Source: https://en.wikipedia.org/wiki/File:Black_hole_-_Messier_87_crop_max_res.jpg

Short definition: A Black Hole is a region of spacetime where the gravitational field is so strong that nothing, not even light or other electromagnetic waves can escape its event horizon. An event horizon is “the point of no return”, meaning the boundary beyond which nothing can escape.

Detailed definition: Since Black Holes can’t be observed directly with telescopes, they’re usually detected by other means, such as observing their gravitational influence on their surroundings.

Most Black Holes are formed from large stars that die in a supernova explosion - these Black Holes are usually around 20 times as massive as the Sun. However, there also exist Black Holes that are incredibly large, called Supermassive Black Holes, which can be millions or even billions times as massive as the Sun. Scientists believe that at the centre of almost every big galaxy lies a Supermassive Black Hole, for example Sagittarius A* at the centre of the Milky Way.

Etymology: Presumably in December 1967, a student suggested the phrase "black hole" at a lecture by John Wheeler; Wheeler adopted the term for its brevity and "advertising value", and it quickly caught on. (Source: Siegfried, T. (2019, August 9). 50 years later, it’s hard to say who named Black Holes. Science News. https://www.sciencenews.org/blog/context/50-years-later-its-hard-say-who-named-black-holes)

Sample sentence(s): Some Black Holes apparently have nonstellar origins. (Source: Lohnes, K. (n.d.). How Do Black Holes Really Work? Encyclopedia Britannica. https://www.britannica.com/story/how-do-black-holes-really-work )

Translations:

French: Trou noir

German: Schwarzes Loch

Italian: buco nero

Polish: Czarna dziura

Swedish: Svart hål

Links to Videos/Articles: 

The Economist. (2022, July 12). Black holes: why they matter [Video]. YouTube. https://youtu.be/qqMAFtIGaq4

Black Holes | Science Mission Directorate. (n.d.). https://science.nasa.gov/astrophysics/focus-areas/black-holes

Source: https://en.wikipedia.org/wiki/File:Black_hole_-_Messier_87_crop_max_res.jpg

Short Definition:

The horizon of a black hole is called event horizon and is an astrophysical phenomenon, which describes the “point of no return” where matter and even light can not cross back according to our understandings of physics. The event horizon is a boundary in spacetime, where the gravitational pull becomes absolute.

Detailed Definition:

The astrophysical phenomenon of the event horizon defines the boundary of spacetime, where the ability of mass to deform spacetime is absolute.

Near this event horizon time seems to work differently, because of gravitational time dilation, which appears to slow down clocks near the horizon more than those farther away and the clock would take an infinite amount of time to reach the black hole in itself.

The huge amounts of gravitational pull causes any light to redshift in a process called gravitational redshift. A clock that is falling into a black hole would change from being visible from an outside perspective, to the light of it red shifting and then finally it would disappear from view and all this in a mere minute. On the contrary an indestructible observer that falls into a black hole would experience time normally and it would fall into the black hole in a finite amount of time.

Etymology:

Black hole  term was coined in astronomy in 1964

Horizon Greekhorizon (kyklos) àboundary

Sample Sentence(s):

From an outside perspective an object falling into the black hole horizon would take an infinite amount of time to reach it.

Sloan Digital Sky Survey image of blazar Markarian 421. Source: https://en.wikipedia.org/wiki/Markarian_421#/media/File:SDSS_Mrk_421.jpg

Short Definition:

A blazar is a type of active galaxy nucleus with a jet composed of ionized matter traveling at nearly the speed of light, which direction is nearly towards an observer. Due to the jet almost directly shooting towards Earth, a blazar appears much brighter on observations than in case of facing another direction. Blazars are a source of powerful radiation in all electromagnetic spectrum, especially in high-energy gamma rays. Blazars are among the most energetic phenomena in the universe and are an important subject to research. 

Detailed Definition:

Blazars are an extremely bright, starlike object characterized by rapid changes in luminosity and a flat spectrum caused by a jet composed of ionized matter traveling at nearly the speed of light directed at the observer. Blazars emit electromagnetic radiation over a very wide range of frequencies, but mostly distinguished by amount of radio and gamma rays. Due to blazar's instabilities its properties change over time, specifically the variability and intensity of their observable brightness, which is distinguishing blazars from another class of active galactic nucleus, quasars. Blazars are important topics of research in astronomy and astrophysics. Blazar research includes investigation of the properties of accretion disks and jets, the central supermassive black holes and surrounding host galaxies, and the emission of high-energy photons, cosmic rays, and neutrinos.

Etymology:

Coined by 1978 by astronomer Edward Spiegel from BL Lac object and quasar.

Sample Sentence(s):

"Blazars are thought to be active galactic nuclei, with relativistic jets oriented close to the line of sight with the observer."
“Strong γ-ray emission is detected in blazars only.”

Translations:

French: 

Blazar

German:

Blazare

Polish:

Blazar

Swedish:

Blazar

Links to Videos/Articles:

https://www.merriam-webster.com/dictionary/blazar

Definition:

Canadian Space Agency is a national space agency of Canada, whose aim is to coordinate spaceflight activities. It is responsible for space exploration (focusing on physical processes in stars), as well as Earth observation and monitoring its resources.

Canadian Space Agency was established in 1989  and works on space science and exploration, satellite communications, and it also provides space awareness and promotes the activities of the organisation. International cooperation with other space agencies is also part of the CSA’s mission. The headquarters are located in Longueuil, Canada.

Sample Sentence(s):

"The Canadian Space Agency is now developing a next generation of satellites."

"The Canadian Space Agency is a founding member of the Charter."

Translations:

• French: Agence spatiale canadienne
  
• German: Kanadische Weltraumorganisation
  
• Polish: Kandyjska Agencja Kosmiczna
  
• Swedish: kanadensiska rymdorganisationen
  

Links to Videos/Articles:

https://www.asc-csa.gc.ca/eng/default.asp

Creator : Unknown Year: (n.d.) Title of image: White Dwarf Mass-Radius Relationship Description of image: Graph illustrating the mass-radius relationship of white dwarf stars Retrieved from URL: https://upload.wikimedia.org/wikipedia/commons/thumb/1/14/WhiteDwarf_mass-radius_en.svg/860px-WhiteDwarf_mass-radius_en.svg.png

Definitions

Short Definition
The Chandrasekhar limit is a fundamental concept in astrophysics that determines the maximum mass a white dwarf star can attain. It is named after the Indian astrophysicist Subrahmanyan Chandrasekhar, who proposed this limit in 1930. According to the Chandrasekhar limit, if a white dwarf exceeds about 1.4 times the mass of the Sun, it will collapse under its own gravity, leading to a catastrophic event such as a supernova explosion.

Detailed Definition
The Chandrasekhar limit is the maximum mass that a white dwarf star can have before it undergoes a collapse and explodes in a type of supernova known as a Type Ia supernova. This limit was first proposed by Indian astrophysicist Subrahmanyan Chandrasekhar in 1930, who showed that if a white dwarf exceeds a certain mass, the pressure generated by electrons in the star's core can no longer balance the force of gravity, causing the star to collapse under its own weight.

The Chandrasekhar limit is currently estimated to be about 1.4 times the mass of the Sun. When a white dwarf reaches this mass, it can no longer support itself through electron degeneracy pressure and instead collapses into a neutron star or black hole. The collapse generates a tremendous amount of energy, which is released in a supernova explosion.

Etymology
This term was first proposed by Indian astrophysicist Subrahmanyan Chandrasekhar in 1930.

Sample Sentence(s)

Please provide 1-2 sample sentences using the term/concept in its appropriate scientific context and most common usage.

The Chandrasekhar limit determines whether a star ends its life as a smoldering white dwarf, or explodes in a supernova to become a neutron star or black hole.

Author : Staff, Space.com Year: (n.d.) Title of the article: Chandrasekhar Limit: Definition, Facts & Equation Title of the Website: Space.com Retrieved Date: May 29, 2023 URL: https://www.space.com/chandrasekhar-limit

Translations of Terms/Concepts into Partner Languages

French
La masse de Chandrasekhar

German
das Chandrasekhar- Grenze

Italian
Limite di Chandrasekhar

Polish
granica Chandrasekhara

Swedish
Chandrasekhargränsen

Additional Translations of Terms/Concepts into Other Lang...

Russian: Предел Чандрасекара

Links to Videos/Articles:

https://www.toppr.com/guides/physics/astronomy/chandrasekhar-limit/

Author(s): Unknown Year: (n.d.) Title of the article: Chandrasekhar Limit Title of the Website: Toppr.com Retrieved Date: May 29, 2023, URL: https://www.toppr.com/guides/physics/astronomy/chandrasekhar-limit/

Source: ESA - ESA commissions world’s first space debris removal

Definition:

ClearSpace-1 is a mission targeting the removal of the Vega Secondary Payload Adapter (Vega) which is planned for launch in 2025. The mission is brought forward as a service contract with a startup-led commercial consortium, to help establish a new market for in-orbit servicing, as well as debris removal.

The ClearSpace-1 ‘chaser’ will be launched into a lower 500-km orbit for commissioning and critical tests before being raised to the target orbit for rendezvous and capture using a quartet of robotic arms under ESA supervision. The combined chaser plus Vespa will then be deorbited to burn up in the atmosphere.

Etymology:

Sample Sentences(s):

Translations:

• French:
  
• German:
  
• Polish: Misja ClearSpace-1
  
• Swedish:

Links to Videos/Articles:

ESA - ESA commissions world’s first space debris

earth observation for sustainable development (esa.int) removal

Source:

Short Definition:
A Comet is a small object orbiting the star (e.g. the Sun) composed of dust, rock and ices. Comets appear in our solar system and have mostly origin in Kuiper belt or Oort Cloud.

Detailed Definition:
Comets show up periodically, orbiting a star on the ecliptic orbit with different span from several to thousands of years. The comet appearance changes depending on the distance from the source of heat. If the comet is far away from the star, it only consists of the nucleus. After approaching the source of a heat, the surface of the icy heart of the comet starts heating up and slowly transforms into gas, creating a coma (fuzzy cloud of gas and dust) around the nucleus. When the coma appears, two tails spread behind the nucleus. Due to the ion tail's electric charge, it always points away from the star. The dust tail indicates the path of the nucleus, which is wide, curved and spread behind the nucleus for millions of miles. The most popular comet is Halley's Comet (1P/Halley) which is visible from Earth every 75–79 years.

Sample Sentence(s):
There are likely billions of comets orbiting our Sun in the Kuiper Belt and even more distant Oort Cloud.

French:
La comète

German:
der Komet

Polish:
kometa

Swedish:
Komet

Spanish
El cometa

Links to Videos/Articles:
https://solarsystem.nasa.gov/asteroids-comets-and-meteors/comets/overview/
https://spaceplace.nasa.gov/comets/en/
https://en.wikipedia.org/wiki/Comet#Etymology
https://en.wikipedia.org/wiki/Comet_Encke
https://en.wikipedia.org/wiki/Halley%27s_Comet

Term/Concept: 

constellation

Image/Video/Audio:

Term/Concept: constellation Image/Video/Audio: Image/Video/Audio Source: Sullivan, R. (2017, June 12). Constellations map. flickr. https://www.flickr.com/photos/47430793@N08/35249283965

Short Definition:

Detailed Definition:

Etymology:

Sample Sentence(s):

Translations of Terms/Concepts into Partner Languages [Multiple fields for entering the translation of the term in each partner language, additional languages can potentially be added, e.g. Russian, Chinese, Portuguese]

French: 

German:

Polish:

Swedish:

Links to Videos/Articles:

Definition:

A European Earth observation programme aiming at monitoring land, atmosphere and the marine environment, supporting emergency management, ensuring civil security and mitigating the consequences of climate change.

Etymology:

The programme is named after Nicolaus Copernicus, who was a Renaissance scientist and the author of the heliocentric model of the Universe.

Translations:

• French:
  
• German:
  
• Polish: Program Copernicus
  
• Swedish:
  

Links to Videos/Articles:

https://www.esa.int/Applications/Observing_the_Earth/Copernicus/Europe_s_Copernicus_programme

https://www.copernicus.eu/en/copernicus-services

https://www.copernicus.eu

Short definition: Cosmic rays are high energy particles that travel through space at nearly the speed of light. Most cosmic rays are represented by atomic nuclei stripped of their atoms.

Detailed definition: Cosmic rays were discovered by Victor Hess in 1912. They originate from the Sun, from the Milky Way, and from distant galaxies. Most cosmic rays (89%) are protons of hydrogen, but some of them are nuclei of helium (around 10%) and other, heavier nuclei. Only about 1% of cosmic rays are lone electrons. Once a cosmic ray reaches the Earth’s atmosphere, it collides with other atoms there and bursts them into different particles, namely pions, muons and neutrinos.
The extremely high energy that cosmic rays have often causes electronics to malfunction: for example, corrupted data in memory devices or incorrect performance in CPUs. Cosmic rays used to be a problem mainly in spacecraft, satellites and high-altitude aircraft, but is becoming a concern in regular electronics too due to transistors becoming smaller in size.

Etymology: Cosmic comes from Ancient Greek κόσμος (kósmos, “order, proper order of the world”). The term ray likely arose because cosmic rays were initially believed to be electromagnetic radiation.

Sample sentence(s): Cosmic rays follow convoluted paths and arrive at the top of the Earth’s atmosphere from all directions.

Translations:

French: Rayonnement cosmique

German: Kosmische Strahlung

Italian: Raggi cosmici

Polish: Promieniowanie kosmiczne, promienie kosmiczne

Swedish:  Kosmiska partiklar

Links to Videos/Articles:

Cosmic Rays - Introduction. (n.d.). https://imagine.gsfc.nasa.gov/science/toolbox/cosmic_rays1.html

Friedlander, M. W. (2023, April 21). Cosmic ray | Definition, Types, Effects, & Facts. Encyclopedia Britannica. https://www.britannica.com/science/cosmic-ray

Vox. (2019, August 30). The mysterious rays shooting at us from space [Video]. YouTube. https://youtu.be/Z9gQLELtbhg