ss Flashcards

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1
Q

Solar Nebula Theory

A

States that the solar system developed out of an interstellar cloud of dust and gas, called a nebula

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2
Q

Terrestrial Planet

A

Planets made of rock

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3
Q

Jovian Planet

A

Planets made of gas

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4
Q

Dwarf Planet

A

A celestial body resembling a small planet but lacking certain technical criteria that are required for it to be classed as such

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5
Q

Order of planets from the Sun

A

Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune

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6
Q

Asteroid

A

A small rocky body orbiting the sun

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7
Q

Comet

A

A celestial object consisting of a nucleus of ice and dust and, when near the sun, a “tail” of gas and dust particles pointing away from the sun

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8
Q

Meteoroid

A

A small body moving in the solar system that would become a meteor if it entered the earth’s atmosphere

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9
Q

Meteor

A

A small body of matter from outer space that enters the earth’s atmosphere, becoming incandescent as a result of friction and appearing as a streak of light

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10
Q

Meteorite

A

A meteor that survives its passage through the earth’s atmosphere such that part of it strikes the ground

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11
Q

Corona

A

The rarefied gaseous envelope of the sun; normally visible only during a total solar eclipse

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12
Q

Chromosphere

A

A reddish gaseous layer immediately above the photosphere of the sun

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13
Q

Photosphere

A

The luminous envelope of the sun from which its light and heat radiate (layer we can see)

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14
Q

Core

A

The center of the sun; densest layer; fusion occur here

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15
Q

Nuclear Fusion

A

A nuclear reaction in which atomic nuclei of low atomic number fuse to form a heavier nucleus with the release of energy

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16
Q

Constellation

A

A group of stars forming a recognizable pattern that is traditionally named after its apparent form or identified with a mythological figure

17
Q

Binary star

A

A system of two stars in which one star revolves around the other or both revolve around a common center

18
Q

Absolute Magnitude

A

The brightness of a celestial object as it would be seen at a standard distance of 10 parsecs (the true brightness)

19
Q

Apparent Magnitude

A

The brightness of a celestial object as it is actually measured from the earth

20
Q

Hertzsprung-Russell (HR) Diagram

A

The graph showing the absolute magnitude plotted against the surface temperature for a group of stars

21
Q

Nebula

A

A cloud of gas and dust in outer space, visible in the night sky either as an indistinct bright patch or as a dark silhouette against other luminous matter (birthplace of stars)

22
Q

Protostar

A

A contracting mass of gas which represents an early stage in the formation of a star, before nucleosynthesis has begun

23
Q

Main Sequence Star

A

A series of star types to which most stars belong, represented on a Hertzsprung–Russell diagram as a continuous band extending from the upper left (hot, bright stars) to the lower right (cool, dim stars

24
Q

Red Giant star

A

A very large star of high luminosity and low surface temperature

25
Q

White dwarf star

A

A small very dense star that is typically the size of a planet

26
Q

Neutron star

A

A star of very small radius (typically 18 miles/30 km) and very high density, composed predominantly of closely packed neutrons

27
Q

Supergiant star

A

A very large star that is even brighter than a giant, often despite being relatively cool.

28
Q

Supernova

A

A star that suddenly increases greatly in brightness because of a catastrophic explosion that ejects most of its mass.

29
Q

Black Hole

A

A region of space having a gravitational field so intense that no matter or radiation can escape

30
Q

Parallax

A

The effect whereby the position or direction of an object appears to differ when viewed from different positions

31
Q

Galaxy

A

A system of millions or billions of stars, together with gas and dust, held together by gravitational attractions

32
Q

Red Shift

A

The displacement of spectral lines toward longer wavelengths (the red end of the spectrum) in radiation from distant galaxies and celestial objects (expanding)

33
Q

Hubble’s Law

A

A law stating that the redshifts in the spectra of distant galaxies (and hence their speeds of recession) are proportional to their distance

34
Q

Big Bang Theory

A

The universe as we know it started with an infinitely hot and dense single point that inflated and stretched — first at unimaginable speeds, and then at a more measurable rate — over the next 13.8 billion years to the still-expanding cosmos that we know today