Distance from Sun to outside galaxy?

In summary, the distance from the Sun to the nearest place officially "outside" the Milky Way galaxy is around 100,000 light years.
  • #1
Holocene
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Distance from Sun to "outside" galaxy?

Does anyone have a general figure regarding the distance from the Sun to the nearest place officially "outside" the Milky Way galaxy?

Thnaks.
 
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  • #2
Depends what you mean by awayfrom the milky way, but at the sun's distance from the centre the galaxy is about 3000 years thick - so you could say 1500 lyr
 
  • #3
By "place" do you simply mean an area of space? In that case, just Google for "size of Milky Way" and "Sun's position in the Milky Way" and subtract the 2 answers to get the distance from the Sun to the edge of the Galaxy. I would guess around 100,000 light years.

Or do you want to know the closest non-Milky Way object to the Sun? The Large and Small Magellanic Clouds are satellite galaxies of the Milky Way. They are roughly 200,000 light years away.
 
  • #4
tony, moving along the galactic plane is not the fastest way to exit the galaxy.


As mgb_phys explains, the fastest way is to travel straight "up" or straight "down" relative to the galactic plane.

According to him, that's a mere 1500ly in wither direction. I would have thought it was more than that, but I'll defer to him.
 
  • #5
I quote the noted cosmologist E. Idle

Our galaxy itself contains a hundred billion stars.
It's a hundred thousand light years side to side.
It bulges in the middle, sixteen thousand light years thick,
But out by us, it's just three thousand light years wide.
We're thirty thousand light years from galactic central point.
We go 'round every two hundred million years,
And our galaxy is only one of millions of billions
In this amazing and expanding universe.

The song is pretty accurate and is a good way of memorising a lot of astronomical distances - most astronomers can sing all of it ( generally rather badly )
 
  • #6
DaveC426913 said:
tony, moving along the galactic plane is not the fastest way to exit the galaxy...

Although the majority of visible matter is concentrated in the galactic plane, the halo contains a lot of matter too, including halo stars, which stand out because their tangental motion relative to the Sun is about 200 km/s rather than 20 km/s for the disk stars. The galactic halo also contains many globular clusters, filled with hundreds of thousands to millions of stars each. Most of these clusters are on orbits highly inclined to the galactic plane. So it would probably be a safer assumption to consider the galaxy as a sphere.
 
  • #7
Wikipedia has a nice description: http://en.wikipedia.org/wiki/Milky_Way#Halo
The galactic disk is surrounded by a spheroid halo of old stars and globular clusters, of which 90% lie within 100,000 light-years,[20] suggesting a stellar halo diameter of 200,000 light-years. However, a few globular clusters have been found farther, such as PAL 4 and AM1 at more than 200,000 light-years away from the galactic center. While the disk contains gas and dust obscuring the view in some wavelengths, the spheroid component does not. Active star formation takes place in the disk (especially in the spiral arms, which represent areas of high density), but not in the halo. Open clusters also occur primarily in the disk.
 

Related to Distance from Sun to outside galaxy?

1. How far is the distance from the Sun to the outermost edge of our galaxy?

The distance from the Sun to the outermost edge of our galaxy, also known as the galactic radius, is estimated to be around 50,000 light-years. This means that it would take around 50,000 years for light to travel from the Sun to the outer edge of the Milky Way galaxy.

2. How is the distance from the Sun to the outer galaxy measured?

The distance from the Sun to the outer galaxy is measured using a variety of techniques, including parallax measurements, which use the Earth's orbit to calculate distances to nearby stars, and the use of standard candles, such as supernovae, to measure distances to more distant objects.

3. Is the distance from the Sun to the outer galaxy constant?

No, the distance from the Sun to the outer galaxy is not constant. Our galaxy, like many others, is constantly expanding and rotating, which means that the distance from the Sun to the outer edge is constantly changing. Currently, it is estimated to be expanding at a rate of about 67 kilometers per second per megaparsec.

4. How does the distance from the Sun to the outer galaxy affect the Earth's orbit?

The distance from the Sun to the outer galaxy does not have a direct impact on the Earth's orbit. However, the gravitational pull of other stars and objects within the galaxy can affect the Earth's orbit, leading to small changes over time.

5. How does the distance from the Sun to the outer galaxy affect the habitability of other planets?

The distance from the Sun to the outer galaxy can have a significant impact on the habitability of other planets. A planet that is too close to the outer edge of the galaxy may be exposed to higher levels of harmful radiation, while a planet that is too far from the outer edge may not receive enough energy from the Sun to support life. The location of a planet within the galaxy's habitable zone is crucial for its potential to sustain life.

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