A big fault on Kepler

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Profile Saiyasodharan
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Message 873237 - Posted: 7 Mar 2009, 3:27:27 UTC

hi,

kepler ll find a planet only if the planer passes between the kepler's field of view and the star...

but i think that the possibility for a planet to orbit its star at a certain degree is very very low, because there are so many other possible orbits.

to make things clear, see this image: Kep
i m not good at drawing, but i think its understandable

in the picture, case 1(above) is the setup we need to detect a planet... but planets may circle around as in case2(below) too. so its impossible to detect it

so, kepler will b finding only a fraction of planets, that it cud see and not all of them...

if i m wrong, pls expain me... also pls tell me how to add image to this post(i tried [img] but its not working)


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Message 873251 - Posted: 7 Mar 2009, 3:51:05 UTC - in response to Message 873237.  

hi,

kepler ll find a planet only if the planer passes between the kepler's field of view and the star...

You are correct. The transit method is just one of a few different ways to detect an extrasolar planet.

Multiple methods help track elusive quarry, HTML version
4 Ways to Find a Planet, interactive Flash presentation
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Message 873293 - Posted: 7 Mar 2009, 7:27:38 UTC - in response to Message 873237.  

hi,

kepler ll find a planet only if the planer passes between the kepler's field of view and the star...

but i think that the possibility for a planet to orbit its star at a certain degree is very very low, because there are so many other possible orbits.

to make things clear, see this image: Kep
i m not good at drawing, but i think its understandable

in the picture, case 1(above) is the setup we need to detect a planet... but planets may circle around as in case2(below) too. so its impossible to detect it

so, kepler will b finding only a fraction of planets, that it cud see and not all of them...

if i m wrong, pls expain me... also pls tell me how to add image to this post(i tried [img] but its not working)



Actually it's not a big fault...it's really the only way we have at this time to detect planets as small as Earth. The designers of Kepler understood this and already figured out that the odds of everything being lined up properly is only about one half of one percent (0.5%). However, given the sheer number of stars that Kepler will be looking at, that still adds up to nearly 500 Earth-like planets. Hardly a fault at all. :)
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Message 873301 - Posted: 7 Mar 2009, 8:26:49 UTC

Kepler night launch
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Message 873422 - Posted: 7 Mar 2009, 16:34:37 UTC

Did you have to title your post in that manner so soon after launch? I thought the spacecraft broke.
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Message 873457 - Posted: 7 Mar 2009, 17:43:16 UTC

The chances are pretty small that the planet will transit its star as seen from Kepler. In the case of something like the Earth, it's about 1/2 degree divided by 180 degrees or about 0.28%. But that's probably why Kepler has been set up to look at over 100,000 stars. Out of 280 possible stars there might be several candidates. It'll probably have to make a lot of measurements because transit times are short.
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Message 873480 - Posted: 7 Mar 2009, 18:38:44 UTC - in response to Message 873457.  
Last modified: 7 Mar 2009, 18:39:11 UTC

thanks everybody for explaining the things to me... but i m very disappointed on knowing that only a small no. of planets cud be detected by kepler... but it okay, there is no other way...

and MRay. i m sorry. the next time i ll keep the title in a more suitable way.
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Message 873503 - Posted: 7 Mar 2009, 19:36:52 UTC - in response to Message 873480.  

thanks everybody for explaining the things to me... but i m very disappointed on knowing that only a small no. of planets cud be detected by kepler... but it okay, there is no other way...

and MRay. i m sorry. the next time i ll keep the title in a more suitable way.


Once Kepler returns with results, we can build larger space telescopes and interferometers which will be able to actually photograph these planets. Once the new equipment has checked out Kepler's results, we can point it at any star and view the planets there visually without needing any transits. :) One step at a time.
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Message 874483 - Posted: 11 Mar 2009, 2:02:31 UTC - in response to Message 874005.  

Just playing with the idea, would it perhaps make sense to pay special SETI attention to the directions this Kepler possibly reveals in the future years?

Regards

PK


Well the only way to get the Seti community focused on one of these new planets is if we confirm that there are biological processes going on. If we find evidence life, then I'll bet every telescope in the world will be pointed in that direction to see if it's simple or advanced life.
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Message 898047 - Posted: 22 May 2009, 3:34:35 UTC

Engineers have begun to check Kepler to ensure it is working properly, a process called "commissioning" that will take about 60 days. In about a month or less, NASA will send up commands for Kepler to eject its dust cover and make its first measurements.


Well, that is quite thoughtful of them. To contribute more space debris!

"Even if we find no planets like Earth, that by itself would be profound. It would indicate that we are probably alone in the galaxy," said Borucki.


That would indeed be profound since we can't see stars inside nearby galaxy. Speaking of which, can Kepler see stars on the opposite side of Milky Way? Past its centre? I suppose not.
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Message 898049 - Posted: 22 May 2009, 3:46:02 UTC - in response to Message 874005.  

Any Earth-size planets orbiting in the habitable zones of stars the size of our Sun would take at least three years to be confirmed.


Now, how did they come to that conclusion? It takes 3 years to confirm.
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Message 898100 - Posted: 22 May 2009, 6:06:23 UTC

...yet Necromancer will unexpectedly exhume the thread’s rotting corpse, and strike horror in the forum as its grotesque form lurches into the discussion. The monster, instantly recognized by all who knew it in life, seems at first to breathe and have a pulse, but, alas, it is beyond Necromancer’s skill to fully restore the thread’s original vitality.
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Message 898146 - Posted: 22 May 2009, 7:59:06 UTC - in response to Message 898049.  



Now, how did they come to that conclusion? It takes 3 years to confirm.


In order for Kepler to confirm the presence of a planet, it needs to observe three transits. Earth takes one year to go around the sun. Thus, if an alien Kepler were looking at us, they'd need to wait three years for us to go around our sun three times.

Most Earthlike planets are expected to be around the same distance from their stars as we are from ours. So about three years.
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Message 898156 - Posted: 22 May 2009, 9:06:07 UTC - in response to Message 898146.  

In order for Kepler to confirm the presence of a planet, it needs to observe three transits. Earth takes one year to go around the sun. Thus, if an alien Kepler were looking at us, they'd need to wait three years for us to go around our sun three times.

Most Earthlike planets are expected to be around the same distance from their stars as we are from ours. So about three years.


Strange, I thought Kepler is looking at a particular part of the Milky Way that is unaffected by Earth orbit about the Sun. Hence, looking at the same spot without blinking for 3 years?
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Message 898164 - Posted: 22 May 2009, 10:05:29 UTC - in response to Message 898156.  

In order for Kepler to confirm the presence of a planet, it needs to observe three transits. Earth takes one year to go around the sun. Thus, if an alien Kepler were looking at us, they'd need to wait three years for us to go around our sun three times.

Most Earthlike planets are expected to be around the same distance from their stars as we are from ours. So about three years.


Strange, I thought Kepler is looking at a particular part of the Milky Way that is unaffected by Earth orbit about the Sun. Hence, looking at the same spot without blinking for 3 years?


I think you missed the point.

If the planet we are trying to detect has a "year" the same length as ours, it would take 3 yrs for it to transit it's own sun three times.
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Message 898168 - Posted: 22 May 2009, 10:37:53 UTC - in response to Message 898164.  

Ah, forgive me for reading too fast. But why 3 transits are needed?
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Message 898179 - Posted: 22 May 2009, 11:35:26 UTC - in response to Message 898168.  

Ah, forgive me for reading too fast. But why 3 transits are needed?


Only my guess but I would think you need 3 so that you can compare timing between 1-2 and 2-3 to verify that you are observing a constant orbital rate.
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Message 898246 - Posted: 22 May 2009, 15:27:55 UTC - in response to Message 898179.  

Ah, forgive me for reading too fast. But why 3 transits are needed?


Only my guess but I would think you need 3 so that you can compare timing between 1-2 and 2-3 to verify that you are observing a constant orbital rate.


Another reason:

If there are multiple planets orbiting/transiting the same star, the intervals between transits will vary. Therefore you need a minimum of 3 detections to validate a single planet and 6 to verify a second.
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Message 898298 - Posted: 22 May 2009, 17:46:51 UTC - in response to Message 898168.  

Ah, forgive me for reading too fast. But why 3 transits are needed?


In order to make sure there's really something there. In theory, a single transit could be "faked" by having some kind of object pass between Kepler and the target star. By observing three full transits, it can be determined whether or not they are the real thing or just false alarms. As a prevoius poster mentioned, if you compare the orbital timing, and find three transits that have a nearly identical period, then it's safe to assume it's not a false alarm.
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Message 898313 - Posted: 22 May 2009, 18:49:37 UTC - in response to Message 898164.  



I think you missed the point.

If the planet we are trying to detect has a "year" the same length as ours, it would take 3 yrs for it to transit it's own sun three times.


Actually we could get results in two years from observations begin.
The first transit now, the second in a year, and the third in two years :-)
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