Dictionary of Space Concepts
The Dictionary of Space Concepts (DSC) provides not only the basis for the advanced English language classes of the Multilingualism Programme; it also serves as larger online support platform for all UNIVERSEH students, with the aim of training specific space terminologies across various fields connected to the space sector. The DSC combines core space concepts and with helpful illustrations, all in an open-project format, which is freely available to everyone inside and outside UNIVERSEH. We welcome your contributions, comments, and expertise!
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Special | A | B | C | D | E | F | G | H | I | J | K | L | M | N | O | P | Q | R | S | T | U | V | W | X | Y | Z | ALL
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Dark energy | |||
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Source: https://astronomy.com/news/2020/03/whats-the-difference-between-dark-matter-and-dark-energy Definition:Dark energy (not to be mistaken with dark matter) makes up approximately 68% of the universe, and it is distributed evenly not only in space, but also in time (therefore it has a global effect on the universe as a whole). This is a repulsive force, that accelerates the expansion of the universe. The rate of expansion and its acceleration can be measured by observations based on the Hubble law. The existence of dark energy is proven and its role in the universe can be described thanks to Albert Einstein’s theory of general relativity. Example Sentence(s):"Dark energy is generally accepted as contributing to the increased acceleration of the expanding universe, so understanding this relationship will help to refine how physicists and astrophysicists understand it." "And there are still no final answers to the questions surrounding dark energy." Translations:
Links to Videos/Articles:https://home.cern/science/physics/dark-matterhttps://astronomy.com/news/2020/03/whats-the-difference-between-dark-matter-and-dark-energy | |||
Dark matter | |||
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Source: https://astronomy.com/news/2020/03/whats-the-difference-between-dark-matter-and-dark-energy Definition:Dark matter (not to be mistaken with dark energy) makes up about 27% of the universe. Unlike normal matter, dark matter does not interact with electromagnetic forces. This means it does not absorb, reflect or emit light, therefore it can't be seen, but researchers can detect it and map it by measuring gravitational lensing. Because of these properties, it works like an attractive force, holding the universe together. In the 1930s, astronomer Fritz Zwicky studied images of around 1,000 galaxies that make up the Coma Cluster and speculated that some kind of matter must be keeping them together. Astronomers Vera Rubin and Kent Ford found a similar phenomenon when they studied the rotation rates of individual galaxies, with even more evidence of the features mentioned above. The existence of dark matter is so widely accepted that it’s part of the "standard model of cosmology", although there is no solid evidence that it is real. There are many theories suggesting that physics beyond the Standard Model, such as supersymmetry and extra dimensions, exist. If other parallel universes exist, then physical features of each universe would be different, therefore the amount of dark matter in each universe would be different. Dark matter helps scientists gain a better understanding of the composition of our universe and how galaxies are held together. Sample Sentence(s):"You can see the galaxy clusters that Professor Zwicky studied to discover Dark Matter." "Dr. Shepherd's work enhances our profile in the area of Dark Matter exploration significantly." Translations:
Links to Videos/Articles:https://home.cern/science/physics/dark-matterhttps://astronomy.com/news/2020/03/whats-the-difference-between-dark-matter-and-dark-energy | |||
DART Mission | |||
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Source: https://dart.jhuapl.edu/Gallery/media/graphics/lg/DART-infographic_v4.jpg Definition:A mission planned by NASA to test a method of planetary defense by redirecting an asteroid, which could hypothetically pose a threat to Earth, by means of the DART spacecraft deliberately crashing itself into this asteroid. The DART spacecraft was built by Johns Hopkins Applied Physics Laboratory and was launched on November 23, 2021 at Vandenberg Space Force Base in California. Its target is the binary near-Earth asteroid Didymos (780 m across) and its secondary body, or “moonlet”, Dimorphos (163 m across). This binary asteroid is situated roughly 11 million kilometers from the Earth and does not pose a threat to the planet, but corresponds to the size of a potentially hazardous celestial body (140 m or more in diameter). As a result of the planned collision at the end of September 2022, the orbit of Dimorphos will change, this change will be observed and measured using telescopes on Earth and the data will be used to predict effectiveness of kinetic impact for the purpose of asteroid deflection as a planetary defense method. (https://blogs.nasa.gov/dart/2021/11/24/nasa-spacex-launch-dart-first-planetary-defense-test-mission/) Etymology:DART stands for “Double Asteroid Redirection Test” Translations:
Links to Videos/Articles:https://www.youtube.com/watch?v=hbL07cZUEMU More detailed information on the project:https://www.nasa.gov/planetarydefense/dart https://dart.jhuapl.edu/ | |||
Dusty Vacuum Chamber (Dirty Vacuum Chamber) | ||
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Source: https://ttu-ir.tdl.org/bitstream/handle/2346/73031/ICES_2017_235.pdf?sequence=2&isAllowed=y Short Definition:An enclosure that constitutes a closed environment developed for the purpose of simulating lunar conditions and allow for the testing of material behaviour in such a space.
Detailed Definition:Sample Sentence(s):Translations:
Links to Videos/Articles: | ||
Dwarf Galaxy | |||
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Picture: Fornax Dwarf Galaxy Image/Video/Audio Source: https://commons.wikimedia.org/wiki/File:Fornax_dwarf_galaxy.jpg Short Definition: A dwarf galaxy is one that contains fewer stars than larger galaxies. A dwarf galaxy is a galaxy made up of material and dark matter ejected from larger galaxies by the force of gravity. Although a dwarf galaxy is defined by astronomers by the number of stars it contains, and hence its size, it is also defined as dwarf by its shape, content, and even appearance. Detailed Definition: Dwarf galaxies, formed from fragments of larger galaxies, are the most abundant type of galaxy in the universe. Dwarf galaxies are galaxies that break apart due to their relatively small size to their neighbors, causing stellar streams and galaxy mergers. However dynamic these relationships with neighboring galaxies may be, they are difficult to detect by astronomers due to their low light, mass and small size. The astronomical importance of these dwarf galaxies actually comes from their tendency to form from other large galaxies and merge again with larger galaxies. Their difference from the usual galaxy shape is that they have low metallicity and gas in abundance. This situation is used by astronomers as evidence to interpret the motion and evolution of galaxies. Dwarf galaxies are basically divided into three groups: Dwarf elliptical galaxies, dwarf spheroidal galaxies, and dwarf irregular galaxies. Etymology: From Old English ‘Dweorg’ + From Latin ‘Galaxias’ Sample Sentence(s): ‘’The most powerful space telescope currently operating has zoomed in on a lonely dwarf galaxy in our galactic neighborhood, imaging it in stunning detail.’’ (Lea, R. (2022, November 11). James Webb Space Telescope peers into lonely dwarf galaxy with sparkling results. Space.com. https://www.space.com/james-webb-space-telescope-wlm-dwarf-galaxy-image) ‘’This Living Collection starts with an introductory Comment and continues with a series of articles on the science of dwarf galaxies, their properties and their theoretical modelling and simulations.’’ (It’s time for some plane speaking. (2021, December 13). Nature. https://www.nature.com/collections/bgegjajcec error=cookies_not_supported&code=03e197b7-7ba4-4db9-a0c7-ee3cf2730af7) Translations of Terms/Concepts into Partner Languages: French: Galaxie Naine German: Zwerggalaxie Polish: Galaktyka karłowata Swedish: DvärggalaxTurkish: Cüce Gökada Links to Videos/Articles: https://esahubble.org/wordbank/dwarf-galaxy/ https://astronomy.swin.edu.au/cosmos/D/dwarf+galaxy https://www.sciencealert.com/webb-is-giving-us-a-stunning-new-look-into-this-lonely-dwarf-galaxy https://esawebb.org/images/WLMb/ https://www.youtube.com/watch?v=hcDrvX6vy0k&ab_channel=EuropeanSouthernObservatory%28ESO%29 https://www.youtube.com/watch?v=gez1RSHQvDE&ab_channel=Engadget | |||
