Search patterns in observational studies

In summary, astronomers use a variety of methods to find planets around stars, but some stars are not good candidates for detection due to their mass or brightness.
  • #1
stargazer3
44
3
Hello Physics Forums!

I've just read about the discovery of GJ 667Cc, and it made me ponder on how do astonomers develop the sequence of stars to be examined in search for exoplanets? I know that some telescopes, like Kepler mission, are just collecting raw data from a certain area of space, but what about more flexible observatories? In other words, why, discovering so many distant exoplanets, we know so little about the closest to Sun hundred or so stars (we are trying to find the closest habitable planet, aren't we)?
 
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  • #2
It depends on the detection method. For example, if you wanted to do direct imaging to detect planets, your telescopes intrinsic resolution limit would set the upper boundary for the distance the star could be at, so you would image stars that were close by. And even then, if you were using Infrared imaging to detect the heat from young star systems and their planets, you would have to observe stars that were still young enough for their planets to be very hot and emit infrared radiation.

Beyond that, the type of star itself is also a major feature that you must consider. Huge, bright, supergiant stars are usually poor candidates for most detection methods,(I think) as their masses are so high that any planets in orbit would barely cause the star to shift around, making it much more difficult to detect planets using the radial velocity method. These stars would also have a much smaller amount of surface area become blocked by a transiting planet, reducing the chances of using that method as well. Plus, most people are more interested in "sun like" stars, as the star system would be much more similar to Earth's.

In other words, why, discovering so many distant exoplanets, we know so little about the closest to Sun hundred or so stars (we are trying to find the closest habitable planet, aren't we)?

Who says we don't know much?
 
  • #3
Drakkith is right, astronomers do know quite a lot about our nearest stars.
Here is an article I found interesting about the Altha Centauri system. Has nice charts displaying what the orbital distances of such planets might be.


Alpha Centauri
A Candidate for Terrestrial Planets And Intelligent Life
http://aether.lbl.gov/www/classes/p139/speed/Alpha-Centauri.html


The following article is also relevant to your question.

 
  • #4
Thanks a lot for both responses, they cover everything I wanted to know to large extend.
 
  • #5


Hello there,

Thank you for your question about search patterns in observational studies. I can explain how astronomers develop the sequence of stars to be examined in search for exoplanets.

Firstly, astronomers use various techniques to identify potential exoplanets, such as the transit method, radial velocity method, and direct imaging. Each of these methods has its own set of limitations and biases, so it is important to use a combination of techniques to increase the chances of detecting exoplanets.

Secondly, astronomers use a variety of tools and instruments to observe different regions of the sky. For example, the Kepler mission focuses on a specific area of the sky, while other telescopes may have a wider field of view. This allows for a more comprehensive search of different types of stars and their potential exoplanets.

In terms of why we know more about distant exoplanets compared to the closest stars, it is a matter of distance and technology. The closest stars are relatively far from Earth, making it more challenging to observe and study them in detail. Additionally, the technology used to detect and study exoplanets is constantly evolving, so we may have more information about distant exoplanets simply because we have had more time and resources to study them.

Overall, the search for exoplanets is an ongoing and complex process that involves careful planning and utilization of various tools and techniques. As we continue to make advancements in technology and observational methods, we will likely uncover more information about both distant and nearby exoplanets. I hope this helps to answer your question. Thank you for your interest in astronomy and exoplanet research.
 

1. What are search patterns in observational studies?

Search patterns in observational studies refer to the systematic methods used to identify and collect data on a particular topic or phenomenon. These patterns can include selecting specific variables to observe, choosing a sample size, and determining the best approach for data collection.

2. Why are search patterns important in observational studies?

Search patterns are important in observational studies because they help ensure that the data collected is accurate, reliable, and relevant to the research question. They also help researchers avoid bias and make more objective conclusions based on the data.

3. What are some common search patterns used in observational studies?

Some common search patterns used in observational studies include cross-sectional studies, case-control studies, cohort studies, and ecological studies. Each of these patterns has its own advantages and limitations and may be more suitable for certain research questions.

4. How do researchers determine the most appropriate search pattern for their study?

Researchers determine the most appropriate search pattern for their study by considering the research question, the available resources, and the limitations of each search pattern. They may also consult with other experts in the field and conduct a pilot study to determine the effectiveness of different search patterns.

5. Are search patterns only used in observational studies?

No, search patterns are not limited to observational studies. They can also be used in other types of research, such as experimental studies or surveys. However, the specific search patterns used may differ depending on the type of research and the research question being addressed.

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