Editing 2931: Chasing

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| The International Date Line || 15% || 10% || A jagged conceptual line running from the North to South poles around 180 degrees of longitude, used to separate the time zones that start and end each day. There's nothing to see at these locations, as the line is an abstraction and does not actually coincide with anything in real life, as well as mostly being in the Pacific Ocean, by-passing actual landfall, as well as across the Arctic Southern Oceans. The zones for {{w|time in Antarctica}} are already more pragmatically simplified or just fall back to {{w|Coordinated Universal Time}}.
 
| The International Date Line || 15% || 10% || A jagged conceptual line running from the North to South poles around 180 degrees of longitude, used to separate the time zones that start and end each day. There's nothing to see at these locations, as the line is an abstraction and does not actually coincide with anything in real life, as well as mostly being in the Pacific Ocean, by-passing actual landfall, as well as across the Arctic Southern Oceans. The zones for {{w|time in Antarctica}} are already more pragmatically simplified or just fall back to {{w|Coordinated Universal Time}}.
 
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| Meteors || 35% || 95% || Also called "shooting stars". These are fleeting streaks of light that are visible when bits of rock or dust enter the atmosphere and burn up. These are generally rare, making them exciting to see, but there are {{w|meteor showers}} when many are visible due to the Earth passing through a large cloud of dust (usually the remnants of a comet). To astronomy buffs, these can be like natural fireworks shows. Because each meteor streak lasts for a fraction of a second, it's not generally possible to chase them, although if the rock is large enough it may survive to the ground and become a {{w|meteorite}}, which chasers [[1723: Meteorite Identification|may be able to find]] by tracking its path through the sky.
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| Meteors || 35% || 95% || Also called "shooting stars". These are fleeting streaks of light that are visible when bits of rock or dust enter the atmosphere and burn up. These are generally rare, making them exciting to see, but there are {{w|meteor showers}} when many are visible due to the Earth passing through a large cloud of dust (usually the remnants of a comet). To astronomy buffs, these can be like natural fireworks shows. Because each meteor streak lasts for a fraction of a second, it's not generally possible to chase them, although if the rock is large enough it may survive to the ground and become a {{w|meteorite}}, which chasers may be able to find by tracking its path through the sky.
 
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| {{w|Rainbows}} || 35% || 90% || A visual effect that occurs when sunlight is refracted by water droplets in the air, spreading the light into a spectrum of different colors. Their 'location' is relative to each observer, so long as the necessary components combine correctly in the first place, so any coordinated movement is restricted to finding the right sort of standpoint from which a rainbow is visible. Moving "towards" a rainbow typically results in the rainbow "moving away" from the observer at the same speed.
 
| {{w|Rainbows}} || 35% || 90% || A visual effect that occurs when sunlight is refracted by water droplets in the air, spreading the light into a spectrum of different colors. Their 'location' is relative to each observer, so long as the necessary components combine correctly in the first place, so any coordinated movement is restricted to finding the right sort of standpoint from which a rainbow is visible. Moving "towards" a rainbow typically results in the rainbow "moving away" from the observer at the same speed.

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