Geschreven door studenten die geslaagd zijn Direct beschikbaar na je betaling Online lezen of als PDF Verkeerd document? Gratis ruilen 4,6 TrustPilot
logo-home
Tentamen (uitwerkingen)

Earth Science 1086 Midterm 1(complete 2022/2023

Beoordeling
-
Verkocht
1
Pagina's
5
Cijfer
A+
Geüpload op
19-08-2022
Geschreven in
2022/2023

Law, Theory, Hypothesis Hypothesis: educated guess with observation. -WHY Theory: summarizes hypothesis by testing. - WHY Law: explains observations - HOW Singularity an area in space-time where gravitational force is so high, all known laws of physics break down. Evidence of Big Bang - Three Pillars of Proof 1. Hubble's Law 2. characteristics of cosmic microwave background radiation 3. abundance of light elements 1. Hubbles Law - there are many galaxies - the universe is explaining - measure distance in space - v=Hod Doppler Shift The apparent change in wavelengths. 2. Cosmic Background Radiation As the universe expanded it cooled 3. Abundance of Light Elements - hydrogen 75%, helium 25%, lithium - observed abundance can be explained if they ORIGINATED FROM ONE SINGLE RATIO OF THE FIRST SUB ATOMIC PARTICLE OF MATTER Shapes of the universe 1. sphere - closed, finite size, contract in a "big crunch" 2. saddle shape - open, negative curve, expansion rate never reaches 0. 3. flat - can expand/contract forever, no boundaries, reaches 0. Conventional Matter stars, planets, asteroids, comets Dark Matter - cannot see as it gives no energy - can detect its gravitational attraction - 27% of matter Dark Energy - Repels matter - controls expansion of space - 70% of universe Age of universe 1. radioactivity 2. cosmic microwave background radiation 3. hubbles expansion constant Radioactivity breakdown of elements. Determines universe age by : a) observing components of gasses around the stars. b) knowing radioactive processes. c) knowing time factors involved in breaking down a component. How old is the universe? 13.8 Years based on CMBR Model Light Years measure distances in space. You are looking at a star that started its journey 1 million years ago. Measuring Light years - 0 to 500 trigonometric parallax: object is at a different place relative to background. Measuring Light years - 500 to 500 million Hertzprung Rusell DIagram: matches brightness of stars compared to their temperature (colour). Distance of Apparent brightness Calculation AB=Intrinsic Brightness/(4pidistance^2) Cepheids stars with pulsing brightness that peaks The Local Group the Milky way galaxy, the andromeda galaxy, the triangulum galaxy Density mass per unit of volume supernova explosive death of a massive star Nebular Hypothesis suggests that the solar system formed over a brief span of time from a giant nebula (cloud of interstellar gas). Fusion reactions releases more energy to create a star. (Heat of Gas). Red Giant Dying Star, sun loses mass and runs out of hydrogen fuel. Momentum measure of an objects tendency to move at a constant speed along a straight path. Angular Momentum measure of the amount of spin of an object. Conservation of angular momentum if no outside force acts on a spinning object, the objects angular momentum will not change with time. Dew Point temperature to which air must be cooled to reach its water saturation Refractory Elements elements that do not readily respond to heat Jupiter vs Mercury When jupiter formed EVERYTHING condensed, whereas where mercury formed only HEAVIER elements condensed. Magin Broom leftover gasses were swept out from solar win T Tauri Stars very strong winds Geocentric Model Earth is at the centre Heliocentric Model Sun is at the centre Pythagorus/Plato put earth at the centre, objects rotated slowly east depending on how far they were from earth Aristarchus put sun in the centre Ptolemy put earth in the centre, placed all other planets on moving spheres. Catholic church supported. Copernicus Put Sun in the centre, earth rotated sun. Church would not publish Tycho wanted to keep copernicus, sun revolves earth and drags the planets with it Kepler planets were pushed into the orbits by the sun periphelion point of nearest approach of a planet to the sun. aphelion point of greatest separation. Galileo Galilei first to observe the planets through a telescope convinced copernicus was right went to trial for arguing 8 planets Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune 5 dwarf planets Ceres Pluto Eris Hamea Makemake Photosphere visible outer layer represents depth within that gas (most inner layer) Chromosphere outside photosphere, humans can't see (middle layer). Has prominences and flares Corona outermost region, can only see in a solar eclipse The Genesis Experiment suns makeup is mostly hydrogen and helium. Mission is to capture particles of solar wind. Solar wind made of Plasma Aurora visual effect of collisions of light elements. Borealis (north) Australis (south) White Dwarf sun will blow off its outer envelope for its core to cool Black Dwarf when the sun stops glowing Telescope Types Refractor (glass), Reflector (mirror) Asteroid belt separates terrestrial planets fo

Meer zien Lees minder
Instelling
Vak

Voorbeeld van de inhoud

Earth Science 1086 Midterm 1
Law, Theory, Hypothesis - Answer Hypothesis: educated guess with observation. -WHY

Theory: summarizes hypothesis by testing. - WHY

Law: explains observations - HOW

Singularity - Answer an area in space-time where gravitational force is so high, all
known laws of physics break down.

Evidence of Big Bang - Three Pillars of Proof - Answer 1. Hubble's Law
2. characteristics of cosmic microwave background radiation
3. abundance of light elements

1. Hubbles Law - Answer - there are many galaxies
- the universe is explaining
- measure distance in space
- v=Hod

Doppler Shift - Answer The apparent change in wavelengths.

2. Cosmic Background Radiation - Answer As the universe expanded it cooled

3. Abundance of Light Elements - Answer - hydrogen 75%, helium 25%, lithium
- observed abundance can be explained if they ORIGINATED FROM ONE SINGLE
RATIO OF THE FIRST SUB ATOMIC PARTICLE OF MATTER

Shapes of the universe - Answer 1. sphere - closed, finite size, contract in a "big
crunch"
2. saddle shape - open, negative curve, expansion rate never reaches 0.
3. flat - can expand/contract forever, no boundaries, reaches 0.

Conventional Matter - Answer stars, planets, asteroids, comets

Dark Matter - Answer - cannot see as it gives no energy
- can detect its gravitational attraction
- 27% of matter

Dark Energy - Answer - Repels matter
- controls expansion of space
- 70% of universe

Age of universe - Answer 1. radioactivity
2. cosmic microwave background radiation

, 3. hubbles expansion constant

Radioactivity - Answer breakdown of elements. Determines universe age by :
a) observing components of gasses around the stars.
b) knowing radioactive processes.
c) knowing time factors involved in breaking down a component.

How old is the universe? - Answer 13.8 Years based on CMBR Model

Light Years - Answer measure distances in space. You are looking at a star that started
its journey 1 million years ago.

Measuring Light years - 0 to 500 - Answer trigonometric parallax: object is at a different
place relative to background.

Measuring Light years - 500 to 500 million - Answer Hertzprung Rusell DIagram:
matches brightness of stars compared to their temperature (colour).

Distance of Apparent brightness Calculation - Answer AB=Intrinsic
Brightness/(4*pi*distance^2)

Cepheids - Answer stars with pulsing brightness that peaks

The Local Group - Answer the Milky way galaxy, the andromeda galaxy, the triangulum
galaxy

Density - Answer mass per unit of volume

supernova - Answer explosive death of a massive star

Nebular Hypothesis - Answer suggests that the solar system formed over a brief span of
time from a giant nebula (cloud of interstellar gas).

Fusion reactions - Answer releases more energy to create a star. (Heat of Gas).

Red Giant - Answer Dying Star, sun loses mass and runs out of hydrogen fuel.

Momentum - Answer measure of an objects tendency to move at a constant speed
along a straight path.

Angular Momentum - Answer measure of the amount of spin of an object.

Conservation of angular momentum - Answer if no outside force acts on a spinning
object, the objects angular momentum will not change with time.

Geschreven voor

Vak

Documentinformatie

Geüpload op
19 augustus 2022
Aantal pagina's
5
Geschreven in
2022/2023
Type
Tentamen (uitwerkingen)
Bevat
Vragen en antwoorden

Onderwerpen

$10.49
Krijg toegang tot het volledige document:

Verkeerd document? Gratis ruilen Binnen 14 dagen na aankoop en voor het downloaden kun je een ander document kiezen. Je kunt het bedrag gewoon opnieuw besteden.
Geschreven door studenten die geslaagd zijn
Direct beschikbaar na je betaling
Online lezen of als PDF

Maak kennis met de verkoper

Seller avatar
De reputatie van een verkoper is gebaseerd op het aantal documenten dat iemand tegen betaling verkocht heeft en de beoordelingen die voor die items ontvangen zijn. Er zijn drie niveau’s te onderscheiden: brons, zilver en goud. Hoe beter de reputatie, hoe meer de kwaliteit van zijn of haar werk te vertrouwen is.
EvaTee Phoenix University
Volgen Je moet ingelogd zijn om studenten of vakken te kunnen volgen
Verkocht
5213
Lid sinds
4 jaar
Aantal volgers
3568
Documenten
55860
Laatst verkocht
4 uur geleden
TIGHT DEADLINE? I CAN HELP

Many students don\'t have the time to work on their academic papers due to balancing with other responsibilities, for example, part-time work. I can relate. kindly don\'t hesitate to contact me, my study guides, notes and exams or test banks, are 100% graded

3.8

951 beoordelingen

5
453
4
167
3
173
2
48
1
110

Recent door jou bekeken

Waarom studenten kiezen voor Stuvia

Gemaakt door medestudenten, geverifieerd door reviews

Kwaliteit die je kunt vertrouwen: geschreven door studenten die slaagden en beoordeeld door anderen die dit document gebruikten.

Niet tevreden? Kies een ander document

Geen zorgen! Je kunt voor hetzelfde geld direct een ander document kiezen dat beter past bij wat je zoekt.

Betaal zoals je wilt, start meteen met leren

Geen abonnement, geen verplichtingen. Betaal zoals je gewend bent via iDeal of creditcard en download je PDF-document meteen.

Student with book image

“Gekocht, gedownload en geslaagd. Zo makkelijk kan het dus zijn.”

Alisha Student

Bezig met je bronvermelding?

Maak nauwkeurige citaten in APA, MLA en Harvard met onze gratis bronnengenerator.

Bezig met je bronvermelding?

Veelgestelde vragen