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B

Binary stars

(Last edited: Friday, 2 June 2023, 5:09 PM)

Sources:

Center for High Angular Resolution Astronomy (2008, August 21). Beta Lyrae - CHARA (inverted colors). wikimedia commons. https://commons.wikimedia.org/w/index.php?curid=86270181

Short Definition:

A system composed of two stars in which both share a common centre of revolution or one revolves around the other.

Detailed Definition:

A binary star is a pair of stars in orbit around their common centre of gravity. The term is different from a double star, which refers to any two stars close together in the sky. If components in binary star systems are close enough, they can gravitationally distort their mutual outer stellar atmospheres. In some cases, binary systems can exchange mass, evolving in a way which is unattainable for single stars.

Etymology:

The term binary was first used in the context of space terminology by Sir William Herschel in 1802, in one of his works regarding the observation of double stars.

Binary - "dual, twofold, double," mid-15c., from Late Latin binarius

Sample Sentence(s):

One of the examples of a binary star is Sirius, the brightest star in the night sky.

Translations of Terms/Concepts into Partner Languages

French: Étoile binaire

German: Doppelstern

Polish: Gwiazda binarna

Swedish: Binär Stjärna


Links to Videos/Articles:

https://www.youtube.com/watch?v=pIFiCLhJmig

https://www.nasa.gov/mission_pages/swift/bursts/binary-clash.html

https://www.scienceabc.com/nature/universe/what-are-binary-stars.html


Black hole Horizon

(Last edited: Friday, 28 April 2023, 6:09 PM)

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.

 

The black hole horizon is the point of no return, where matter or light are not able to cross back.

French:
Horizon du trou noir
German:
Schwarzes Loch-Horizont
Polish:
Horyzont czarnej dziury
Swedish:
Horisont för svarta hål





Blazar

(Last edited: Friday, 28 April 2023, 6:09 PM)

Sloan Digital Sky Survey image of blazar Markarian 421

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