Stars And The Universe Continued
Overzicht
The Sun is just one ordinary star among hundreds of billions in our galaxy, the Milky Way, and the Milky Way is just one galaxy among billions in the Universe. Across these vast distances, measured in light-years, stars are born, shine for ages, and die in spectacular ways.
In this lesson you will learn how galaxies, stars and the Milky Way fit together, what a light-year is and its value in metres, and the full life cycle of a star from a cloud of gas to a white dwarf, neutron star or black hole. You will see how the death of one star seeds the birth of the next.
Doelstellingen
- State that: (a) galaxies are each made up of many billions of stars (b) the Sun is a star in the galaxy known as the Milky Way (c) other stars that make up the Milky Way are much further away from the Earth than the Sun is from the Earth (d) astronomical distances can be measured in light-years, where one light-year is the distance travelled in (the vacuum of) space by light in one year
- [Supplement] Know that one light-year is equal to 9.5 × 1015 m
- [Supplement] Describe the life cycle of a star: (a) a star is formed from interstellar clouds of gas and dust that contain hydrogen (b) a protostar is an interstellar cloud collapsing and increasing in temperature as a result of its internal gravitational attraction (c) a protostar becomes a stable star when the inward force of gravitational attraction is balanced by an outward force due to the high temperature in the centre of the star (d) all stars eventually run out of hydrogen as fuel for the nuclear reaction (e) most stars expand to form red giants and more massive stars expand to form red supergiants when most of the hydrogen in the centre of the star has been converted to helium (f) a red giant from a less massive star forms a planetary nebula with a white dwarf star at its centre (g) a red supergiant explodes as a supernova, forming a nebula containing hydrogen and new heavier elements, leaving behind a neutron star or a black hole at its centre (h) the nebula from a supernova may form new stars with orbiting planets
Lesnotitie
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Lesevaluatie
Gefeliciteerd met het voltooien van de les op Stars And The Universe Continued. Nu je de sleutelconcepten en ideeën, het is tijd om uw kennis op de proef te stellen. Deze sectie biedt een verscheidenheid aan oefeningen vragen die bedoeld zijn om uw begrip te vergroten en u te helpen uw begrip van de stof te peilen.
Je zult een mix van vraagtypen tegenkomen, waaronder meerkeuzevragen, korte antwoordvragen en essayvragen. Elke vraag is zorgvuldig samengesteld om verschillende aspecten van je kennis en kritisch denkvermogen te beoordelen.
Gebruik dit evaluatiegedeelte als een kans om je begrip van het onderwerp te versterken en om gebieden te identificeren waar je mogelijk extra studie nodig hebt. Laat je niet ontmoedigen door eventuele uitdagingen die je tegenkomt; beschouw ze in plaats daarvan als kansen voor groei en verbetering.
- The Sun is a star in the galaxy known as the: A. Andromeda B. Milky Way C. Solar System D. Orion Answer: B
- One light-year is equal to: A. 9.5 x 10^12 m B. 9.5 x 10^15 m C. 3.0 x 10^8 m D. 365 m Answer: B
- A star much more massive than the Sun ends its life as a supernova, leaving behind a: A. white dwarf B. planetary nebula C. neutron star or black hole D. protostar Answer: C
- A stable star is one in which gravity is balanced by: A. the magnetic field B. the outward push from its high core temperature C. the solar wind D. nothing Answer: B
- A star 2.0 light-years away is a distance in metres of about: A. 1.9 x 10^16 m B. 4.75 x 10^15 m C. 9.5 x 10^15 m D. 2.0 m Answer: A
Beschikbaar in de Green Bridge-app
Download de Green Bridge CBT-app op je telefoon of computer voor toegang tot volledige lesnotities, oefenvragen en meer.
Beschikbaar in de Green Bridge-app
Download de Green Bridge CBT-app op je telefoon of computer voor toegang tot volledige lesnotities, oefenvragen en meer.
Aanbevolen Boeken
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