Science Double Award - 4SD0 PearsonEdexcel

Stellar Evolution

Akopọ

Stars are born, they shine for millions or billions of years, and eventually they die. The path a star takes depends on one thing above all: its mass. Our Sun will end quietly as a white dwarf; a star ten times more massive will explode as a supernova.

In this lesson you will learn how to classify stars by colour and temperature, and trace the life cycle of both Sun-like and massive stars from nebula to final remnant.

Awọn Afojusun

  1. Understand how stars can be classified according to their colour
  2. Know that a star's colour is related to its temperature
  3. Describe the evolution of stars of similar mass to the Sun through the stages: nebula, star (main sequence), red giant, white dwarf
  4. Describe the evolution of stars with a mass larger than the Sun

Akọ̀wé Ẹ̀kọ́

Every star you see in the night sky is at a different stage of its life. Some are young and hot, burning through hydrogen at a furious rate. Others are old and swollen, running out of fuel. The colour of a star tells you its surface temperature, and its mass determines how it will eventually die.

O wa lori ohun elo Green Bridge

Gba ohun elo Green Bridge CBT sori foonu tabi kọmputa rẹ lati ri awọn akọsilẹ ẹkọ ni kikun, awọn ibeere adaṣe, ati diẹ sii.

Awọn akọsilẹ ẹkọ ni kikun pẹlu awọn aworan apejuwe
Oluranlọwọ ẹkọ ti AI ṣe agbara rẹ
Kọ ẹkọ laisi intanẹẹti, nigbakugba, nibikibi
O wa lori Android, Windows, macOS, ati Linux

Ìdánwò Ẹ̀kọ́

Oriire fun ipari ẹkọ lori Stellar Evolution. Ni bayi ti o ti ṣawari naa awọn imọran bọtini ati awọn imọran, o to akoko lati fi imọ rẹ si idanwo. Ẹka yii nfunni ni ọpọlọpọ awọn adaṣe awọn ibeere ti a ṣe lati fun oye rẹ lokun ati ṣe iranlọwọ fun ọ lati ṣe iwọn oye ohun elo naa.

Iwọ yoo pade adalu awọn iru ibeere, pẹlu awọn ibeere olumulo pupọ, awọn ibeere idahun kukuru, ati awọn ibeere iwe kikọ. Gbogbo ibeere kọọkan ni a ṣe pẹlu iṣaro lati ṣe ayẹwo awọn ẹya oriṣiriṣi ti imọ rẹ ati awọn ogbon ironu pataki.

Lo ise abala yii gege bi anfaani lati mu oye re lori koko-ọrọ naa lagbara ati lati ṣe idanimọ eyikeyi agbegbe ti o le nilo afikun ikẹkọ. Maṣe jẹ ki awọn italaya eyikeyi ti o ba pade da ọ lójú; dipo, wo wọn gẹgẹ bi awọn anfaani fun idagbasoke ati ilọsiwaju.

  1. A blue star has a surface temperature that is: A) Lower than a red star B) The same as a red star C) Higher than a red star D) Unrelated to colour Answer: C
  2. After the main sequence, a Sun-like star becomes a: A) Supernova B) Red giant C) Black hole D) Neutron star Answer: B
  3. The final remnant of a Sun-like star is a: A) Black hole B) Neutron star C) White dwarf D) Red supergiant Answer: C
  4. A supernova occurs in the life cycle of: A) Any star B) Only Sun-like stars C) Only massive stars D) Only red dwarfs Answer: C
  5. Stars are born in: A) White dwarfs B) Black holes C) Nebulae D) Neutron stars Answer: C

O wa lori ohun elo Green Bridge

Gba ohun elo Green Bridge CBT sori foonu tabi kọmputa rẹ lati ri awọn akọsilẹ ẹkọ ni kikun, awọn ibeere adaṣe, ati diẹ sii.

Awọn akọsilẹ ẹkọ ni kikun pẹlu awọn aworan apejuwe
Oluranlọwọ ẹkọ ti AI ṣe agbara rẹ
Kọ ẹkọ laisi intanẹẹti, nigbakugba, nibikibi
O wa lori Android, Windows, macOS, ati Linux

O wa lori ohun elo Green Bridge

Gba ohun elo Green Bridge CBT sori foonu tabi kọmputa rẹ lati ri awọn akọsilẹ ẹkọ ni kikun, awọn ibeere adaṣe, ati diẹ sii.

Awọn akọsilẹ ẹkọ ni kikun pẹlu awọn aworan apejuwe
Oluranlọwọ ẹkọ ti AI ṣe agbara rẹ
Kọ ẹkọ laisi intanẹẹti, nigbakugba, nibikibi
O wa lori Android, Windows, macOS, ati Linux

Ṣe Adaṣe Awọn Ibeere Idanwo Adaṣe

Ṣe o fẹ ṣe adaṣe awọn ibeere idanwo adaṣe nipa Stellar Evolution? Ṣe igbasilẹ ohun elo Green Bridge CBT lati wọle si awọn ibeere idanwo adaṣe ati awọn ayẹwo adaṣe kikun fun koko-ọrọ yii.

Ṣe igbasilẹ ohun elo naa lori Google Playstore

Gbogbo ohun ti o nilo lati ṣe dara julọ ninu JAMB, WAEC ati NECO.

Green Bridge CBT Mobile App
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Fiwọn 1200 Awọn akọsilẹ Ẹkọ ju.
Atilẹyin Aisinipo - Kọ ẹkọ Nigbakugba, Nibi gbogbo
Tẹ̀dí Green Bridge
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