Facts (GCSE) Flashcards

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1
Q

Telescopes found fuzzy objects?

A

Nebulae.

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2
Q

Intergalactic distances are usually measured in:

A

Mega Parsecs (Mpc)

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3
Q

All objects(stars too) emit a continuous range of:

A

electromagnetic radiation.

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4
Q

The luminosity and peak frequency of all hot objects(including stars) changes with:

A

Temperature.

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5
Q

Ionisation =

A

The removal of electrons from atoms.

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6
Q

The line spectra is produced by:

A

The movement of electrons in the atoms.

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7
Q

The spectra of a star contains:

A

Specific spectral lines, which can tell us what chemical elements are in the star.

Hydrogen and helium are in all stars.

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8
Q

H + H + brought close together to fuse =

A

He + energy

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9
Q

Compressing gas in a protostar will raise its

A

Temperature

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10
Q

Hotter core

A

Fusion

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11
Q

(Hotter core ->) radiative zone

A

Energy transported to the surface by photons.

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12
Q

(Hot core -> Radiative zone ->) Convective zone

A

Energy to the surface through convection.

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13
Q

(Hot core -> Radiative zone -> Convective zone ->) Photosphere

A

Energy is radiated into space.

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14
Q

Smaller stars become:

A

Red giants, when the core H is depleted.

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15
Q

Larger stars become:

A

Red supergiants, when the core H is depleted.

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16
Q

Red giants and supergiants will then both fuse helium atoms together to form heavier elements

A

C, N, O in order to make more energy.

17
Q

Major optical and infrared observatories on Earth are mostly in

A

Chile, Hawaii, Australia, the Canary Islands.

18
Q

To collect weak radiation from distant sources,

A

You’ll need large telescopes.

19
Q

Telescopes revealed that the Milky Way consisted of many stars =

A

Realisation that the sun is part of the Milky Way galaxy.