Stamp: Aternernative sources of energy (UNO Vienna 1981)

Aternernative sources of energy (UNO Vienna 1981)

01 January (UNO Vienna ) within release Aternernative sources of energy goes into circulation Stamp Aternernative sources of energy face value 7.50 Austrian schilling

Stamp Aternernative sources of energy in catalogues
Michel: Mi:NT-WN 20
Yvert et Tellier: Yt:NT-WN 20

Stamp is horizontal format.

Also in the issue Aternernative sources of energy:

Data entry completed
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Stamp Aternernative sources of energy in digits
Country: UNO Vienna
Date: 1981-01-01
Size: 37 x 27
Perforation: 13½ x 13
Emission: Commemorative
Format: Stamp
Face Value: 7.50 Austrian schilling
Print run: 1611130

Stamp Aternernative sources of energy it reflects the thematic directions:

Celestial bodies or heavenly bodies are objects in space such as the sun, moon, planets, and stars. They form a part of the vast universe we live in and are usually very far from us.

In physics, energy (from Ancient Greek ἐνέργεια (enérgeia) 'activity') is the quantitative property that is transferred to a body or to a physical system, recognizable in the performance of work and in the form of heat and light. Energy is a conserved quantity—the law of conservation of energy states that energy can be converted in form, but not created or destroyed. The unit of measurement for energy in the International System of Units (SI) is the joule (J).

The Sun, also known as Sol, is a star at the center of the solar system. It is a white star that gives off different types of energy such as infrared energy (heat), ultraviolet light, radio waves and light. It also gives off a stream of particles, which reaches Earth as "solar wind". The source of all this energy is nuclear fusion. Nuclear fusion is the reaction in the star which turns hydrogen into helium and makes huge amounts of energy. It is a nearly perfect ball of hot plasma.

Stamp, Aternernative sources of energy, UNO Vienna,  , Celestial Bodies, Energy, Sun