The Atmosphere WS | Quizalize

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The Atmosphere WS

Quiz by Wendy Lathem

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Q 1/15
Score 0
What is the lowest layer of the atmosphere?
45
Troposphere
Q 2/15
Score 0
What is the highest layer of the atmosphere?
45
Exosphere

15 questions

Q.

What is the lowest layer of the atmosphere?

1

45 sec

Q.

What is the highest layer of the atmosphere?

2

45 sec

Q.

What is the 2nd layer of the atmosphere (from the ground)?

3

45 sec

Q.

What is the 3rd layer of the atmosphere (from the ground)?

4

45 sec

Q.

How are layers of the atmosphere divided?

5

60 sec

Q.

How does the temperature in the stratosphere change with increasing altitude?

6

45 sec

Q.

How does the temperature in the thermosphere change with increasing altitude?

7

45 sec

Q.

How does the temperature in the mesosphere change with increasing altitude?

8

45 sec

Q.

How does the temperature in the troposphere change with increasing altitude?

9

45 sec

Q.

Which layer of the atmosphere has the coldest temperatures?

10

30 sec

Q.

Which layer of the atmosphere has the hottest temperatures?

11

45 sec

Q.

What layer of the atmosphere contains the ozone layer?

12

45 sec

Q.

What layer of the atmosphere contains wind and rain?

13

45 sec

Q.

What layer of the atmosphere is the densest (contains the most gasses)?

14

45 sec

Q.

Why do the temperatures in the mesosphere get colder with increasing altitude?

15

60 sec

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THE SOAR SYSTEM A solar system is a group of planets and other celestial bodies that revolve around a star. A solar nebula- a vast cloud of gas and dust, mostly hydrogen and helium. How the Solar System Form • COLLAPSE AND SPINNING DISK FORMATION - Gravity pulls material inward. The cloud flattens into a spinning disk due to conservation of angular momentum. • PROTOSTAR FORMATION- (BIRTH OF THE SUN). Material collects at the center, and begun to heat up. When it reaches to 10 million KELVIN, nuclear fusion begins. thus, SUN is born. • PLANETESIMALS AND PROTOPLANETS. Dust and gas in the disk stick together via static and gravitational forces. These form planetesimals, which grow into protoplanets collision and accretion. • PLANET FORMATION. Inner disk: too hot for gas rocky planets form Mercury, Venus, Earth, Mars. • PLANET FORMATION. Outer disk: gas and ice giants. Jupiter, Saturn, Uranus, Neptune • LEFTOVER DEBRIS. Remaining materials forms moon, asteroids, comets and dwarf planets. DIFFERENT HYPOTHESIS IN THE FORMATION OF SOLAR SYSTEM. 1. NEBULAR HYPOTHESIS- The Solar system formed from a rotating cloud of Gas and Dust (solar nebula). As it rotates conservation of angular momentum caused the cloud to flatten into a disk. the Sun formed at the center (DISK) while planets formed from the surrounding materials through acceleration. thus, it explains the coplanar and nearly circular orbit of the planets all planets orbits around the sun on the same flat, disk shaped plane. Proposed by Immanuel Kant in 1755 and Modified by Pierre Simon Laplace in 1756. PROTOPLANET HYPOTHESIS. The Solar system formed from a rotating cloud of Gas and Dust (solar nebula). As it rotates conservation of angular momentum caused the cloud to flatten into a disk. 2. Protoplanet hypothesis. Builds on the nebular model but focuses more on the role of planetesimals which then form into full planets. PROCESS: - Small solid particles stick together through collisions. As collisions takes place, it grows into kilometer-sized planetesimals. Gravitational interactions lead to the formation of planets. Lead to formation of steroids belts and varying planet sizes 3. Encounter hypothesis. States that the sun encountered a rogue star. The encounter led to the removal of hot gas from both stars due to their gravitational interaction. The hot gas then accumulated and formed the planets. The materials from the less dense rogue star formed the other planets, while that from the sun formed the inner planets. 4. TIDAL HYPOTHESIS. (also called the Tidal Theory) is an early scientific idea about how the solar system might have formed. Proposed by James Jeans and Harold Jeffreys. A massive star passed very close to the early Sun. The hot gas then accumulated and formed the planets. The materials from the less dense rogue star formed the other planets, while that from the sun formed the inner planets. 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