(unit 1 chp1) origin & formation of the universe

0.0(0)
Studied by 10 people
call kaiCall Kai
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
GameKnowt Play
Card Sorting

1/53

encourage image

There's no tags or description

Looks like no tags are added yet.

Last updated 12:26 PM on 4/30/26
Name
Mastery
Learn
Test
Matching
Spaced
Call with Kai

No analytics yet

Send a link to your students to track their progress

54 Terms

1
New cards

the understanding of the origin, evolution and structure of of the universe.

cosmology

2
New cards

reveals that ancient Indians believed that the universe had an origin and pondered about how and where the world and everything in it began.

The Hymn of Creation in the Rigveda

3
New cards

What was the first thing that existed based on the Hymn of Creation in the Rigveda?

Darkness

4
New cards

What was the second thing that existed based on the Hymn of Creation in the Rigveda?

Desire

5
New cards

they believed that the cosmos has always existed.

ancient Greeks

6
New cards

beliefs of ancient Greeks

  • the cosmos was neither created nor is it perishable

  • it was timeless and infinite in extent.

  • the universe has a center 

7
New cards

He first proposed that Earth was not the center of the universe, but a central fire around which the sun, moon, the planets, and other celestial objects revolved uniformly.

Philolaus (470-385 B.C.)

8
New cards

He supported the idea of Philolaus but suggested that the central fire was the sun.

Aristarchus (310-230 B.C.)

9
New cards

He proposed the Heliocentric model of the universe.

Aristarchus

10
New cards

He proposed the center of the cosmos is Earth.

Aristotle

11
New cards

Aristotle’s geocentric cosmology dominated all studies and speculations about the arrangement of the cosmos until

16th Century

12
New cards

popularized and advanced the geocentric model

Claudius Ptolemy

13
New cards

heavenly bodies revolved around a stationary Earth placed at the center of the universe.

Geocentric model

14
New cards

designed the Ptolemaic model

Claudius Ptolemy

15
New cards

Ptolemy’s design even tried to explain the planetary and solar motions through different paths known as:

  • epicycle

  • deferent

  • eccentric

16
New cards

the planetary and solar motions through different paths known as epicycle, deferent and eccentric. A dominant model of the universe until the scientific revolution in the 16th century.

Ptolemaic model

17
New cards

During these centuries, the western worldview the dominated the world of science projected a history that directed toward progress.

17th and 18th century

18
New cards

Who proposed the Big Bang Theory?

Georges Lemaitre

19
New cards

Who proposed the general relativity?

Albert Einstein

20
New cards

He believed that the universe was a finite and static four-dimensional closed sphere. The universe was homogeneous, where matter spread smoothly throughout space.

Albert Einstein

21
New cards
  • the most accepted theory today

  • the universe is approximately 13.7 billion years old.

  • cosmologists who supported this theory divided the history of the universe into a series of eras or time periods.

Big Bang Theory

22
New cards

Eras of the Big Bang Theory

  1. The Planck Era

  2. The Grand Unified Theory (GUT) Era

  3. Electroweak Era

  4. Particle Era

  5. The Era of Nucleosynthesis

  6. Era of Nuclei

  7. Era of Atoms and Galaxies

23
New cards

Enumerate the pieces of evidence in testing earlier theories:

  1. Mass Distribution

  2. Angular Momentum Distribution

  3. Shape and alignment of orbits

  4. Chemical Composition

24
New cards

the mass of the system is not evenly distributed. Most of the mass is concentrated in the sun.

Mass Distribution

25
New cards

or the tendency to rotate is concentrated more among the planets instead of the sun.

Angular momentum distribution

26
New cards

the planets moved in nearly circular orbits that nearly align with the equator of the sun in the same direction.

Shape and Alignment of Orbits

27
New cards

the planets and the sun have similar chemical compositions, although varying in proportions.

Chemical composition

28
New cards

CMBR

Cosmic Microwave Background Radiation

29
New cards

who accidentally proved the CMBR

Arno Penzias and Robert Wilson

30
New cards

this is the afterglow of the Big Bang Theory

(CMBR) Cosmic Microwave Background Radiation

31
New cards

theory of cosmos

Hubble

32
New cards

This shocked a nearby interstellar system and triggered the collapse of a solar nebula.

supernova

33
New cards

pancake-shpaed circumstellar disk of dust and gas known as the?

protoplanetary disk

34
New cards

particles in the protoplanetary disk started to collide and form ___, which led go a series of formations of planets in the solar system.

planetesimals

35
New cards

the planetesimals were also assimilating other materials in yheir surroundings. this is known as

accretion

36
New cards

terrestrial planets

  • mercury

  • venus

  • earth

  • mars

37
New cards

the icy planetesimals have a gravitational force stronv enough to capture the abundant hydrogen and helium gases within the solar nebula. this process is called?

nebular capture

38
New cards

large jovian planets

  • jupiter

  • saturn

  • neptune

  • uranus

39
New cards

the outermost layer of a terrestrial planet. it is composed of igneous, metamorphic, and sedimentary rocks.

crust

40
New cards

two types of crust

  • continental

  • oceanic

41
New cards

is composed primarily of basalt, diabase, and gabbro.

oceanic crust

42
New cards

is mostly composed if rocks less dense than the other type of crust, it includes granitez silicates, and aluminum.

continental crust

43
New cards

the section comprising the crust and the upper portion of the mantle, covering a depth of about 100 km

lithosphere

44
New cards

the rock shell surrounding the outer core of other planets.

mantle

45
New cards

thickest layer of Earth

mantle

46
New cards

extends from the crust to a depth of about 410 km and is often described to comprise two regions: the lithosphere and the asthenosphere.

upper mantle

47
New cards

is the section beneath the lithosphere that reaches to a depth of around 410 km

asthenosphere

48
New cards

these plates are said to float above the asthenosphere

lithospheric plates

49
New cards

this portion is hotter and denser than the upper mantle, but its rock composition is more solid due to the intense pressure.

lower mantle

50
New cards

is where rocks undergo significant transformations and become denser.

transition zone

51
New cards

the central layer of the planet, divided into inner and outer portions

Core

52
New cards

is composed mostly of metals, particularly solid iron and nickel. this portion is solid.

inner core

53
New cards

the inner core is surrounded by the liquid iron, which has a thickness of 2,270 km. this portion is liquid.

outer core

54
New cards

the relative measure of the increase in Earth's interior heat and pressure.

geothermal gradient