Browse the glossary using this index

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

H

Heavy Element

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

Image/Video/Audio:


Image: Periodical Table

Image/Video/Audio Source:

https://commons.wikimedia.org/wiki/File:Ionization_energy_periodic_table.svg

Short Definition:

Heavy elements are the general name for elements containing atomic numbers greater than 92. Above these, elements with atomic numbers 112 and above are called superheavy elements. The state that creates the atomic number is the number of protons in the nucleus of the element.

Detailed Definition:

Heavy elements, which are determined by the number of protons in the nucleus of the element (this called atomic number) are elements with atomic number greater than 92. One row above them there is superheavy elements with atomic numbers greater than 112. The first artificially produced heavy and superheavy elements were first produced during the Cyclotron experiments.

One of the most important issues about heavy elements is the concept of 'island of stability'. This concept refers to the region in the table of nucleides where elements with half-lives longer than some other super heavy elements are found. However, it should be noted that we are ona narrow time scale, from minutes to micro/nano seconds at most. The term was first coined in 1998 with the discovery of the super heavy element 114 (Flerovium).

Etymology:

Heavy – From Proto Germanic (hafiga)

Element – From Latin (elementum)

(origin and meaning of heavy. (n.d.). Etymonline. https://www.etymonline.com/word/heavy)

(element - Wiktionary. (n.d.). https://en.wiktionary.org/wiki/element)

Sample Sentence(s):

‘’The heaviest element known at the end of the 19th century was uranium, with an atomic mass of approximately 240 (now known to be 238) amu.’’

(Wikipedia contributors. (2022, December 31). Superheavy element. Wikipedia. https://en.wikipedia.org/wiki/Superheavy_element)

‘’Although the scientific community has assigned these heaviest elements to their own spots on the periodic table, there is still a lot we don’t know about them.’’

(Exploring the superheavy elements at the end of the periodic table. (n.d.). cen.acs.org.)

Translations of Terms/Concepts into Partner Languages:

French:

Élément lourd

German:

Schweres element

Polish:

Ciężki pierwiastek

Swedish:

Tungt element

Turkish:

Ağır Element

Links to Videos/Articles:

Cookie Absent. (n.d.). https://physicstoday.scitation.org/action/cookieAbsent

Discovery of Elements 113 and 115. (n.d.). https://pls.llnl.gov/research-and-development/nuclear-science/project-highlights/livermorium/elements-113-and-115

Seeker. (2019, November 10). This Superheavy Atom Factory Is Pushing the Limits of the Periodic Table [Video]. YouTube. https://www.youtube.com/watch?v=kg0AN8bZ4us

Wikipedia contributors. (2022, December 31). Superheavy element. Wikipedia. https://en.wikipedia.org/wiki/Superheavy_element














Heliosphere

(Last edited: Friday, 26 May 2023, 5:25 PM)

Term/Concept: 

Heliosphere

Image/Video/Audio:




Image/Video/Audio Source:


Short Definition:

The Heliosphere is the extended layer of the Sun consisting of its magnetosphere, astrosphere and atmosphere. It has a bubble-like shape, covering the entire Solar System. 


Detailed Definition:

The Heliosphere in physics terms is a cavity that is formed by the Sun in its neighbourhood. It binds our solar system together, like an atmosphere on Earth binds life on the surface. It also produces weather conditions like the ones on Earth, but the weather happens on a larger, solar system scale. 

The Heliosphere consists of plasma, particles and magnetic fields that interact with the space environment, producing what we call space weather. It is also a shield, without which we probably would not exist, as it protects our planet from cosmic rays, particles created far away in space. Without the existence of a heliosphere, our living cells would be continuously bombarded, causing damage.

As this wave of solar wind wanders away from the Sun, at some point it reaches termination shock, where its speed suddenly drops from even 700 km/s. Beyond the termination shock lies the heliosheath, the outer region of the heliosphere, where solar wind becomes denser and hotter as it presses towards wind in interstellar space. The boundary between it and the interstellar wind is called heliopause, the pressure of both of the winds stays in balance there. 


Etymology:

helio- +‎ -sphere

helio - from Ancient Greek ἥλιος (hḗlios).

sphere - from Ancient Greek σφαῖρα (sphaîra, “ball, globe”)



Sample Sentence(s):

Voyager 1 travelled through the heliosphere and encountered heliopause in 2015. 


As the heliopause marks the boundary between the matter originating from the Sun and matter originating from the rest of the galaxy, the spacecrafts that left the heliosphere are travelling through interstellar space.


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: 

Héliosphère


German:

Die Heliosphäre


Polish:

Heliosfera


Swedish:

Heliosfären


Links to Videos/Articles: