4.2: Galaxies Flashcards
(22 cards)
Who suggested the most widespread system of classifying galaxies
Edwin Hubble in 1920’s
What are the 4 type of galaxy
- spiral (S)
- barred spiral (SB)
- elliptical (E)
- irregular (Irr)
Describe a spiral galaxy
Flattened disk-shaped systems e.g. Andromeda
Describe a barred spiral galaxy
Similar to a spiral but with a bright ‘bar’ running through the nucleus from which spiral arms emerge
Describe an elliptical galaxy
Relatively smooth spheroidal distributions of stars,showing a gradual decrease in brightness from centre outwards
Describe an irregular galaxy
Very little structure or symmetry
How are S and SB galaxies distinguished further
By sub-classifying them with letters a,b or c depending on the strength of the nuclear bulge and ‘openness’ of the spiral arms (Sa galaxies have big nuclear and tightly wound arms, Sc galaxies have small nucleus and open arms)
How are E galaxies distinguishe further
By sub-classifying then with numbers 0-7 depending on their shape (E0 is almost circular and E7 is highly elongated)
What do later versions of Hubbles scheme include
Lenticular galaxies (S0) as a class between ellipticals and spirals
What is Hubble’s classification scheme shown on
A tuning fork diagram. It was first published in 1936 in his book The Realm of the Nebulae
When was the galaxy zoo launched and what is it
Launched in July 2007 and is a web-based project that has invited members of public to access images of galaxies in order to classify them
What galaxy type is the Milky Way
SBb
What does the local group included
- the andromeda galaxy
- the LMC and SMC
- the Triangulum Galaxy
- several satellite and dwarf galaxies such as Pisces Dwarf and Aquarius Dwarf
How far across is the local group
3 Mpc
What supercluster is local group part of
The Virgo Supercluster
What are active galaxies/active galactic nuclei
Galaxies that emit vast amounts of energy at wavelengths other than those of visible light
What are the 4 main types of active galaxy/active galactic nuclei
- radio galaxies
- seyfert galaxies
- quasars
- blazars
Describe radio galaxies
- discovered in 1950s
- mainly elliptical galaxies
- intense sources of radio waves
- radio emissions often originate from symmetrical pairs of ‘lobes’ that lie on opposite sides of the galaxy
Describe seyfert galaxy
- discovered by carl seyfert in 1943
- spiral galaxy
- have extremely compact but bright nuclei
- have strong emission lines in their spectra
- show strong and often variable emissions of radiation at IR and X-ray wavelengths
Describe quasars
- discovered by radio astronomers in 1963
- compact appearance make the look star-like
- emit huge quantities of energy from X-rays to (sometimes)radio waves
- high redshifts reveal quasars are some of most distant objects in universe
Describe Blazars
- discovered in 1970s
- appear star-like
- lie much closer than quasars
- emir strongly in all regions of spectrum from Radio to gamma-rays
- can vary in optical brightness in a timescale of 1/2 days
How do astronomers believe AGNs are powered
By matter falling onto a supermassive black hole that lies at the centre of the galaxy