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Astronomy
Regents Review Cocepts
| Question | Answer |
|---|---|
| How Does the Sun Produce Energy? | nuclear fusion |
| During nucleosynthesis hydrogen atoms within the Sun collide and fuse together to form | Helium |
| During nucleosynthesis within a massive star, Oxygen (O) atoms fuse together to form | Silicon |
| explains the origin of the universe as an enormous explosion that occurred about 13.8 billion years ago. | The Big Bnag Theory |
| Proves that distant galaxies appear to be moving away from us,stretching their light toward the red end of the spectrum. | red-shift |
| A faint glow of radiation left over from the early universe. | Cosmic background radiation |
| A cloud of gas and dust where stars form | nebula |
| The longest stage in an average stars life cycle, where the stars burns off hydrogen. | The Main Sequence |
| *The Star Group in which Vega, Sirius and our Sun are found | The Main Sequence |
| *The spectral class of a star with a temperature of 4200 degrees | K |
| A massive explosion which spreads heavier elements into space. | Supernova |
| *the final stage in a Sun-like star's life cycle | White Dwarf |
| Planets stay in orbit due to the balance between inertia and | Gravity |
| The orbital velocity of an astronomical object is determined by the object mass and ____________________ from its primary. | Distance |
| The degree or elongation within the orbital path of a planet or comet is known as | Eccentricity of orbit |
| When a planet is at its closest approach to its primary it is said to be at ___________________________ | Perihelion |
| When a planet is at its farthest approach to its primary it is said to be at ___________________________ | Aphelion |
| As the distant between a planet and it perihelion decreases, its orbital velocity will____________________ | Increase |