Nebulae and Tectonic Plates
Nebulae and Tectonic Plates
Nebulae and Tectonic Plates
What Is a Nebula?
A nebula is a giant cloud of dust and gas in space. Some nebulae (more than
one nebula) come from the gas and dust thrown out by the explosion of a dying
star, such as a supernova. Other nebulae are regions where new stars are
beginning to form. For this reason, some nebulae are called "star nurseries.”
The closest nebula to us is the Helix Nebula (NGC 7293)
How do stars form in a nebula?
Nebulae are made of dust and gases—mostly hydrogen and helium. The dust
and gases in a nebula are very spread out, but gravity can slowly begin to pull
together clumps of dust and gas. As these clumps get bigger and bigger, their
gravity gets stronger and stronger.
Eventually, the clump of dust and gas gets so big that it collapses from its own
gravity. The collapse causes the material at the center of the cloud to heat up-
and this hot core is the beginning of a star.
Where are nebulae?
Structure of earth:
Tectonic plates
It causes earthquakes
It causes volcanism
It induces recycling of elements within the biosphere and between the
geosphere and biosphere
It causes mountain-building
Transform boundaries:
These boundaries happen where two lithosphere plates move apart, or maybe
further precisely, collide away from one other despite the transform faults, where
plates are neither created nor destroyed.
Divergent boundaries:
These boundaries happen when both plates move apart from one other.
Convergent boundaries:
These boundaries happen where both plates move towards one other to form a
zone of subduction or a continental collision.
Transform boundaries:
These boundaries happen when natural or human-made structures that cross a
transform boundary are offset—split into pieces and carried in opposite
directions.