A11 - Exploring the solar system Flashcards
Name 4 dwarf planets and their location within the solar system:
Asteroid Belt - Ceres
Kuiper Belt - Pluto, Eris, Makemake
What are SSSOs? Give some examples:
-Small Solar System Objects
-asteroids, meteoroids, comets
Describe the structure of a comet:
-nucleus (“dirty snowball”, solid ice and rock)
-coma (gases and dust that envelope the nucleus)
-dust tail (dust that gets left behind the comet because it moves more slowly)
-ion tail (atoms are ionised by the solar wind, and the tail always points away from the Sun)
Comas get brighter/bigger as the comet approaches the Sun
What types of comets are there? Describe both:
short-period - from Kuiper Belt, orbital period of less than 200 years
long-period - from Oort Cloud, orbital period of more than 200 years
note that this is a log scale diagram
Name the 3 major trans-Neptunian regions of space in the solar system:
-Kuiper Belt
-heliosphere (ends between KB and OC, where the solar wind can no longer be felt)
-Oort Cloud
Who discovered Pluto?
Clyde Tombaugh
What was the first planet discovered using a telescope, and who did it?
Uranus, by William Herschel
What is the difference between a meteorite, meteor, and a meteoroid?
-meteoroids are pebble-sized fragments of larger asteroids that orbit the Sun
-meteors are meteoroids that burn up in the atmosphere
-meteorites are meteors that land on the ground
How are meteoroids formed? Describe their structure:
-collisions of asteroids/other bodies
-made of mostly silicate rocks and some iron/nickel
-usually contains a crystalline Widmanstätten pattern of iron/nickel that is only produced after slow cooling over millions of years
Who determined the size of the AU and the absolute size of the solar system? Briefly outline their method:
-Halley, with the Venus transit method
-he realised that the transit of Venus viewed from different latitudes (along the same line of longitude) were slightly different, and had different transit times
Describe the 3 main theories for the origin of water on Earth:
-water and rock was all accreted to form proto-Earth, so it was always here
-smaller icy comets may have been dislodged from their orbits and brought water to Earth after its formation
-Theia brought water from outer Solar System to Earth when it collided with it (formed the Moon too)
Isotope studies of water suggests that less than 10% of water comes from comet impacts
Why is the eye limited for making observations?
-very small aperture
-low sensitivity to light
What is an objective element?
the lens/mirror that collects and focuses the light from an object to form a brighter image, which can be magnified by an eyepiece
Name 2 refracting and 2 reflecting telescopes:
refracting
-Keplerian
-Galilean
reflecting
-Newtonian
-Cassegrain
Describe how a Keplerian refracting telescope works:
-use convex lens (the objective element) to converge light, making a real image on the other side of the lens, close to the principal focus
-look through another convex lens (the eyepiece) to look at the real image, such that the image is less than one focal distance away from the secondary lens
-this forms a virtual image that is much bigger than the object
How is a Galilean refracting telescope different to the Keplerian refracting telescope?
Galilean has a one-sided convex lens, and a concave eyepiece lens
The objective has a flat side to reduce abberations
Ignore the labels on the diagram, just look at the lenses used
Describe how a Newtonian reflecting telescope operates:
-parabolic mirror reflects light from object to form a real image
-the image is reflected off a plane mirror into an eyepiece where it is magnified
How does a Cassegrain telescope work?
-light reflects off the objective parabolic mirror
-reflects off another secondary hyperbolic mirror
-the light goes through a hole in the objective
-magnified by an eyepiece
What is the “light grasp”?
the amount of the light that a telescope can gather, which is directly proportional to the square of the aperture’s diameter
Define field of view, in the context of telescopes:
the angle of sky that can be seen through the eyepiece
What is the resolving power of a telescope? How can it be increased?
-the ability to distinguish between 2 separate objects (eg binary star system)
-increase aperture
-shorten wavelength of the light being observed
θ needs to be minimised to increase angular resolution, which would need the diameter to increase or the wavelength to decrease
How can the magnification of a telescope be calculated?
the magnification is the focal length of the objective element, divided by the focal length of the eyepiece
When referencing a telescope’s specs, what should you always mention?
explicitly say what the telescope has (eg large diameter, therefore the telescope has a large aperture)
Give comparative answers if necessary
Why were Galileo’s observations important? Name 2 pieces of evidence he collected:
-he showed that the Sun was at the centre of the Solar System (heliocentric)
-he saw that Venus had phases
-he saw that moon’s orbited Jupiter (the Galilean moons)
Venus’s angular size would also change, meaning it was getting closer and further in its orbit around the Sun