Data on the Velocity of the Celestial Bodies Orbiting a Galaxy

In summary, the conversation touched on researching dark matter and obtaining data on the individual velocities of bodies orbiting a galaxy's center. It was suggested to look for these data in scientific publications, particularly in the references provided in a Wikipedia article on the subject. The speaker also mentioned Vera Rubin as a noteworthy researcher in this field.
  • #1
ecastro
254
8
I am currently researching about the behavior of dark matter and their possible characteristics, and I am needing the individual velocities of the bodies orbiting a center of a galaxy. The collection of data where physicists hypothesized the existence of Dark Matter. Where can I find these data? If ever possible.

Thank you in advance.
 
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  • #2
ecastro said:
I am currently researching about the behavior of dark matter and their possible characteristics, and I am needing the individual velocities of the bodies orbiting a center of a galaxy. The collection of data where physicists hypothesized the existence of Dark Matter. Where can I find these data? If ever possible.
In scientific publications. The references in this wikipedia article should be a good starting point.
 
  • #3
Thanks a lot! I think I found what I need.
 
  • #4
Be sure to click on that link in the wiki for Vera Rubin. She seems an amazing researcher and receives far too little credit for the storm she caused.
 
  • #5


I appreciate your interest in researching the behavior of dark matter. The individual velocities of celestial bodies orbiting a galaxy can be obtained through various astronomical databases and observations. Some examples include the Sloan Digital Sky Survey, the Hubble Space Telescope, and the Gaia Mission. These sources provide data on the velocities of stars and other celestial bodies within galaxies, which can then be used to study the effects of dark matter on their orbits.

However, it is important to note that the exact velocities of celestial bodies may vary depending on the specific galaxy and its characteristics. Additionally, the study of dark matter is an ongoing and complex area of research, so it is crucial to carefully analyze and interpret the data in order to draw meaningful conclusions. I recommend consulting with other experts in the field and utilizing multiple sources of data to ensure accuracy in your research. Best of luck in your studies.
 

1. What is the significance of studying the velocity of celestial bodies orbiting a galaxy?

The velocity of celestial bodies orbiting a galaxy can provide valuable information about the structure, dynamics, and evolution of the galaxy. It can also help us understand the distribution of dark matter within the galaxy and the effects of gravitational interactions between different objects.

2. How is the velocity of celestial bodies measured?

The velocity of celestial bodies can be measured using various techniques such as spectroscopy, interferometry, and astrometry. These methods involve analyzing the light emitted from the bodies and measuring the Doppler shift to determine their velocity.

3. What type of data is collected when studying the velocity of celestial bodies?

The data collected when studying the velocity of celestial bodies includes information about their orbital speeds, direction of motion, and distance from the center of the galaxy. It may also include data on the composition, mass, and size of the bodies.

4. How do scientists use data on the velocity of celestial bodies to make predictions?

Scientists can use data on the velocity of celestial bodies to create models and simulations that can predict future movements and interactions. By studying the patterns and changes in velocity, scientists can make predictions about the evolution of the galaxy and the behavior of its celestial bodies.

5. What are some challenges of collecting and analyzing data on the velocity of celestial bodies?

Some challenges of collecting and analyzing data on the velocity of celestial bodies include technical limitations of instruments, the vast distances involved, and the complex interactions between objects. Additionally, the presence of dark matter and the effects of gravitational lensing can also complicate the interpretation of data.

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