DEFINITION OF ERMS: Define the toti ASEOA
CONSTELLATOS
Constellation
Stars
Magnitude
Light year
Temperature
Parallax
Brightness
Photosphere
Corona
Fusion
Fission
Sunspots
Solar flare
Aurora
Prominences
Chromosphere
Protostar
REFLECTION

Explain how a star is form and dies.​


Sagot :

Answer:

  • A constellation is a group of stars that appears to form a pattern or picture like Orion the Great Hunter, Leo the Lion, or Taurus the Bull. Constellations are easily recognizable patterns that help people orient themselves using the night sky. There are 88 “official” constellations.
  • a fixed luminous point in the night sky which is a large, remote incandescent body like the sun.
  • magnitude is described in simple words as 'distance or quantity'. It shows the direction or size that is absolute or relative in which an object moves in the sense of motion. ... Magnitude defines the size of an entity, or its speed when moving, in comparison to motion.(physics terms)
  • The light-year is a unit of length used to express astronomical distances and is equivalent to about 9.46 trillion
  • the degree or intensity of heat present in a substance or object, especially as expressed according to a comparative scale and shown by a thermometer or perceived by touch
  • Parallax (from Ancient Greek παράλλαξις (parallaxis) 'alternation') is a displacement or difference in the apparent position of an object viewed along two different lines of sight, and is measured by the angle or semi-angle of inclination between those two lines.
  • Brightness is an attribute of visual perception in which a source appears to be radiating or reflecting light. In other words, brightness is the perception elicited by the luminance of a visual target
  • The photosphere is the lowest layer of the solar atmosphere. It is essentially the solar "surface" that we see when we look at the Sun in "white" (i.e. regular, or visible) light. When we observe sunspots and faculae (bright little cloud-like features) we are observing them in the photosphere.
  • the rarefied gaseous envelope of the sun and other stars. The sun's corona is normally visible only during a total solar eclipse, when it is seen as an irregularly shaped pearly glow surrounding the darkened disk of the moon.
  • Fusion is a reaction in which two or more atomic nuclei are combined to form one or more different atomic nuclei and subatomic particles. The difference in mass between the reactants and products is manifested as either the release or the absorption of energy.
  • Fission is the splitting of a heavy nucleus into lighter nuclei and fusion is the combining of nuclei to form a bigger and heavier nucleus. The consequence of fission or fusion is the absorption or release of energy.
  • Sunspots are temporary phenomena on the Sun's photosphere that appear as spots darker than the surrounding areas. They are regions of reduced surface temperature caused by concentrations of magnetic field flux that inhibit convection. Sunspots usually appear in pairs of opposite magnetic polarity.
  • Solar flares are a sudden explosion of energy caused by tangling, crossing or reorganizing of magnetic field lines near sunspots. The surface of the Sun is a very busy place. It has electrically charged gases that generate areas of powerful magnetic forces. These areas are called magnetic fields.
  • Aurora is a natural light display in the Earth's sky, predominantly seen in high-latitude regions (around the Arctic and Antarctic).
  • A prominence is a large, bright, gaseous feature extending outward from the Sun's surface, often in a loop shape. Prominences are anchored to the Sun's surface in the photosphere, and extend outwards into the solar corona
  • Reflection. Light can reflect off of a surface. When light encounters a discontinuity in the medium through which it is being transmitted, a fraction will be reflected. We define the angle of incidence and the angle of reflection relative to the normal with respect to the plane of discontinuity.