How to measure the Sun's acceleration relative to the galaxy?

In summary, the acceleration of our sun relative to our galaxy would be determined by measuring the distances to nearby stars, which are also moving, and by measuring the brightness of stars to determine their distances.
  • #1
KurtLudwig
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How would the acceleration of our sun relative to our galaxy be determined?
A spaceship in orbit around our sun, with engines turned off, is in free fall. Accelerometers will read zero. Turning the engines on, the accelerometers will read the acceleration due to the thrust from the engines. Measuring the distances to nearby stars, which are also moving, is tricky. Measuring the distances to stars toward the center of our galaxy, maybe the best answer. Can brightness be used to measure distances in our galaxy?
 
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  • #2
KurtLudwig said:
How would the acceleration of our sun relative to our galaxy be determined?

The sun is in free fall, just like the spaceship you mention, so the "acceleration" you refer to is coordinate acceleration, not proper acceleration. It is much too small to be measurable directly. You can estimate what it should be from the Sun's distance from the center and orbital period or velocity around the center, which are easily found online; we can estimate those numbers fairly well from observations.

KurtLudwig said:
Measuring the distances to nearby stars, which are also moving, is tricky.

Actually, distances to nearby stars--near enough to get a measurable parallax--are the easiest and most accurate distance measurements we have beyond the solar system.

KurtLudwig said:
Can brightness be used to measure distances in our galaxy?

For certain types of stars, the "standard candles" (such as Cepheid variables) where we have an independent way to measure brightness, yes. But for most stars, we try to measure the distance and then infer the brightness (absolute magnitude) from that and the apparent magnitude.
 
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  • #3
Please correct if false or clarify: Is proper acceleration as measured by an accelerometer? Isn't coordinate acceleration a term used in relativity? Is our sun moving that fast that relativity is coming into play? According to Wikipedia, the sun travels at only 220km/s around the center of the milky way.
I understand, that there is no preferred or fixed reference position. The only constant is the speed of light. Can inertia be considered a momentary local reference frame? I still do not understand how inertia comes to be, almost as if matter is connected to other matter. An object in free fall has inertia, although its potential and kinetic energies are changing. By conservation of energy, the sum of potential and kinetic energy must stay constant, in the absence of heat dissipation. All the planets moving at different velocities have inertia. Is inertia the resistance to a change of momentum?
 
  • #4
KurtLudwig said:
Is proper acceleration as measured by an accelerometer?

Yes.

KurtLudwig said:
Isn't coordinate acceleration a term used in relativity?

Typically, but that doesn't mean it's only applicable to things moving at relativistic speeds.

KurtLudwig said:
Is our sun moving that fast that relativity is coming into play?

It depends on how accurate you want your predictions and measurements to be.

KurtLudwig said:
Can inertia be considered a momentary local reference frame?

This doesn't make sense; inertia is a property of objects, not a frame.

KurtLudwig said:
I still do not understand how inertia comes to be

This is a separate question which should be asked in a separate thread.
 
  • #5
KurtLudwig said:
Is proper acceleration as measured by an accelerometer?
Yes (which means that it's trivially zero for the sun because the sun is in free-fall). But here you aren't asking how we measure the proper acceleration, you're asking for the acceleration relative to the center of the galaxy, and acceleration "relative to" something else is cooordinate acceleration - indeed, that's fairly close to being the definition of coordinate acceleration.
Isn't coordinate acceleration a term used in relativity? Is our sun moving that fast that relativity is coming into play?
The term is used in relativity, but like "speed"and "position" that's not the only place it's used. Any time you're talking about acceleration "relative to" something else, you're talking coordinate acceleration; relativity doesn't have to be involved.

And as for how we measure coordinate acceleration? We don't. We measure the distance between the accelerating object and the "relative to" point in space, and see how it changes over time.
 
  • #6
KurtLudwig said:
Is inertia the resistance to a change of momentum?
Doesn't the word 'Mass' do a perfectly adequate job here - at least in Newtonian Mechanics?
KurtLudwig said:
Can brightness be used to measure distances in our galaxy?
Red Shift and Parallax measurements work for distances within the Galaxy. At least over the near regions in the galaxy, parallax gives fairly accurate results. Also Cepheid Variables can be used for all galactic distances (your 'brightness' idea).
I'm always gobsmacked by the accuracy of (or at least the confidence in) measurements of stellar distances and speeds.
 
  • #7
After viewing the Milky Way, while camping in Utah, I became hooked on astronomy and cosmology. You, the advisors at Physics Forums, are lucky to have chosen this field of study. I was building machinery to manufacture cars.
Thank you for your answers.
To support Physics Forums, I will buy all books, from your website
 

Related to How to measure the Sun's acceleration relative to the galaxy?

1. How is the Sun's acceleration measured?

The Sun's acceleration is measured by observing the motion of stars in our galaxy. By tracking the positions and velocities of stars over time, scientists can calculate the gravitational forces acting on them and determine the acceleration of the Sun.

2. What is the unit of measurement for the Sun's acceleration?

The Sun's acceleration is typically measured in units of meters per second squared (m/s²). This is the standard unit for acceleration and represents the change in velocity over time.

3. How does the Sun's acceleration affect Earth?

The Sun's acceleration does not have a direct effect on Earth. However, the Sun's gravitational pull is what keeps Earth in orbit around it, so any changes in the Sun's acceleration can indirectly affect Earth's orbit and the length of our year.

4. How does the Sun's acceleration compare to other celestial bodies?

The Sun's acceleration is relatively low compared to other celestial bodies. It is about 0.0059 m/s², which is much smaller than the acceleration of Earth (9.8 m/s²) or even the Moon (1.62 m/s²). This is because the Sun is much more massive and therefore has a stronger gravitational pull.

5. Can the Sun's acceleration change over time?

Yes, the Sun's acceleration can change over time. This is due to the fact that the Sun is constantly moving through the galaxy and experiencing gravitational forces from other celestial bodies. Additionally, changes in the distribution of mass in the galaxy can also affect the Sun's acceleration.

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