Faster access than browser!Similarities between Astronomy and Universe
Astronomy and Universe have 81 things in common (in Unionpedia): Abu Maʿshar, Age of the universe, Ancient Greece, Ancient Greek astronomy, Andromeda Galaxy, Aristarchus of Samos, Astronomy in the medieval Islamic world, Astrophysics, Atom, Babylonian astronomy, Big Bang, Big Bang nucleosynthesis, Chemistry, Chronology of the universe, Comet, Cosmic Background Explorer, Cosmic microwave background, Cosmic ray, Cosmology, Dark energy, Dark matter, Earth, Electromagnetic radiation, Electromagnetic spectrum, Electron, Exoplanet, Expansion of the universe, Galaxy, Galaxy filament, Galaxy groups and clusters, ..., General relativity, Geocentric model, Gravity, Heliocentrism, Helium, Hubble's law, Hydrogen, Indian astronomy, Inflation (cosmology), Interstellar medium, Isaac Newton, Isotope, Jeans instability, Johannes Kepler, Kelvin, Lambda-CDM model, Light, Local Group, Matter, Metallicity, Middle Ages, Milky Way, Moon, Nanometre, Natural satellite, Neutrino, Nicolaus Copernicus, Nuclear fusion, Nucleocosmochronology, Observable universe, Observational astronomy, Open cluster, Photon, Physical cosmology, Physics, Planet, Ptolemy, Quasar, Reionization, Solar System, Star, Stellar parallax, Stellar population, String theory, Sun, Supercluster, The Astrophysical Journal, Ultimate fate of the universe, Void (astronomy), Wave, Wavelength. Expand index (51 more) »
Abu Maʿshar
Abu Maʿshar, Latinized as Albumasar (also Albusar, Albuxar; full name Abū Maʿshar Jaʿfar ibn Muḥammad ibn ʿUmar al-Balkhī أبو معشر جعفر بن محمد بن عمر البلخي; –, AH 171–272), was an early Persian Muslim astrologer, thought to be the greatest astrologer of the Abbasid court in Baghdad.
Abu Maʿshar and Astronomy · Abu Maʿshar and Universe ·
Age of the universe
In physical cosmology, the age of the universe is the time elapsed since the Big Bang.
Age of the universe and Astronomy · Age of the universe and Universe ·
Ancient Greece
Ancient Greece was a civilization belonging to a period of Greek history from the Greek Dark Ages of the 13th–9th centuries BC to the end of antiquity (AD 600).
Ancient Greece and Astronomy · Ancient Greece and Universe ·
Ancient Greek astronomy
Greek astronomy is astronomy written in the Greek language in classical antiquity.
Ancient Greek astronomy and Astronomy · Ancient Greek astronomy and Universe ·
Andromeda Galaxy
The Andromeda Galaxy, also known as Messier 31, M31, or NGC 224, is a spiral galaxy approximately 780 kiloparsecs (2.5 million light-years) from Earth, and the nearest major galaxy to the Milky Way.
Andromeda Galaxy and Astronomy · Andromeda Galaxy and Universe ·
Aristarchus of Samos
Aristarchus of Samos (Ἀρίσταρχος ὁ Σάμιος, Aristarkhos ho Samios; c. 310 – c. 230 BC) was an ancient Greek astronomer and mathematician who presented the first known model that placed the Sun at the center of the known universe with the Earth revolving around it (see Solar system).
Aristarchus of Samos and Astronomy · Aristarchus of Samos and Universe ·
Astronomy in the medieval Islamic world
Islamic astronomy comprises the astronomical developments made in the Islamic world, particularly during the Islamic Golden Age (9th–13th centuries), and mostly written in the Arabic language.
Astronomy and Astronomy in the medieval Islamic world · Astronomy in the medieval Islamic world and Universe ·
Astrophysics
Astrophysics is the branch of astronomy that employs the principles of physics and chemistry "to ascertain the nature of the astronomical objects, rather than their positions or motions in space".
Astronomy and Astrophysics · Astrophysics and Universe ·
Atom
An atom is the smallest constituent unit of ordinary matter that has the properties of a chemical element.
Astronomy and Atom · Atom and Universe ·
Babylonian astronomy
The history of astronomy in Mesopotamia, and the world, begins with the Sumerians who developed the earliest writing system—known as cuneiform—around 3500–3200 BC.
Astronomy and Babylonian astronomy · Babylonian astronomy and Universe ·
Big Bang
The Big Bang theory is the prevailing cosmological model for the universe from the earliest known periods through its subsequent large-scale evolution.
Astronomy and Big Bang · Big Bang and Universe ·
Big Bang nucleosynthesis
In physical cosmology, Big Bang nucleosynthesis (abbreviated BBN, also known as primordial nucleosynthesis, arch(a)eonucleosynthesis, archonucleosynthesis, protonucleosynthesis and pal(a)eonucleosynthesis) refers to the production of nuclei other than those of the lightest isotope of hydrogen (hydrogen-1, 1H, having a single proton as a nucleus) during the early phases of the Universe.
Astronomy and Big Bang nucleosynthesis · Big Bang nucleosynthesis and Universe ·
Chemistry
Chemistry is the scientific discipline involved with compounds composed of atoms, i.e. elements, and molecules, i.e. combinations of atoms: their composition, structure, properties, behavior and the changes they undergo during a reaction with other compounds.
Astronomy and Chemistry · Chemistry and Universe ·
Chronology of the universe
The chronology of the universe describes the history and future of the universe according to Big Bang cosmology.
Astronomy and Chronology of the universe · Chronology of the universe and Universe ·
Comet
A comet is an icy small Solar System body that, when passing close to the Sun, warms and begins to release gases, a process called outgassing.
Astronomy and Comet · Comet and Universe ·
Cosmic Background Explorer
The Cosmic Background Explorer (COBE), also referred to as Explorer 66, was a satellite dedicated to cosmology, which operated from 1989 to 1993.
Astronomy and Cosmic Background Explorer · Cosmic Background Explorer and Universe ·
Cosmic microwave background
The cosmic microwave background (CMB, CMBR) is electromagnetic radiation as a remnant from an early stage of the universe in Big Bang cosmology.
Astronomy and Cosmic microwave background · Cosmic microwave background and Universe ·
Cosmic ray
Cosmic rays are high-energy radiation, mainly originating outside the Solar System and even from distant galaxies.
Astronomy and Cosmic ray · Cosmic ray and Universe ·
Cosmology
Cosmology (from the Greek κόσμος, kosmos "world" and -λογία, -logia "study of") is the study of the origin, evolution, and eventual fate of the universe.
Astronomy and Cosmology · Cosmology and Universe ·
Dark energy
In physical cosmology and astronomy, dark energy is an unknown form of energy which is hypothesized to permeate all of space, tending to accelerate the expansion of the universe.
Astronomy and Dark energy · Dark energy and Universe ·
Dark matter
Dark matter is a theorized form of matter that is thought to account for approximately 80% of the matter in the universe, and about a quarter of its total energy density.
Astronomy and Dark matter · Dark matter and Universe ·
Earth
Earth is the third planet from the Sun and the only astronomical object known to harbor life.
Astronomy and Earth · Earth and Universe ·
Electromagnetic radiation
In physics, electromagnetic radiation (EM radiation or EMR) refers to the waves (or their quanta, photons) of the electromagnetic field, propagating (radiating) through space-time, carrying electromagnetic radiant energy.
Astronomy and Electromagnetic radiation · Electromagnetic radiation and Universe ·
Electromagnetic spectrum
The electromagnetic spectrum is the range of frequencies (the spectrum) of electromagnetic radiation and their respective wavelengths and photon energies.
Astronomy and Electromagnetic spectrum · Electromagnetic spectrum and Universe ·
Electron
The electron is a subatomic particle, symbol or, whose electric charge is negative one elementary charge.
Astronomy and Electron · Electron and Universe ·
Exoplanet
An exoplanet or extrasolar planet is a planet outside our solar system.
Astronomy and Exoplanet · Exoplanet and Universe ·
Expansion of the universe
The expansion of the universe is the increase of the distance between two distant parts of the universe with time.
Astronomy and Expansion of the universe · Expansion of the universe and Universe ·
Galaxy
A galaxy is a gravitationally bound system of stars, stellar remnants, interstellar gas, dust, and dark matter.
Astronomy and Galaxy · Galaxy and Universe ·
Galaxy filament
The distribution reveals fine, filamentary structures.
Astronomy and Galaxy filament · Galaxy filament and Universe ·
Galaxy groups and clusters
Galaxy groups and clusters are the largest known gravitationally bound objects to have arisen thus far in the process of cosmic structure formation.
Astronomy and Galaxy groups and clusters · Galaxy groups and clusters and Universe ·
General relativity
General relativity (GR, also known as the general theory of relativity or GTR) is the geometric theory of gravitation published by Albert Einstein in 1915 and the current description of gravitation in modern physics.
Astronomy and General relativity · General relativity and Universe ·
Geocentric model
In astronomy, the geocentric model (also known as geocentrism, or the Ptolemaic system) is a superseded description of the universe with Earth at the center.
Astronomy and Geocentric model · Geocentric model and Universe ·
Gravity
Gravity, or gravitation, is a natural phenomenon by which all things with mass or energy—including planets, stars, galaxies, and even light—are brought toward (or gravitate toward) one another.
Astronomy and Gravity · Gravity and Universe ·
Heliocentrism
Heliocentrism is the astronomical model in which the Earth and planets revolve around the Sun at the center of the Solar System.
Astronomy and Heliocentrism · Heliocentrism and Universe ·
Helium
Helium (from lit) is a chemical element with symbol He and atomic number 2.
Astronomy and Helium · Helium and Universe ·
Hubble's law
Hubble's law is the name for the observation in physical cosmology that.
Astronomy and Hubble's law · Hubble's law and Universe ·
Hydrogen
Hydrogen is a chemical element with symbol H and atomic number 1.
Astronomy and Hydrogen · Hydrogen and Universe ·
Indian astronomy
Indian astronomy has a long history stretching from pre-historic to modern times.
Astronomy and Indian astronomy · Indian astronomy and Universe ·
Inflation (cosmology)
In physical cosmology, cosmic inflation, cosmological inflation, or just inflation, is a theory of exponential expansion of space in the early universe.
Astronomy and Inflation (cosmology) · Inflation (cosmology) and Universe ·
Interstellar medium
In astronomy, the interstellar medium (ISM) is the matter and radiation that exists in the space between the star systems in a galaxy.
Astronomy and Interstellar medium · Interstellar medium and Universe ·
Isaac Newton
Sir Isaac Newton (25 December 1642 – 20 March 1726/27) was an English mathematician, astronomer, theologian, author and physicist (described in his own day as a "natural philosopher") who is widely recognised as one of the most influential scientists of all time, and a key figure in the scientific revolution.
Astronomy and Isaac Newton · Isaac Newton and Universe ·
Isotope
Isotopes are variants of a particular chemical element which differ in neutron number.
Astronomy and Isotope · Isotope and Universe ·
Jeans instability
In stellar physics, the Jeans instability causes the collapse of interstellar gas clouds and subsequent star formation.
Astronomy and Jeans instability · Jeans instability and Universe ·
Johannes Kepler
Johannes Kepler (December 27, 1571 – November 15, 1630) was a German mathematician, astronomer, and astrologer.
Astronomy and Johannes Kepler · Johannes Kepler and Universe ·
Kelvin
The Kelvin scale is an absolute thermodynamic temperature scale using as its null point absolute zero, the temperature at which all thermal motion ceases in the classical description of thermodynamics.
Astronomy and Kelvin · Kelvin and Universe ·
Lambda-CDM model
The ΛCDM (Lambda cold dark matter) or Lambda-CDM model is a parametrization of the Big Bang cosmological model in which the universe contains a cosmological constant, denoted by Lambda (Greek Λ), associated with dark energy, and cold dark matter (abbreviated CDM).
Astronomy and Lambda-CDM model · Lambda-CDM model and Universe ·
Light
Light is electromagnetic radiation within a certain portion of the electromagnetic spectrum.
Astronomy and Light · Light and Universe ·
Local Group
The Local Group is the galaxy group that includes the Milky Way.
Astronomy and Local Group · Local Group and Universe ·
Matter
In the classical physics observed in everyday life, matter is any substance that has mass and takes up space by having volume.
Astronomy and Matter · Matter and Universe ·
Metallicity
In astronomy, metallicity is used to describe the abundance of elements present in an object that are heavier than hydrogen or helium.
Astronomy and Metallicity · Metallicity and Universe ·
Middle Ages
In the history of Europe, the Middle Ages (or Medieval Period) lasted from the 5th to the 15th century.
Astronomy and Middle Ages · Middle Ages and Universe ·
Milky Way
The Milky Way is the galaxy that contains our Solar System.
Astronomy and Milky Way · Milky Way and Universe ·
Moon
The Moon is an astronomical body that orbits planet Earth and is Earth's only permanent natural satellite.
Astronomy and Moon · Moon and Universe ·
Nanometre
The nanometre (International spelling as used by the International Bureau of Weights and Measures; SI symbol: nm) or nanometer (American spelling) is a unit of length in the metric system, equal to one billionth (short scale) of a metre (m).
Astronomy and Nanometre · Nanometre and Universe ·
Natural satellite
A natural satellite or moon is, in the most common usage, an astronomical body that orbits a planet or minor planet (or sometimes another small Solar System body).
Astronomy and Natural satellite · Natural satellite and Universe ·
Neutrino
A neutrino (denoted by the Greek letter ν) is a fermion (an elementary particle with half-integer spin) that interacts only via the weak subatomic force and gravity.
Astronomy and Neutrino · Neutrino and Universe ·
Nicolaus Copernicus
Nicolaus Copernicus (Mikołaj Kopernik; Nikolaus Kopernikus; Niklas Koppernigk; 19 February 1473 – 24 May 1543) was a Renaissance-era mathematician and astronomer who formulated a model of the universe that placed the Sun rather than the Earth at the center of the universe, likely independently of Aristarchus of Samos, who had formulated such a model some eighteen centuries earlier.
Astronomy and Nicolaus Copernicus · Nicolaus Copernicus and Universe ·
Nuclear fusion
In nuclear physics, nuclear fusion is a reaction in which two or more atomic nuclei come close enough to form one or more different atomic nuclei and subatomic particles (neutrons or protons).
Astronomy and Nuclear fusion · Nuclear fusion and Universe ·
Nucleocosmochronology
Nucleocosmochronology or nuclear cosmochronology is a technique used to determine timescales for astrophysical objects and events.
Astronomy and Nucleocosmochronology · Nucleocosmochronology and Universe ·
Observable universe
The observable universe is a spherical region of the Universe comprising all matter that can be observed from Earth at the present time, because electromagnetic radiation from these objects has had time to reach Earth since the beginning of the cosmological expansion.
Astronomy and Observable universe · Observable universe and Universe ·
Observational astronomy
Observational astronomy is a division of astronomy that is concerned with recording data about the observable universe, in contrast with theoretical astronomy, which is mainly concerned with calculating the measurable implications of physical models.
Astronomy and Observational astronomy · Observational astronomy and Universe ·
Open cluster
An open cluster is a group of up to a few thousand stars that were formed from the same giant molecular cloud and have roughly the same age.
Astronomy and Open cluster · Open cluster and Universe ·
Photon
The photon is a type of elementary particle, the quantum of the electromagnetic field including electromagnetic radiation such as light, and the force carrier for the electromagnetic force (even when static via virtual particles).
Astronomy and Photon · Photon and Universe ·
Physical cosmology
Physical cosmology is the study of the largest-scale structures and dynamics of the Universe and is concerned with fundamental questions about its origin, structure, evolution, and ultimate fate.
Astronomy and Physical cosmology · Physical cosmology and Universe ·
Physics
Physics (from knowledge of nature, from φύσις phýsis "nature") is the natural science that studies matterAt the start of The Feynman Lectures on Physics, Richard Feynman offers the atomic hypothesis as the single most prolific scientific concept: "If, in some cataclysm, all scientific knowledge were to be destroyed one sentence what statement would contain the most information in the fewest words? I believe it is that all things are made up of atoms – little particles that move around in perpetual motion, attracting each other when they are a little distance apart, but repelling upon being squeezed into one another..." and its motion and behavior through space and time and that studies the related entities of energy and force."Physical science is that department of knowledge which relates to the order of nature, or, in other words, to the regular succession of events." Physics is one of the most fundamental scientific disciplines, and its main goal is to understand how the universe behaves."Physics is one of the most fundamental of the sciences. Scientists of all disciplines use the ideas of physics, including chemists who study the structure of molecules, paleontologists who try to reconstruct how dinosaurs walked, and climatologists who study how human activities affect the atmosphere and oceans. Physics is also the foundation of all engineering and technology. No engineer could design a flat-screen TV, an interplanetary spacecraft, or even a better mousetrap without first understanding the basic laws of physics. (...) You will come to see physics as a towering achievement of the human intellect in its quest to understand our world and ourselves."Physics is an experimental science. Physicists observe the phenomena of nature and try to find patterns that relate these phenomena.""Physics is the study of your world and the world and universe around you." Physics is one of the oldest academic disciplines and, through its inclusion of astronomy, perhaps the oldest. Over the last two millennia, physics, chemistry, biology, and certain branches of mathematics were a part of natural philosophy, but during the scientific revolution in the 17th century, these natural sciences emerged as unique research endeavors in their own right. Physics intersects with many interdisciplinary areas of research, such as biophysics and quantum chemistry, and the boundaries of physics are not rigidly defined. New ideas in physics often explain the fundamental mechanisms studied by other sciences and suggest new avenues of research in academic disciplines such as mathematics and philosophy. Advances in physics often enable advances in new technologies. For example, advances in the understanding of electromagnetism and nuclear physics led directly to the development of new products that have dramatically transformed modern-day society, such as television, computers, domestic appliances, and nuclear weapons; advances in thermodynamics led to the development of industrialization; and advances in mechanics inspired the development of calculus.
Astronomy and Physics · Physics and Universe ·
Planet
A planet is an astronomical body orbiting a star or stellar remnant that is massive enough to be rounded by its own gravity, is not massive enough to cause thermonuclear fusion, and has cleared its neighbouring region of planetesimals.
Astronomy and Planet · Planet and Universe ·
Ptolemy
Claudius Ptolemy (Κλαύδιος Πτολεμαῖος, Klaúdios Ptolemaîos; Claudius Ptolemaeus) was a Greco-Roman mathematician, astronomer, geographer, astrologer, and poet of a single epigram in the Greek Anthology.
Astronomy and Ptolemy · Ptolemy and Universe ·
Quasar
A quasar (also known as a QSO or quasi-stellar object) is an extremely luminous active galactic nucleus (AGN).
Astronomy and Quasar · Quasar and Universe ·
Reionization
In the field of Big Bang theory, and cosmology, reionization is the process that caused the matter in the universe to reionize after the lapse of the "dark ages".
Astronomy and Reionization · Reionization and Universe ·
Solar System
The Solar SystemCapitalization of the name varies.
Astronomy and Solar System · Solar System and Universe ·
Star
A star is type of astronomical object consisting of a luminous spheroid of plasma held together by its own gravity.
Astronomy and Star · Star and Universe ·
Stellar parallax
Stellar parallax is the apparent shift of position of any nearby star (or other object) against the background of distant objects.
Astronomy and Stellar parallax · Stellar parallax and Universe ·
Stellar population
During 1944, Walter Baade categorized groups of stars within the Milky Way into bluer stars associated with the spiral arms and the general position of yellow stars near the central galactic bulge or within globular star clusters.
Astronomy and Stellar population · Stellar population and Universe ·
String theory
In physics, string theory is a theoretical framework in which the point-like particles of particle physics are replaced by one-dimensional objects called strings.
Astronomy and String theory · String theory and Universe ·
Sun
The Sun is the star at the center of the Solar System.
Astronomy and Sun · Sun and Universe ·
Supercluster
A supercluster is a large group of smaller galaxy clusters or galaxy groups; it is among the largest-known structures of the cosmos.
Astronomy and Supercluster · Supercluster and Universe ·
The Astrophysical Journal
The Astrophysical Journal, often abbreviated ApJ (pronounced "ap jay") in references and speech, is a peer-reviewed scientific journal of astrophysics and astronomy, established in 1895 by American astronomers George Ellery Hale and James Edward Keeler.
Astronomy and The Astrophysical Journal · The Astrophysical Journal and Universe ·
Ultimate fate of the universe
The ultimate fate of the universe is a topic in physical cosmology, whose theoretical restrictions allow possible scenarios for the evolution and ultimate fate of the universe to be described and evaluated.
Astronomy and Ultimate fate of the universe · Ultimate fate of the universe and Universe ·
Void (astronomy)
Cosmic voids are vast spaces between filaments (the largest-scale structures in the universe), which contain very few or no galaxies.
Astronomy and Void (astronomy) · Universe and Void (astronomy) ·
Wave
In physics, a wave is a disturbance that transfers energy through matter or space, with little or no associated mass transport.
Astronomy and Wave · Universe and Wave ·
Wavelength
In physics, the wavelength is the spatial period of a periodic wave—the distance over which the wave's shape repeats.
The list above answers the following questions
- What Astronomy and Universe have in common
- What are the similarities between Astronomy and Universe
Astronomy and Universe Comparison
Astronomy has 344 relations, while Universe has 479. As they have in common 81, the Jaccard index is 9.84% = 81 / (344 + 479).
References
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