Chapter 5: Geometry of the Solar System Flashcards

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1
Q

How do camera shop owners get rich from people’s passing interest in astronomy? What can you buy instead that is just as good and cheaper?

A

by touting the great properties of small telescopes - they are actually a pain to use and not much better than binoculars.

You can use binoculars and clamp to connect them to a tripod, which is much cheaper

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2
Q

What is the use of an optical telescope?

A

optical telescope gathers light and allows you to examine an image at a focal point

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3
Q

Why do even the best optics have a limited resolution in telescopes?

How does the atmosphere affect the image? Why do stars twinkle?

A

because of the wave nature of light

ie. water waves bend when they strike the edge of a barrier - light waves do the same

the twinkling of stars comes from the turbulence in the air that makes up the atmosphere – the atmosphere basically acts as a huge distorting lens.

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4
Q

What are the 2 basic type of astronomical telescopes

A
  1. refractors
  2. reflectors
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5
Q

What are refractors vs reflectors

A

refractors collect light. by means of a glass lens (or combination of lenses)

reflectors colect light with a curved mirror

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6
Q

What is the aperature of a telescope determined by ?

A

aperature of any telescope is determined by the diameter of the glass lens or mirror

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7
Q

How is the magnification done in any telescope?

A

done by a smaller lens known as an eyepiece or ocular

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8
Q

What allows a higher magnification to be used in a telescope?

A

larger aperatures (larger diameter of the gass or mirror) because more light can be collected and therefore a higher magnification can be used

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9
Q

What are the 2 largest telescopes in the world?

A

the two Keck telescopes mounted on Mauna Kea, Hawaii

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10
Q

What discovery determined that stars other than the sun have planets (where, which telescope, when, what did they observe)

A

It was the Keck observatory in 1999 that observed the transit of a massive planet in front of it’s star 153 light years away - confirming or the first time that stars other than the Sun have planets

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11
Q

Describe what is depicted in this image

A

This is a refractor telescope.

the primary lens is a convex spherical lens which collects and concentrates the light - parallel light rays from the star are concentrated onto a smaller area called the eyepiece

the eyepiece is a concave lens which makes th concentrades light rays parallel again

the focal point is behind the eyepiece

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12
Q

Describe what is depicted in this image

A

this is a reflector telescope

the light from a celestial body bounces off a primary (objective) mirror onto a secondary mirror, which reflects the light into the eyepiece.

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13
Q

What instruments does Canada use for observing space

A

a number of joint venture instruments

best known: the Canada-France-Hawaii Telescope (CFHT) on Mauna Kea, Hawaii

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14
Q

What is depicted in this Image? What is it called, how many light years away? What does the red vs. green depict? What telescope was it taken from and when?

A

This is an image taken by the CFHT in 2004

This is the Lagoon Nebula, ~5000 light years away
* it is home to a cluster of very young stars, developing among globules and pillars of gas

the red colour depicts hydrogen
the green depicts oxygen

Note: You can see the Lagoon Nebula even without a telescope close to the constellation of Sagittarius

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15
Q

For what reason do we have telescopes orbiting outside earth’s atmosphere? The most famous one?

A

any telescope on earth has to make some compensation for earth’s atsmosphere and the distortions it creates

Thus the Hubble Space Telescope (HST) orbits some 600km above earth

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16
Q

Describe the characteristics of the HST:

  • where does it orbit
  • the size and shape
  • is fitted with …?
  • how often is it operated and how?
A

Hubble Space Telescope, which orbits ~600km above earth, has a 2.44 m mirror mounted inside a hollow tube (to avoid glare from the sun, moon and earth)

it is fitted with a great array of signal detectors

it is operated 24 hours a day remotely from earth

The Hubble Space Telescope
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17
Q

When was the HST launched? How many service calls has it had since then and how have they improved it?

What was installed during the last service call in 2009?

Why did NASA ban any further service calls to HST? What efforts were made to prolong its life in light of this?

A

Hubble Space Telescope was launched in 1990 and has had 5 service calls since; each scientific package that has been replaced on those calls has increased the telescope’s power by something like 10 times

The last service call in 2009 installed a wide field camera to see 3 types of light and a Cosmic Origins Spectrograph which breaks light into its component colours.

NASA announced they are banning any further service calls to HST because new safety regulations (arising from the Shuttle Columbia disaster) prohibit it.

In the last service call, it was replaced with all new parts to prolong its life as long as possible before it eventually falls to earth.

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18
Q

What is the JWST?

When is it scheduled to launch? Characteristics?

A

the James Webb Space Telescope is a replacement for the HST, scheduled to be launched into orbit around earth in 2018

this telecope will have a 6.5 meter in diameter mirror and a “sunshield the size of a tennis court” to allow astronomers to find galaxies and planetary systems.

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19
Q

The use of non optical telescopes is sometimes called what?

A

Invisible astronomy

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20
Q

All telescopes gather energy

what range of wavelengths of energy is gathered by optical telescopes vs. non optical telescopes

A

Optical telescopes gather wavelengths of energy between 400nm and 700nm - the very tiny band of energy that is visible light

Non optical telescopes gather wavelength energy beyond the visible spectrum (gamma rays, X-rays, ultraviolet, infrared, and radio waves)

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21
Q

Describe the detectable energy spectrum from the shortest to longest wavelengths

A

gamma rays → X-Rays → Ultra-violet → Visible Light → infared → radio waves

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22
Q

What was the first non optical telescope built to detect? When?

Since then what range have dishes been built to capture?

A

first non optical telescope build to collect radio waves in 1931

Since then, dishes have been built to collect every other possible range of detectable energy

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23
Q

What type of telescopes are carried on Rockets, satellites and space probes? Why?

A

they may carry optical cameras.
virtually all of them carry at least one type of non-optical telescope.
These allow scientists to gather data from wavelengths that Earth-based telescopes cannot easily capture, often due to atmospheric interference.

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24
Q

What is needed in order to insert a satellite (like the HST) into orbit around Earth?

A

you need a rocket which will deliver orbital velocity – just enough velocity to place the satellite in a position that exactly balances gravity’s pull on the satellite with the inertia of the satellite’s motion

25
Q

What is orbital velocity and what does it depend on ?

A

Orbital velocity is the speed required for a satellite to stay in orbit around a planet (like Earth) without falling back down or flying off into space.

It occurs when the satellite’s inertia (its tendency to move in a straight line) perfectly balances the pull of gravity from the planet.

The orbital velocity depends on the altitude it is placed above earth:

  • If a satellite is placed closer to Earth, it needs a higher orbital velocity to counteract the stronger gravitational pull.
  • If the satellite is farther from Earth, a lower orbital velocity is sufficient since gravity weakens with distance.
26
Q

In the computer age, modern technology has allowed us to create incrediby sensitive detection systems. How?

A

Modern technology has allowed for the networking of many radio wave receivers to create incredibly sensitive detection systems. This leads to higher resolution and better sensitivity to faint signals from distant objects in space.

27
Q

Describe the Lovell Telescope.
Size?
Where?
When was it built?
What purpose was it famously used for?
Is it still in use today?

A

One of the earliest large radio telescopes was the Lovell Telescope – a 76-meter dish at Jodrell Bank in the UK, built in 1957.

It was famously used to track Russia’s Sputnik 1 satellite.

Though it has been upgraded many times, it is still in use today and often works in conjunction with other telescopes to enhance resolution.

The Lovell Telescope at Jodrell Bank, UK
28
Q

What is a geostationary satellite? At what altitude and velocity? What is the point of it?

A

Geostationary satellites match earth’s rotation so it stays in the same spot above earth at all times. therefore it has to stay in orbital velocity.

We can maintain a satellite in geostationary orbit at, say, 35,786 km above Earth with a velocity of 11,300 km/h.

At this velocity, it will make exactly 1 revolution of Earth every 24 hours - it matches earth’s rotation so it stays in the same spot above earth at all times.

This simplifies signal collection from ground-based receivers, therefore they are used for communications, like TV satellites.

29
Q

What is escape velocity?

A

the minimum velocity needed for an object to just overcome Earth’s gravitational attraction, essential for sending things into space.

you would need to have a rocket attain escape velocity if you want to send it to mars for example - obviously requires more power than orbital velocity

30
Q

What mnemonic was used to remember the planets before 2006?

A

“My Very Excellent Mother Just Served Us Nine Pizzas” to list the nine planets in order from the sun outward:
Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, and Pluto.

31
Q

What are the terrestrial planets?

do they have satellites?

A

The four dense, rocky planets closest to the Sun: Mercury, Venus, Earth, and Mars.

two of these have satellites (earth and mars) and 2 do not (venus and mercury)

32
Q

What are the jovian or gas giant planets?

describe their composition and do they have satellites?

A

The four large, low-density planets far from the Sun: Jupiter, Saturn, Uranus, and Neptune.

they are composed mostly of hydrogen and helium and surrounded by rings, and many many satellites

33
Q

What lies between the terrestrial and jovian planets?

A

The asteroid belt, a region filled with small rocky objects, including Ceres, the largest asteroid.

34
Q

Traditionally, we have divided the objects of the solar system into 4 categories

A
  1. Planets
  2. their satellites
  3. asteroids (dense objects orbiting the Sun that are much smaller than planets)
  4. Comets (icy objects orbiting in highly eccentric patterns)
35
Q

Why was Pluto reclassified as a dwarf planet in 2006?

Where is pluto? When was it discovered?

A

Pluto is too small, too dense, has a satellite (Charon) almost as large as itself, and follows an eccentric orbit, making it different from the other planets.

pluto is out past the gas giants (jovian planets) and was discovered in 1930.

36
Q

What is the Kuiper Belt, and what objects are found there?

A

A thick band of icy bodies beyond Pluto, home to icy objects like Eris and Sedna, which may be the source of many comets.

37
Q

What is the Oort Cloud?

A

A hypothetical region marking the outer limits of the Solar System, thought to be an enormous belt of of icy bodies and the source of many comets, though it has not been directly observed.

38
Q

How did the discovery of Eris in 2005 affect the number of planets?

A

In 2003, someone spotted an orbiting object 27% larger than pluto and ~3x further away from the Sun than pluto.

Finally, by 2005, they had clearly identified it and named it Eris.

this sparked debate about the number of planets, as more distant orbiting objects were discovered, leading to the need for a formal definition of “planet.”

39
Q

What was the initial definition of a planet proposed by the International Astronomical Union (IAU) in 2006? (that was rejected)

A

A planet is a celestial body that:

a) has sufficient mass for its self-gravity to overcome rigod body forces so that it assumes a nearly round shape

b) is in orbit about a star, and is neither a star nor a satellite of a planet

40
Q

After many rejected drafts, and desperation to adopt something, the IAU reduced consideration to only our solar system and the following scheme for defining celestial bodies was passed in 2006:

A
  • A planet is a celestial body that (a) is in orbit around the sun (b) has sufficient mass for its self gravity to overcome rigod body forces so that it assumes a nearly round shape, and (c) has cleared the neighborhood around its orbit
  • a dwarf planet is a celestial body that (a) is in orbit around the sun (b) has a sufficient mass for its self-gravity to overcpome rigid body forces so that it assumes a nearly round shape, (c) has not cleared the neighborhood around its orbit and (d) is not a satellite
  • All other objects, except satellites, orbiting the Sun shall be referred to as ‘Small Solar System Bodies’

Note: Small Solar System Bodies that orbit (at least part of the time) past the orbit of Neptune have been termed “Trans-Neptunian Objects” (TNOs)

41
Q

What are Trans-Neptunian Objects (TNOs)?

A

Small Solar System Bodies that orbit (at least part of the time) past the orbit of Neptune have been termed “Trans-Neptunian Objects”

Pluto fits this defintion as well as dwarf planet defintion.
Charon (Pluto’s partner) is left out of things if it is considered a satellite, and otherwise is considered a TNO

42
Q

What mnemonic replaced the old one after Pluto’s reclassification? (for the updated classification passed in 2006)

A

“My Very Evil Mother Just Served Us Nectarines,” excluding Pluto from the list of planets.

43
Q

What are “plutoids,” according to the IAU’s 2008 decision?

A

Dwarf planets located in the outer regions of the Solar System, such as Pluto, Eris, Haumea, and Makemake.

44
Q

Describe Ceres

A

Ceres is the largest object in the asteroid belt - it is spherical and may even have an ocean and atmosphere

it is a tiny fraction of the Moon’s size.

45
Q

Current Classification of Bodies in our Solar System:

As a result of the scheme for defining celestial bodies in our solar system passed by IAU in 2006, the solar system contains how many planets and how many officially recognized dwarf planets? What are their names?

Are there other bodies that may meet the specfications of dwarf planet that have not been “offically recognized”?

A

8 planets:
* Mercury
* Venus
* Earth
* Jupiter
* Saturn
* Uranus
* Neptune)

5 “officially recognized” dwarf planets:
* Ceres
* Pluto
* Eris
* Haumea
* Makemake

(Haumea and Makemake were added later)

Note: There are many more bodies that fit the definition of dwarf planet - at least a hundred have been discovered so far - but the IAU, in its wisdom, has only given out official dwarf planet status to these 5

46
Q

What is the key issue with the Nebular Hypothesis in explaining the present order of planets in our solar system?

A

It does not fully explain how large planets like Uranus and Neptune formed far from the Sun, while smaller planets like Mars formed closer, where planet-building material was plentiful.

47
Q

What is planetary reshuffling?

A

The idea that the planets didn’t remain where they formed but were moved into different positions due to gravitational interactions early in the Solar System’s history.

48
Q

What is the “Nice Model” (Named after the French City). What does it explain and what does it fail to explain?

A

the “big four” planets were assembled very quickly between 5 and 12 AU from the Sun, but after a couple million years, they started interacting with each other since their orbits were close. Those interactions pushed them out to different positions.

This still does not explain why terrestrial planets are so small

49
Q

What does the Grand Tack model explain?

A

It explains how Jupiter’s and Saturn’s migrations reshaped the inner Solar System, helping to form the terrestrial planets and influencing the asteroid belt’s composition.

Jupiter’s Migration:
Jupiter, the largest planet, initially formed between 5 and 12 AU from the Sun.
It began movinginward , being pulled toward the Sun. As it migrates, it pushes rocky planetesimals inward - like a snowplough - to create a “mini-disk” from which the terrestrial planets were formed.

Saturn’s Influence:
Saturn also formed further out but was eventually pulled inward as well.
Saturn’s gravitational influence stopped Jupiter’s inward migration, and both planets swung around and migrated outward to their current positions.

Impact on Terrestrial Planets:
Jupiter’s inward and outward migration shaped the small rocky planets by compressing the inner disk of material into a smaller region, forming the planets we see today.
Mars, which formed at the edge of the disk, was pushed outward, leading to its relatively small size.

Explaining the Asteroid Belt:
The Grand Tack model also explains how the asteroid belt has more rock rich material closer in and more water rich material farther out.
Jupiter’s movement would have stirred up the material, helping to distribute it differently across the Solar System.

50
Q

What is an important point about the time period of the Nice and Grand Tack Models?

A

an important point to remember about these models is that jupiter grows to become large really quickly.

All of the Grand Tack action takes place over 5 million years, and the Nice model covers the next 500 million years.

51
Q

Describe what is being depicted in this image

A

Solar system bodies

52
Q

Explain this image depicting the Nice and Grand Tack Models by time period.

A
53
Q

What is the Late Heavy Bombardment (LHB) ?

A

A period from 4.1 to 3.8 billion years ago when many small bodies in the outer Solar System were displaced and collided with the inner planets.

their orbits were disturbed by the reshuffling of the gas giants (Jupiter, Saturn, Uranus, and Neptune).
As these bodies were displaced, many fell inward toward the Sun, passing through the inner Solar System, where they collided with planets like Earth, the Moon, and Mercury.

54
Q

Evidence for Late Heavy Bombardment (LHB)

A

Evidence on the Moon:
The surface of the Moon is heavily cratered, with most of the craters dating back to the LHB. Rock samples from the Moon, brought back by the Apollo missions, were dated to confirm this bombardment period.

Evidence on Earth:
While Earth’s surface has been geologically reworked since the LHB, scientists have found evidence of the bombardment in ancient rocks in places like Greenland and northern Canada. These rocks contain an unusual isotope of tungsten that is thought to have an extraterrestrial origin.

Mercury:
The planet Mercury also shows signs of intense cratering from this time period, although we lack sufficient data to confirm this as strongly as on the Moon.

55
Q

What is Obliquity? If our theories of panetary formation in our solar system our correct, what would we expect for obliquity of planets? Is this the case? Why or why not?

A

Obliquity is the angle between Earth’s equatorial plane and its orbital pane (its eliptic)

If our theories of formation of solar system are correct, we should expect all planets to have the same sense of rotation and essentially a zero obliquity (the planets should coincide)

This is not the case: Mercury’s obliquity is pretty close to 0 but the others vary greatly.

Why?
most scientists believe that toward the end of the planet formation period - particularly at end of the planet suffle stage - the final few large collisions of large protoplanets/planetestimals knocked the planets askew.

(for example, venus has angle of obliquity of about 180 degrees, that means the planet began life with opposite sense of rotation or more likely that it was given such a hard knock that it started rotating on it’s head)

Obliquity of the Planets
56
Q

Why is obliquity important (what does it affect on earth)

A

influences the planets seasons, like on earth

57
Q

What are exoplanets or extrasolar planets?

A

Planets outside our solar system

58
Q

How did scientists predict other solar systems should look before we were able to detect them?

What has been the actual result now that we have data to test this hypothesis

A

they thought other solar systems should like something ike ours, with rocky planets appearing inside a ‘frost line’ and big, gassy planets farther out.

turned out to be completely wrong – it seems our solar system is actually quite unusual, with only 1 our of nearly 700 planetary systems looking anything like ours.