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!
Do you want to take part of developing the Dictionary of Space Concepts? Enrol in the Collaborative Dictionary of Space Concepts.
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
N |
---|
Nebula | |||
---|---|---|---|
Source: Kirk, A. (2015, April 25). The Mighty Orion Nebula from New Zealand. flickr. https://www.flickr.com/photos/67481624@N05/17243621226 Short Definition: Any kind of giant cloud that includes miscellaneous gas and dust; especially hydrogen, cosmic dust, and helium located in outer space. Detailed Definition: As the basic components of galaxies, nebulae were stars before they formed. During the formation phase of these stars, the gases released into space initiate a fusion reaction with hydrogen atoms and form the foundations of a new star. Thus, the universe continues to expand. Etymology: Ancient Greek (νεφέλη - nephélē): Cloud Sample Sentences: 'Today the term nebula generally refers exclusively to the interstellar medium.' 'A nebula that is visible to the human eye from Earth would appear larger, but no brighter, from close by.' Translations of Terms/Concepts into Partner Languages: French: Nébuleuse Italian: Nebulosa German: Nebel Polish: Mgławica Turkish: Nebula Links to Videos/Articles: https://spacecenter.org/what-is-a-nebula/ https://spaceplace.nasa.gov/nebula/en/ https://www.space.com/nebula-definition-types https://www.britannica.com/science/nebula | |||
NEO (Near-Earth Object) | ||
---|---|---|
Source: Video from NASA explaining NEO: https://www.youtube.com/watch?v=r-OCcFnp2RA Short Definition:NEO, or near-Earth object, is a celestial body which is in the size range of meters to tens of kilometres, that orbits the sun and approaches the earth within the distance of 1.3 AU (astronomical units). Detailed Definition:Among the 600,000 known asteroids, only 20,000 of them are NEOs. To be classified as such, the object must be natural and cannot be manmade. Some of them could potentially hit the earth and for this reason, some organisation keep track of them everyday. Historically speaking, NEOs have had an impact of the earths geological and biological history. Most of the NEOs are Apollo asteroids (55.4%), meaning that they come from the Apollo asteroid group. The second most common are Amor asteroids (36.4%), and third most common are Aten asteroids (7.7%). Etymology:Acronym of "near-Earth object." Sample Sentence:An astronomer would for example say during a lecture: “The Amor asteroid, 433 Eros, was the first NEO discovered in 1898, by D. Witt of Berlin, Germany, using a photographic plate to record its position.” Translations:
Links to Articles/Videos: | ||
Neutron star | |||
---|---|---|---|
Short Definition: A Neutron star is a celestial body
and is the collapsed core of a massive supergiant star that had a total mass of
about 10-25 solar masses. Compared to other stellar objects, they are much
smaller and much denser. Not counting black holes or hypothetical stellar
objects, they are the densest stellar object in the universe. Detailed Definition: A Neutron stars is a stellar object, which is only a few kilometres in
diameter, but has the mass of a star. So even compared to others stellar objects they have a mind-boggling density and are even so dense, that they are on the
cusp of becoming a black hole. Stars hold an equilibrium between the force of
gravity forcing plasma inwards, which in turn enables fusion of hydrogen to
helium, and this releases energy that pushes outwards. So the equilibrium is
directly linked to the amount of hydrogen available in stars. Breaking this equilibrium
in our sun would result in it transforming to a red giant and then to a white
dwarf. In those massive supergiant stars, gravity will prevail and will
compress the core to the density of an atomic nucleus, which in turn forces
heavier elements to fuse, and thus the outer layer will get bigger by a factor
of x100. After a time the heavier elements are fused to iron and can not be fused any more, so the fusion activity will cease, and the star will collapse to its
core. Electrons and Protons will be forced into each other and form Neutrons as
dense as in atomic nuclei, where nuclei are so densely packed, they form a
layer that is called nuclear pasta. Another interesting property is that they
are spinning really fast, which empowers their magnet fields and gives them the
strongest magnet field in our universe. Etymology: Neutron from Ne and uterà neutral +on ending from ion subatomic particle suffix Star from Proto-Indo-European rooth₂stḗrSample Sentence(s): The physics in the core of the Neutron stars are still largely unknown and are still subject of speculation. Scientists were able to detect gravitational
waves of two merging Neutron stars and confirmed the theory of Albert Einstein. French: Étoile à neutrons German: Neutronenstern Polish: Gwiazda neutronowa Swedish: Neutronstjärna Links to Videos/Articles: https://www.youtube.com/watch?v=udFxKZRyQt4&list=PLFs4vir_WsTwEd-nJgVJCZPNL3HALHHpF&index=16 https://www.nasa.gov/mission_pages/GLAST/science/neutron_stars.html | |||