noooooooooooooooooooo!
The lunar highlands are older than the maria because they have accumulated more impact craters over time. This suggests that the highlands are composed of older, more geologically stable rock compared to the volcanic plains of the maria.
The maria (large, dark, flat plains formed by ancient volcanic activity) on the moon are younger than the craters (impact sites from asteroids or meteoroids). The maria are estimated to be around 3 billion years old, while many of the craters are thought to be upwards of 4 billion years old.
The light spots on the moon are called lunar highlands and they are elevated regions made up of ancient crustal rocks. These areas appear brighter than the dark lunar maria because they reflect more sunlight.
Highlands are mountainous areas that have been in existence for millions of years, while mares are large dark plains on the moon that were formed by volcanic activity more recently. Therefore, highlands are older than mares.
To determine the relative ages of the Moon's maria and highlands, scientists analyze the density and distribution of impact craters on their surfaces. The highlands, which are heavily cratered, are older than the maria, which have fewer craters due to younger volcanic activity that filled in the basins. Radiometric dating of lunar samples can also provide age estimates, but crater counting is a primary method for establishing relative ages. By comparing these features, researchers can infer the geological history of the Moon.
The lunar highlands are older than the maria because they have accumulated more impact craters over time. This suggests that the highlands are composed of older, more geologically stable rock compared to the volcanic plains of the maria.
The lunar highlands are older than the maria.
Lunar mare are dark, smooth plains formed by ancient volcanic activity, while lunar highlands are lighter-colored, rugged terrains composed of mountains, hills, and craters. Mare regions have fewer impact craters than highlands, indicating younger geological features. Mare plains formed from lava flows that filled large impact basins, while highlands represent the original lunar crust.
Younger mares and mares with good uterine characteristics tend to foal earlier than older mares. With age the uterus tends to be compromised to a greater or lesser degree which slows the development of the foal and increases gestation.
The maria (large, dark, flat plains formed by ancient volcanic activity) on the moon are younger than the craters (impact sites from asteroids or meteoroids). The maria are estimated to be around 3 billion years old, while many of the craters are thought to be upwards of 4 billion years old.
no silly, HARD Mares is the plural of mare, which is a female horse/pony. So "mares" would be more than one female horse/pony.
Highlands are mountainous areas that have been in existence for millions of years, while mares are large dark plains on the moon that were formed by volcanic activity more recently. Therefore, highlands are older than mares.
The light spots on the moon are called lunar highlands and they are elevated regions made up of ancient crustal rocks. These areas appear brighter than the dark lunar maria because they reflect more sunlight.
Impact craters on the moon have no water/weather to erode the craters away, but on Earth the erosion erases the craters over time.
Younger than me is correct.
There is no significant amount of erosion on the Moon.
Craters on the moon are formed by impacts from asteroids or meteoroids. When these objects collide with the moon's surface, they create depressions that we see as craters. These craters can vary in size and shape, and they impact the lunar surface by altering its topography and composition. They also provide valuable information about the history of impacts in the solar system.