Expolanets Flashcards

1
Q

exoplanet

A

orbit another star

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2
Q

solar nebula theory

A

describes the formation of our solar system from a nebula cloud made from a collection of dust and gas

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3
Q

we tend to find exoplanets around ______
stars

A

metal-rich

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4
Q

Exoplanet Detection - Transit Method

A

When the exoplanet passes Infront of its host star we can measure the amount of dimming and the transit time, allowing us to determine the exoplanets size and orbital characteristics

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5
Q

Exoplanet Detection - Gravitational Microlensing

A

General Relativity tells us that massive objects cause
spacetime to curve. Light changes and can be focused just like a lens

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6
Q

Exoplanet Detection - MOA telescope

A

Microlensing Observations in
Astrophysics”
The MOA telescope is a Japanese/NZ
collaboration, located in Tekapo, South Island

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7
Q

Exoplanet Detection - Radial Velocity

A

spectroscopy determines it, characteristic spectral lines in the light
we receive from the star, and determine whether
they are redshifted (as the star moves away from
us) or blueshifted (as the star moves toward us)

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8
Q

Exoplanet Detection - Astrometry

A

The motion can also be visible as changes in the star’s
apparent position in the sky relative to other reference
stars

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9
Q

The motion can also be visible as changes in the star’s
apparent position in the sky relative to other reference
stars

A

Astrometry

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10
Q

Pulsars are rapidly rotating neutron stars which emit
beams of intense radiation.Tiny variations in the timing of the pulses indicate that
the pulsar is orbiting the center of mass of a system
with one or more planets

A

Pulsar Timing

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11
Q

direct imaging

A

Exoplanets are millions of times dimmer than the
stars they orbit, so direct imaging of them is very
difficult

a device inside a telescope which blocks light from
a star before it reaches the telescope’s detecto

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12
Q

Transits: In simple words

A

Looking for passing
shadows (eclipses)

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13
Q

Microlensing:

A

Looking for light
focused by
gravitational lenses

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14
Q

Radial Velocity:

A

Looking for redshift
and blueshift as a host
star wobbles

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15
Q

Astrometry:

A

Measuring change in
position of a star in
the sky

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16
Q

Pulsars

A

Measuring shifts in
‘lighthouse’ pulsar
beam timing

17
Q

Direct imaging:

A

Blocking out light from
a host star so that
dimmer objects
become visibl

18
Q

the majority of exoplanets have
been discovered using

A

transit
method, followed by the radial
velocity method

19
Q

how many confirmed exoplanets

A

5000

20
Q

Exoplanets are typically grouped in four broad
categories

A

Gas giants, Neptunians,
super-Earths(2-10 times bigger than earth) and terrestrials(smaller than earth)