Hockey Stick Galaxy NGC 4656
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Hockey Stick Galaxy NGC 4656

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Giant elliptical galaxy M60 and spiral galaxy NGC 4647 do look like an odd couple inĀ this sharp cosmic portraitĀ from the Hubble Space Telescope. But they are found in a region of space where galaxies tend to gather, on the eastern side of the nearbyĀ Virgo Galaxy Cluster. About 54 million light-years distant, bright M60āsĀ simpler egg-like shapeĀ is created by its randomly swarming older stars, while NGC 4647ās young blue stars, gas and dust are organized into winding arms rotating in a flattened disk. Spiral NGC 4647 isĀ estimated to be more distantĀ than M60, some 63 million light-years away. Also knownĀ as Arp 116, the pair of galaxies may be on the verge of a significant gravitationalĀ encounter, though. M60 (aka NGC 4649) is about 120,000 light-years across. The smaller NGC 4647 spans around 90,000 light-years, about the sizeĀ of our own Milky Way.
Like dust bunnies that lurk in corners and under beds, surprisingly complex loops and blobs of cosmic dust lie hidden in the giant elliptical galaxy NGC 1316. This image made from data obtained with the NASA/ESA Hubble Space Telescope reveals the dust lanes and star clusters of this giant galaxy that give evidence that it was formed from a past merger of two gas-rich galaxies.
credit: NASA, ESA, and The Hubble Heritage Team STScI/AURA
Barred Spiral Galaxy NGC 1672 by Hubble Heritage on Flickr.
Via Flickr: Barred Spiral Galaxy NGC 1672. HST ACS/WFC. NASA, ESA, & The Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration
Barred Spiral Galaxy NGC 1300 Credit: Hubble Heritage Team, ESA, NASA

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About This Image
This giant spiral disk of stars, dust and gas is 170,000 light-years across, or nearly twice the diameter of our Milky Way galaxy. M101 is estimated to contain at least one trillion stars. About 100 billion of them could be similar to our Sun.
Credit for Hubble Image: NASA, ESA, K. Kuntz (JHU), F. Bresolin (University of Hawaii), J. Trauger (Jet Propulsion Lab), J. Mould (NOAO), Y.-H. Chu (University of Illinois, Urbana), and STScI
Credit for CFHT Image: Canada-France-Hawaii Telescope/ J.-C. Cuillandre/Coelum
Credit for NOAO Image: G. Jacoby, B. Bohannan, M. Hanna/ NOAO/AURA/NSF
Diagram of "The Local Bubble"
(source)
Some basics of gravity and orbits explained, from a general relativity perspective.
Animation showing an orbiting pulsar and the radiation of gravitational waves.
The spin-period/magnetic field diagram of pulsar evolution.
(source)

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Spectral types listed on the H-R Diagram.
(source)
The apparent magnitude scale.
(source)
A star-forming region in the Orion Nebula.
Horsehead Rides Again
RS Puppis: a Cepheid type variable star, a class of stars whose brightness is used to estimate distances to nearby galaxies. It is surrounded by a reflection nebula, and is 10x more massive than the Sun.

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Watch a sun-sized star go through its evolution on the H-R diagram.
An interactive look at the relationship between size, temperature, and luminosity on the H-R diagram.