Photo AI
Question 3
3. The Universe (a) Which row of the table shows these objects in the correct order of size? Put a cross (X) in the box next to your answer. | ... show full transcript
Step 1
Step 2
Answer
The images produced by telescopes on Earth are less clear due to atmospheric interference. The Earth's atmosphere can distort light from celestial objects due to turbulence, dust, and moisture, which results in reduced clarity. In contrast, telescopes in space are free from these atmospheric effects, allowing for clearer and more stable images.
Step 3
Answer
The redshifts observed from galaxies 1 and 2 indicate that both galaxies are moving away from us. This movement suggests that the universe is expanding. The greater the redshift, the faster a galaxy is receding, which can be used to estimate its distance from us.
Step 4
Answer
For stars much more massive than the Sun, the process begins similarly with the formation of a protostar amidst a nebula. As the protostar gathers mass, it eventually enters the main sequence phase where it fuses hydrogen into helium. Once the hydrogen is depleted, the star expands into a supergiant. After this phase, it undergoes a supernova explosion. Depending on the remaining mass, the remnants may form a neutron star or, if massive enough, collapse into a black hole. It is important to note that more massive stars have shorter lifespans due to the rapid consumption of fuel.
Report Improved Results
Recommend to friends
Students Supported
Questions answered
1.1 Energy Changes in a System
Physics - AQA
1.2 National & Global Energy Resources
Physics - AQA
2.1 Current, Potential Difference & Resistance
Physics - AQA
2.2 Series & Parallel Circuits
Physics - AQA
2.3 Energy Transfers
Physics - AQA
2.4 Static Electricity
Physics - AQA
3.1 Changes of State & the Particle Model
Physics - AQA
3.2 Internal Energy & Energy Transfers
Physics - AQA
3.3 Particle Model & Pressure
Physics - AQA
4.1 Atoms & Isotopes
Physics - AQA
4.2 Atoms & Nuclear Radiation
Physics - AQA
4.3 Hazards & Uses of Radioactive Emissions & of Background Radiation
Physics - AQA
4.4 Nuclear Fission & Fusion
Physics - AQA
5.1 Forces & their Interactions
Physics - AQA
5.2 Work Done & Energy Transfer
Physics - AQA
5.3 Forces & Elasticity
Physics - AQA
5.4 Moments, Levers & Gears
Physics - AQA
5.5 Pressure & Pressure Differences in Fluids
Physics - AQA
5.6 Describing Motion
Physics - AQA
5.7 Newton's Laws of Motion
Physics - AQA
5.8 Stopping Distances
Physics - AQA
5.9 Momentum
Physics - AQA
6.1 Waves in Air, Fluids & Solids
Physics - AQA
6.2 Electromagnetic Waves
Physics - AQA
6.3 Optics
Physics - AQA
6.4 Black Body Radiation
Physics - AQA
7.1 Permanent & Induced Magnetism, Magnetic Forces & Fields
Physics - AQA
7.2 The Motor Effect
Physics - AQA
7.3 Induced Potential, Transformers & the National Grid
Physics - AQA
8.1 Solar system, Stability of Orbital Motions & Satellites
Physics - AQA
8.2 Red-shift
Physics - AQA