The Andromeda Galaxy, known as M31, is the nearest spiral galaxy to our Milky Way. The Andromeda Galaxy contains billions of stars and spans a distance across space. Andromeda Galaxy presents information about its composition, structure, and future collision course with our own galaxy. Learn to observe Andromeda Galaxy through telescopes or binoculars to witness…
The Triangulum Galaxy, known as Messier 33 or M33, is a spiral galaxy located in the constellation Triangulum. Triangulum Galaxy is the third-largest member of the Local Group of galaxies, which includes the Milky Way and Andromeda. The Triangulum Galaxy is characterized by its size, position within the Triangulum constellation, abundance of stars, and distance…
The Sunflower Galaxy, known as Messier 63 or M63, is a spiral galaxy located in the constellation Canes Venatici. Sunflower Galaxy is classified as a type of spiral galaxy with characteristics. Sunflower Galaxy resides at a location in the night sky, observable from Earth under conditions. Learn about Sunflower Galaxy’s structure, size, distance from Earth,…
A barred spiral galaxy is a distinct type of spiral galaxy characterized by a central bar-shaped structure composed of stars. Barred spiral galaxies possess features including their overall structure, the prominent central bar, and characteristics that set them apart from other galaxy types. These galaxies exhibit facts related to their formation, evolution, and distribution in…
The Black Eye Galaxy, known as M64, is a distinctive spiral galaxy located in the constellation Coma Berenices. M64 gained its nickname due to a prominent dark band of absorbing dust in front of its nucleus, creating the appearance of a black eye. The Black Eye Galaxy was discovered in the 18th century by astronomer…
The Alcyoneus Galaxy is a radio galaxy located in the constellation Lynx. Astronomers have identified Alcyoneus Galaxy’s type, location, and details of its discovery. Alcyoneus Galaxy holds the record for being the largest known galaxy in the universe. Learn about Alcyoneus Galaxy’s size, unique structure, and the radio emissions it produces. Alcyoneus Galaxy challenges our…
The Whirlpool Galaxy, known as M51, is a design spiral galaxy located in the constellation Canes Venatici. The Whirlpool Galaxy features a striking spiral structure, an active galactic nucleus, and a companion galaxy. Learn about Whirlpool Galaxy’s facts, including its size, distance from Earth, and characteristics. Whirlpool Galaxy’s center harbors a supermassive black hole, which…
The Tadpole Galaxy is a distinctive spiral galaxy located in the constellation Draco. Tadpole Galaxy features a tail structure extending from its main body. The Tadpole Galaxy’s shape results from a gravitational interaction with another galaxy. Learn about Tadpole Galaxy’s location coordinates, distance from Earth, and its position to other celestial objects in the Draco…
The Cartwheel Galaxy is a ring-shaped galaxy located in the constellation Sculptor. Cartwheel Galaxy’s appearance resulted from a collision with another galaxy. Astronomers classify Cartwheel Galaxy as a lenticular galaxy due to its disk structure and lack of spiral arms. Cartwheel Galaxy’s discovery occurred through astronomical observations and has since interested researchers with its form….
The Sombrero Galaxy, known as M104, is a distinctive spiral galaxy located in the constellation Virgo. Sombrero Galaxy’s appearance is characterized by its bright central bulge and dust lane. Sombrero Galaxy’s location in the night sky makes it a target for amateur astronomers and researchers. Learn about Sombrero Galaxy’s distance from Earth, its size, and…
A spiral galaxy is a type of galaxy characterized by its distinctive spiral arm structure. Spiral galaxies consist of a rotating disk containing stars, gas, and dust, with a central bulge or bar. The spiral arms of these galaxies extend outward from the center, creating a pattern visible across vast cosmic distances. Spiral galaxies are…
The Pinwheel Galaxy, known as Messier 101 or NGC 5457, is a design spiral galaxy located in the constellation Ursa Major. Pinwheel Galaxy spans 170,000 light-years in diameter and shines with a magnitude of 7.9. Pinwheel Galaxy gained attention in 2011 when astronomers observed a Type Ia supernova within its spiral arms, providing data for…
A peculiar galaxy is a celestial object with an unusual or distorted shape that deviates from typical galaxy classifications. Peculiar galaxies exhibit morphologies resulting from gravitational interactions, mergers, or collisions with other galaxies. The characteristics of peculiar galaxies include irregular structures, tidal tails, and disrupted stellar distributions. Learn and explore the facts, examples, and defining…
It contains 1 trillion stars and spans 120,000 light-years in diameter. A supermassive black hole resides at its center, weighing 6.5 billion solar masses. It lacks spiral arms and has a rounded appearance. M87 houses over 12,000 globular star clusters, compared to the Milky Way’s 150-200 clusters. The galaxy is located in the constellation Virgo,…
Lenticular galaxies are a unique type of galaxy classified as S0 in the Hubble system. They exhibit properties of both spiral and elliptical galaxies, possessing a central bulge like ellipticals and a disk like spirals but lacking spiral arms. Lenticular galaxies consist mainly of aging stars with little ongoing star formation. They retain some dust…
The Cigar Galaxy, known as Messier 82 (M82), is a starburst galaxy located in the constellation Ursa Major. M82 belongs to the M81 galaxy group and has a D₂₅ diameter of 37 kiloparsecs. Starburst activity in M82 creates thousands of new stars, triggered by a collision with neighboring galaxy M81. M82 is classified as a…
Irregular galaxies lack symmetrical shapes or patterns, exhibiting chaotic appearances with patches of dust and gas. These galaxies differ from spiral galaxies in structure and range in size from thousands to billions of light-years across. The Large Magellanic Cloud measures 14,000 light-years, while the Small Magellanic Cloud spans 7,000 light-years. Astronomers classify irregular galaxies as…
Elliptical galaxies are oval-shaped objects with featureless appearances. Hubble’s classification system categorizes them from E0 (circular) to E7 (elongated). These galaxies contain stars, including red giants, and gas or dust. Elliptical galaxies exhibit low star formation, extensive dark matter, and range from 1,000 to 100,000 light-years in diameter. The shape is characterized by three axes:…
Galaxy clusters are the largest known structures in the universe, held together by gravity. These groupings contain hundreds to thousands of galaxies spanning millions of light-years. Cluster masses range from 10^14 to 10^15 solar masses, with dark matter comprising 85% of the total mass. Galaxy clusters form through the merging of galaxy groups, driven by…
HD1 is a proposed galaxy considered one of the earliest and distant known in the universe. Scientists discovered HD1 using the Subaru Telescope and ALMA. HD1 is classified as a starburst galaxy with an increased rate of star formation. Researchers discovered HD1 in 2022. The star formation rate in HD1 is estimated at 100 stars…
The Elephant Trunk Nebula (IC 1396) is a concentration of interstellar gas and dust within the IC 1396 emission nebula complex. It is located 2,400 light-years from Earth in the Cepheus constellation. The nebula spans 20 light-years in length and 2 light-years in width. Its elephant trunk shape is formed by dense gas and dust…
The North America Nebula (NGC 7000) is a glowing cloud of interstellar gas and dust located 1,800 light-years away in the constellation Cygnus. Hot, young stars within the nebula ionize the surrounding gas through intense radiation. The nebula’s shape resembles the North American continent, with outlines resembling the Gulf of Mexico and eastern U.S. coast….
The Jellyfish Nebula (IC 443) is a supernova remnant located in the constellation Gemini. It spans 70 light-years and lies 5,000 light-years from Earth. William Herschel discovered this 8,000-year nebula in 1784. The nebula’s shape resembles a jellyfish, with a bright central region and tendrils. Its structure formed from the interaction between the supernova’s shockwave…
The Iris Nebula (NGC 7023) is a reflection nebula located 1,300 light-years from Earth. A massive star illuminates the interstellar cloud, creating a glow resembling an eye’s iris. NGC 7023 spans 6 light-years across and contains a density of gas and dust contributing to star formation processes. William Herschel discovered the Iris Nebula on October…
The Flame Nebula (NGC 2024) is an emission nebula located 1,350 light-years from Earth in the constellation Orion. William Herschel first observed it in 1786. The nebula exhibits a flame shape characterized by dark dust lanes creating a pattern. Alnitak’s energetic ultraviolet light causes the Flame Nebula to shine. The nebula spans 6 light-years across…
The Tarantula Nebula (NGC 2070) is a massive H II region located in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. It spans 1,000 light-years in diameter and forms a corner of the Large Magellanic Cloud in the constellation Doradus. Star formation occurs at a rate 10 times higher than in the…
NGC 6302, known as the Butterfly Nebula, is a spectacular bipolar planetary nebula in the constellation Scorpius. The nebula’s butterfly structure is formed by ejected material from a dying star. NGC 6302 is located 3,800 light-years from Earth and estimated to be 2,000 years old. Its wings extend 3 light-years from the star and consist…
The Boomerang Nebula is a celestial object located in the Centaurus constellation, 5,000 light-years from Earth. It was discovered in 1980 and holds the title of coldest known place in the Universe at -272°C. The nebula’s structure features a distinctive bipolar outflow of gas and dust from a dying star, creating an hourglass or bow-tie…
The Bubble Nebula (NGC 7635) is an emission nebula located 7,100 light-years in the constellation Cassiopeia. Its bubble structure is shaped by intense radiation from a massive young star. Hubble Space Telescope captured images of the nebula, revealing its composition and details. The nebula’s gas reaches temperatures of 10,000 Kelvin and emits light across visible,…
The Rosette Nebula is an H II region located in the Monoceros constellation of the Milky Way galaxy. It spans 130 light-years across and extends 1.3 degrees in the sky. The nebula is associated with the open cluster NGC 2244, which formed from its matter. Rosette Nebula emits light at wavelengths due to its ionized…
Ring nebulae are planetary nebulae formed when stars exhaust their fuel in final evolutionary stages. Stars expel their outer layers, creating ring structures ionized by hot central white dwarfs. The Ring Nebula (M57) in the constellation Lyra exemplifies this phenomenon, located 2,300 light-years from Earth. M57 measures 1 light-year across and is expanding at 20-30…
Reflection nebulae are clouds of gas and dust in space illuminated by nearby stars. Stars cause these nebulae to shine by reflecting starlight. Reflection nebulae appear blue due to the scattering of blue light by dust particles measuring 0.01-1 micrometers in size. The dust in reflection nebulae consists of silicates, graphites, and minerals. Reflection nebulae…
Planetary nebulae are emission nebulae created when low-mass stars exhaust their fuel and shed outer layers into space. The core of the dying star illuminates a gas shell composed of hydrogen and helium, spanning tens of light-years. 1,500 known planetary nebulae exist in the Milky Way galaxy. The planetary nebula stage lasts 10,000 to 50,000…
The Orion Nebula is a stellar nursery located 1,300 light-years from Earth in the constellation Orion. It spans 24 light-years across and serves as a region of star formation close to our solar system. The nebula’s heart contains the Trapezium cluster, whose ultraviolet radiation illuminates the surrounding gas. Astronomers classify it as Messier 42 and…
The Dumbbell Nebula (Messier 27) is a planetary nebula located 1,200 light-years from Earth in the constellation Vulpecula. Charles Messier discovered the Dumbbell Nebula in 1764 as the first planetary nebula. The nebula consists of a glowing gas shell surrounding a white dwarf star at its center. The dwarf has a surface temperature of 85,000…
The Crescent Nebula (NGC 6888) is an emission nebula located 4,700 light-years from Earth in the constellation Cygnus. William Herschel discovered the nebula in 1792. The nebula spans 25 light-years across and is shaped by strong stellar winds from a massive central star. The nebula’s crescent shape results from the interaction between stellar winds and…
The California Nebula (NGC 1499) is an emission nebula located in the constellation Perseus. It resides 1,500 light-years from Earth and measures 100 light-years across. The nebula’s nickname comes from its resemblance to the outline of California. Xi Persei’s radiation causes the nebula to glow with a distinctive pinkish-red hue. California Nebula spans 2.5° x…
The Omega Nebula, known as Messier 17, is an H II region located in the Sagittarius constellation. It spans 15 light-years and lies 5,500 light-years from Earth. Philippe Loys de Chéseaux discovered the nebula in 1745, and Charles Messier cataloged it in 1764. The nebula contains ionized hydrogen, helium, and heavier elements, with hot stars…
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…