Kepler Telescope Views Single Point in Space 4.2ly Away

Click For Summary

Discussion Overview

The discussion revolves around the observation of a distant planet using the Kepler space telescope, focusing on the techniques employed to infer the presence of planets despite the limitations of resolution. Participants explore various methods of detecting exoplanets, including light curve analysis and Doppler shift techniques, while questioning the implications of resolution limits in astronomical observations.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants explain that the Kepler telescope infers the presence of planets through stellar light curves, where a planet transiting a star causes a measurable dip in luminosity.
  • Others introduce the Doppler shift method, suggesting that the wobble of a star due to an orbiting planet can be detected without requiring a transit, although this method may favor larger planets.
  • There is a discussion about the physical separation referred to in the original post, with participants seeking clarification on the specific measurements being discussed.
  • Some participants express concern that many planets may be missed due to their orbits not presenting transits.
  • Speckle interferometry is mentioned as a technique that can enhance resolution and extract details from light sources, suggesting potential advancements in observational capabilities.

Areas of Agreement / Disagreement

Participants express differing views on the effectiveness of various detection methods and the implications of resolution limits. There is no consensus on the specific physical measurements being discussed, and the conversation remains unresolved regarding the limitations of current observational techniques.

Contextual Notes

Participants note the challenges of discussing complex topics via mobile devices, which may hinder the ability to follow the conversation effectively. The discussion also highlights the dependence on specific definitions and assumptions regarding measurement techniques.

bill ginger
Messages
1
Reaction score
0
Astronomers are viewing a single point in space (.1 arcseconds), using the Kepler space telescope but to view a planet 4.2 light years from the Earth that would require a planet with a diameter of more than ten times the diameter of our solar system.
 
Astronomy news on Phys.org
Do you have a question or did you just need to let us know about that?
 
The question seems to be: how is it possible to observe a planet when your instrument has insufficient resolution.

The answer lies in the technique used - the planets observed by Kepler are not directly resolved, but their presence is inferred from stellar light curves. That is, the CCD camera on the spacecraft collects light from a star, measuring its intensity. When a planet transits in front of the star, it obscures some of this light. The size and orbit of the planet can be determined from the depth and duration of the dip in luminosity (i.e. 'light curves').

More on the method can be found here:
http://kepler.arc.nasa.gov/Mission/QuickGuide/howKeplerFindsPlanets/
 
  • Like
Likes   Reactions: 1oldman2
There is another technique. Kevin Apps, credited with finding the first exoplanet (Planet Kevin) told a group of my students that they used Doppler shift due to the Wobble, as a large planet orbits a star. I seem to remember that it required Jupiter sized planets.
 
To which physical point do you refer? The star-planet separation?
 
DrSteve said:
To which physical point do you refer? The star-planet separation?
The wobble in relative star/Earth velocity gives a measurable (apparently) shifting on wavelength (presumably of some sharp absorption lines).
Afair, his talk was given around ten years ago. I guess the method would have an advantage in that the effect would be detectable even without a transit of the planet. It always bothers me that we must be missing a significant number of planets that have orbits which don't present us with a transit.
 
sophiecentaur said:
The wobble in relative star/Earth velocity gives a measurable (apparently) shifting on wavelength (presumably of some sharp absorption lines).
Afair, his talk was given around ten years ago. I guess the method would have an advantage in that the effect would be detectable even without a transit of the planet. It always bothers me that we must be missing a significant number of planets that have orbits which don't present us with a transit.

I understand the Doopler shift method but still don't know which physical separation you refer to in your original post.
 
DrSteve said:
I understand the Doopler shift method but still don't know which physical separation you refer to in your original post.
?? The relevant measurement was of the change of relative velocity of the Star (the source) and the Earth (receiver). The variation in velocity (amplitude and frequency) and the 'known' mass of the star (from other data such as absolute magnitude and spectrum) would give the probable mass and orbital radius of the orbiting planet. He was well chuffed with himself about that - but then, so would anyone be. Thing was, he didn't invent the technique, he made a calculation to suggest the part of the galaxy in which to look. They looked . . . . and they found.
 
Then the .1 arcsec separation mentioned in the original post has no bearing on anything. Did you have a question that you wanted to pose to the forum?
 
  • Like
Likes   Reactions: sophiecentaur
  • #10
DrSteve, you're confusing sophiecentaur with the OP, who has absconded.
 
  • #11
Bandersnatch said:
DrSteve, you're confusing sophiecentaur with the OP, who has absconded.
Thanks much. Responding via my cell phone leaves much to be desired.
 
  • #12
DrSteve said:
Thanks much. Responding via my cell phone leaves much to be desired.

So I'm not the only one. The small screen is like viewing the world through a toilet roll tube.
We already decided that resolution is just no enough. I wonder if it will ever be.
 
  • Like
Likes   Reactions: DrSteve
  • #13
It's difficult, if not impossible, to get a sweeping overview of an online conversation from a phone, especially if a thread gets hijacked.
 
  • Like
Likes   Reactions: sophiecentaur
  • #14
Bandersnatch said:
DrSteve, you're confusing sophiecentaur
That's not hard to do! :smile:
 
  • Like
Likes   Reactions: phinds and Bandersnatch
  • #15
Speckle interferometry can tease amazing details from an otherwise apparently random collection of photons.
 
  • #16
Chronos said:
Speckle interferometry can tease amazing details from an otherwise apparently random collection of photons.
Yes. Mr Shannon implies that, given time, there is no limit to the possible resolving power.
 

Similar threads

  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 12 ·
Replies
12
Views
3K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 11 ·
Replies
11
Views
4K
  • · Replies 16 ·
Replies
16
Views
5K
  • · Replies 14 ·
Replies
14
Views
3K
  • · Replies 22 ·
Replies
22
Views
4K
  • · Replies 10 ·
Replies
10
Views
3K
  • · Replies 24 ·
Replies
24
Views
3K