon orbits Mars every 30 hours, 11 minutes, and 9 seconds at a distance of 20,000 kilometers. Deimos has a diameter of 12 kilometers and is named after Ares’ son in Greek mythology. Deimos orbits Mars at…
Quasars are exceptionally luminous active galactic nuclei powered by supermassive black holes at galaxy cores. They emit massive amounts of electromagnetic radiation across the spectrum, outshining entire galaxies. Quasar light is visible from billions of light-years away, offering insights into early universe formation and black hole evolution. Most observed quasars have redshifts greater than 1,…
The Kuiper Belt is a circumstellar disc in the outer solar system, extending from Neptune’s orbit at 30 astronomical units (AU) to approximately 50 AU from the Sun. It contains numerous small, icy bodies and dwarf planets, including Pluto, Eris, Haumea, and Makemake. Kuiper Belt objects are primarily composed of frozen volatiles such as water,…
Exoplanets are planets orbiting stars outside our solar system. Astronomers discovered the first confirmed exoplanet in 1992. Thousands of exoplanets have been found since, ranging from rocky terrestrial worlds to massive gas giants. Some exoplanets exist in habitable zones of stars, potentially providing conditions suitable for life as we know it. Trillions of exoplanets are…
Dwarf planets are small celestial objects orbiting the Sun that meet specific criteria. The International Astronomical Union (IAU) defines dwarf planets as bodies that orbit the Sun, have sufficient mass for hydrostatic equilibrium, and fail to clear their orbital neighborhoods. Five officially recognized dwarf planets exist in our solar system: Ceres, Pluto, Haumea, Makemake, and…
TON 618 is a hyperluminous quasar located near the border of Canes Venatici and Coma Berenices constellations. Its comoving distance from Earth is 3.2 billion parsecs. TON 618’s luminosity is 40 billion times greater than the Sun’s. The supermassive black hole powering TON 618 has an estimated mass of 6.6 billion solar masses. TON 618’s…
J1407b is a massive exoplanet or brown dwarf located 430 light-years from Earth. J1407b orbits a young, sun-like star called J1407 in the constellation Scorpius. J1407b’s mass is estimated to be 10-40 times that of Jupiter. J1407b possesses an enormous ring system measuring approximately 90 million km in radius. The rings appear 200 times larger…
The Milky Way is a large barred spiral galaxy containing 200-400 billion stars. It spans approximately 100,000 light-years in diameter. Observers on Earth see it as a bright, hazy band of light across the night sky. The galaxy’s center is located 26,000 light-years away from Earth in the direction of the constellation Sagittarius. A supermassive…
A solar system is a collection of celestial bodies orbiting a central star. Our solar system contains eight planets, five dwarf planets, over 190 known moons, and numerous smaller objects. The Sun contains 99.8% of the solar system’s total mass. Solar system objects include planets, dwarf planets, moons, asteroids, comets, and Kuiper belt objects. Our…
Zeta Reticuli is a binary star system located 39.5 light-years from Earth. The system resides in the Reticulum constellation and consists of two Sun-like G-type stars, Zeta-1 and Zeta-2 Reticuli. Zeta Reticuli is visible to the naked eye from Earth’s southern hemisphere, appearing as a double star. Astrobiologists study the system for potential life-supporting planets…
Betelgeuse is a massive red supergiant star in the Orion constellation. It occupies the hunter’s shoulder position and is visible to the naked eye in the night sky. Betelgeuse ranks as the 10th brightest star, with its brightness fluctuating in a semi-regular pattern. Its diameter measures 700-900 times larger than our Sun, extending past Mars’…
UY Scuti is a red supergiant star in the constellation Scutum. It lies 9,500 light-years from Earth and has a radius 1,708-2,100 times that of the Sun. UY Scuti’s brightness fluctuates between magnitude 8.9 and 10.5, classifying it as a pulsating variable star. The star has a cool surface temperature of 3,300 Kelvin, giving it…
T Coronae Borealis is a recurrent nova located 3,000 light-years away in the Corona Borealis constellation. The binary star system consists of a white dwarf and a red giant companion, orbiting each other every 227.5 days. T Coronae Borealis experiences periodic explosive eruptions every 80-100 years, causing a 10,000-fold increase in luminosity. Astronomers predict T…