Astronomy Flashcards

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1
Q

Define Photosphere

A

the luminous envelope of a star from which its light and heat radiate

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2
Q

Define Convection Zone

A

A region of turbulent plasma between a star’s core and its visible photosphere at the surface, through which energy is transferred by convection. In the convection zone, hot plasma rises, cools as it nears the surface, and falls to be heated and rise again.

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3
Q

Define flare

A

a brief powerful eruption of particles and intense electromagnetic radiation from the sun’s surface, associated with sunspots and causing disturbances to radio communication on earth

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4
Q

Define nuclear fusion

A

The nuclear PROCESS whereby several small nuclei are combined to make a larger one whose mass is slightly smaller than the sum of the small ones. Nuclear fusion is the reaction that fuels the Sun, where hydrogen nuclei are fused to form helium.

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5
Q

Define nuclear fission

A

a nuclear reaction in which a heavy nucleus splits spontaneously or on impact with another particle, with the release of energy.

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6
Q

Define geocentric

A

having or representing the earth as the center, as in former astronomical systems.

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7
Q

Define chromosphere

A

a reddish gaseous layer immediately above the photosphere of the sun or another star. Together with the corona, it constitutes the star’s outer atmosphere.

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8
Q

Define sunspot

A

a spot or patch appearing from time to time on the sun’s surface, appearing dark by contrast with its surroundings.

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9
Q

Define granule

A

a small compact particle of a substance.

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10
Q

Define red giant

A

a very large star of high luminosity and low surface temperature. Red giants are thought to be in a late stage of evolution when no hydrogen remains in the core to fuel nuclear fusion.

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11
Q

Define electromagnetic spectrum

A

the range of wavelengths or frequencies over which electromagnetic radiation extends.

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12
Q

Define ellipse

A

An ellipse is defined as the locus of all points such that the sum of the distances from two foci to any point on the ellipse is a constant.

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13
Q

Define radius

A

Solar radius is a unit of distance used to express the size of stars in astronomy equal to the current radius of the Sun

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14
Q

Define corona

A

A corona (Latin, ‘crown’) is an aura of plasma that surrounds the Sun and other celestial bodies. The Sun’s corona extends millions of kilometres into space and is most easily seen during a total solar eclipse, but it is also observable with a coronagraph.

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15
Q

Define prominence

A

an eruption of a flamelike tongue of relatively cool, high-density gas from the solar chromosphere into the corona where it can be seen during a solar eclipse or by observing strong spectral lines in its emission spectrum.

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16
Q

Define solar wind

A

the continuous flow of charged particles from the sun that permeates the solar system.

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17
Q

Define white dwarf

A

a small very dense star that is typically the size of a planet.

18
Q

Define coronal mass ejection

A

A coronal mass ejection (CME) is a massive burst of gas and magnetic field arising from the solarcorona and being released into the solar wind, as observed in a coronagraph.

19
Q

Define radiation

A

the emission of energy as electromagnetic waves or as moving subatomic particles, especially high-energy particles that cause ionization.

20
Q

Define nebula

A

a cloud of gas and dust in outer space, visible in the night sky either as an indistinct bright patch or as a dark silhouette against other luminous matter.

21
Q

Define brown dwarf

A

a celestial object intermediate in size between a giant planet and a small star, believed to emit mainly infrared radiation.

22
Q

Define magnetoshere

A

the region surrounding the earth or another astronomical body in which its magnetic field is the predominant effective magnetic field.

23
Q

Define heliocentric

A

measured from or considered in relation to the center of the sun.

24
Q

Define percent error

A

When you calculate results that are aiming for known values, thepercent error formula is useful tool for determining the precision of your calculations .

25
Q

What was the solar system like at the beginning?

A

A big bang of meteors crashed together and made planets. Once plaents were created, moons were pulled in by that planets gravitational force.

26
Q

How did the sun form?

A

As the material drew together, gravity caused it to spin. The spin caused the cloud to flatten into a disk like a pancake. In the center, the material clumped together to form a protostar that would eventually become the sun.

27
Q

How does gravity work?

A

We know from Isaac Newton and his law of gravitation that any two objects in the Universe exert a force of attraction on each other. This relationship is based on the mass of the two objects and the distance between them

28
Q

How has our understanding of gravity changed over time?

A

Ever since Sir Isaac Newton came into this world he has shaped our minds to his three gravitational rules.

29
Q

List three differences between the inner and outer planets.

A
  • Inner planets are fairly small and outer planets are huge!
  • Inner planets have solid surfaces and thin/no atmosphere and outer planets are balls of gas with no surface
  • Inner planets have a greater amount of density and outer planets have a smaller amount of density
30
Q

Namethe planets in order from nearest to the sun to farthest.

A

SUN Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, Pluto

31
Q

Describe the shape of orbits of most people

A

Most planets have oval or circular orbit.

32
Q

Identify the layers of the sun

A
33
Q

How is the energy produced within the sun?

A

Through most of the Sun’s life, energy is produced by nuclear fusion in the core region

34
Q

what elements evolve in the sun?

A

Chemically, about three quarters of the Sun’s mass consists ofhydrogen, whereas the rest is mostly helium, and much smaller quantities of heavier elements, including oxygen, carbon, neon and iron.

35
Q

How does nuclear fusion seem to violate the Law of Conservation of Mass?

A

According to the law of conservation of mass, during any physical or chemical changes, the total mass of the products is equal to the total mass of the reactants. But in nuclear fusion reaction if considered an example, energy that sun emits in its core is due to collision of hydrogen nuclei and formation of helium nuclei. Here conservation of mass is not obeyed as certain part of mass is converted into energy. So, law of conservation of mass is violated here. Then law of conservation must be redefined as: during any physical or chemical change, the total mass of the reactants is equal to the total mass of reactants provided mass has not undergone conversion into energy.

36
Q

Which layer of the sun is considered the surface?

A

The Sun’s visible surface the photosphere is “only” about 5,800 K (10,000 degrees F).

37
Q

Which two layers are the sun’s atmosphere?

A

Chromosphere and corona

38
Q

What is the sun’s hottest layer?

What is the coolest?

A

While the center of the Sun’s core can get as hot as 30 million degrees F, its outer layers cool down. The photosphere, which is outside the core, is the coolest layer. This is as expected, because normally heat passes outwardly from hot to cold.

39
Q

Which layer is visible during a total solar eclipse?

A

During a total solar eclipse some parts of the Sun that we normally can’t see become visible,including the corona (the outermost layer of the sun’s atmosphere).

40
Q

What causes sunspots?

A

They correspond to concentrations of magnetic field that inhibit convection and result in reduced surface temperature compared to the surrounding photosphere.

41
Q

What effects do solar events have on Earth?

A

Well, for one, the weather… All weather systems get their energy from the Sun, ultimately.

Second, life couldn’t exist, as pretty much all plants get their energy from the sun, which in turn goes up the food chain.

Third, the sun can interfere with our spaceborne platforms, as the satellites aren’t shielded as well as we are here on Earth (thank you Magnetic Field and Atmosphere).

42
Q
A