Discover Gliese 581g - Just 20 Light-Years Away!

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Discussion Overview

The discussion revolves around the discovery of Gliese 581g, an exoplanet located approximately 20 light-years away, and its potential for hosting life. Participants explore various implications of this discovery, including the nature of the planet, the possibility of intelligent life, and the challenges of communication with extraterrestrial beings.

Discussion Character

  • Exploratory
  • Debate/contested
  • Conceptual clarification
  • Technical explanation

Main Points Raised

  • Some participants express excitement about the discovery, suggesting it could be a potential destination for future exploration.
  • There are humorous suggestions about sending Stephen Hawking as a probe or transmitting signals to the planet.
  • Concerns are raised regarding the implications of contacting potential extraterrestrial life, referencing Hawking's warnings about revealing our presence.
  • Participants discuss the characteristics of Gliese 581g, noting it may have extreme temperature variations and a one-face planet scenario.
  • Some argue that just because a planet is in the habitable zone does not guarantee the existence of intelligent life, highlighting the uncertainty of life evolving there.
  • There is mention of the planet's mass and radius, with estimates suggesting it could have a significantly higher gravity than Earth.
  • Confusion arises regarding the classification of the planets in the Gliese system, with some participants correcting each other about the specific planets being discussed.
  • One participant speculates about the potential for life on Gliese 581g, considering the age of the star system compared to our own.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the likelihood of life existing on Gliese 581g or the implications of contacting extraterrestrial beings. Multiple competing views are presented regarding the planet's characteristics and the nature of potential life forms.

Contextual Notes

There are unresolved assumptions regarding the conditions necessary for life and the implications of the planet's environment on the potential for intelligent life. The discussion also reflects varying interpretations of the data regarding the Gliese 581 system.

  • #61
is it possible that gliese581g has a twin and that the two are locked together in tango in what i understand to be the pluto/charon combination, hence we need to wider our search?
in which case the tidal locking calculation could be a double waste of time , beyond math quiz.
 
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  • #62
Gaius Baltar said:
Just look how misleading this is:



http://www.jb.man.ac.uk/~drl/publications/clf+00.pdf"

http://en.wikipedia.org/wiki/47_Tucanae"

Just goes to show, research goes a long way...

DaveC426913 said:
What a terrible article.

Apparently, hey have already decided its composition is "...rocky with liquid water and atmosphere..."

And I like this comment: "It takes just 37 days to orbit its sun which means its seasons last for just a few days."

The one-face Gliese planets do not have seasons.

Nevermind the fact that they give no details about the mysterious light.

guys i am a bit confused here, so i have done some reading around the net; the conclusion i have come to is that you are quoting a newspaper article which was based on Ragbir Bathals laser-like one-off signal from 47 Tucanae, a galaxy "about 16,700 light years away from Earth" (wikipedia). GLiese 581g is 20light years away need i remind you all. However according to a rival forum, the http://setiathome.berkeley.edu/forum_thread.php?id=61590&sort=7
the error lies in the delay that Prof Ragbir Bathal reported his findings and a mistaken belief that they were the same signal i presume.
in fact, the signals were from different parts of the sky, and so Prof Ragbir Bathals group have no link to GLiese581 at all as far as i can tell and certainly not Gliese 581g.

Thus, DaveC426913, with all due respect, it appears that you are quoting the wrong article in your criticism of the conclusions about the nature of the planet, as you have referenced Camilo et al (2000). I can't see how it could be referring to any planets as there have yet to be any planets detected in this entire galaxy, again according to Wikipedia today.
 
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  • #63
Well, since the planet is gravitationally locked with one side always in perpetual darkness and the other in light then the only habitable zone tempertature-wise would be the line between shadow and light (known as the "terminator"). The planet's almost circular orbit will tend to keep this zone fairly stable. However, having a mass three to four times that of Earth means that we weigh more there and will probably have to exert ourselves considerably more just to get about. Neither is a twenty light year distance a paltry consideration in view of our present technology since it would take a spacecraft traveling at Voyager speed well over 70,000 years to get to Alpha Centauri which is apprtox 4 ly away and approx. 350,000 years to get to Gliese.

>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>>

Excerpt:

horseshoe7 Wrote:

However, if my calculations are correct, my 200lb body would feel like about 867lbs on the surface of Gliese 581 d... even if I went on a crash diet to get to ~150lbs, I'd STILL weigh about 650 pounds there!... maybe we need to "continue the seach" for more suitable habitable planets? ... hopefully, there is a more Earth-sized planet Gliese 581 f that is right in the middle of the habitable zone of the Gliese 581 system?


https://www.physicsforums.com/showthread.php?t=359589
 
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  • #64
GlieseWorm said:
i have only read of one blip being recorded and the next time they looked the blip didnt appear. to me , if me reading so far is correct, then this would seem to suggest that the confirmation is lacking and that the so called planet is an artefact. combined with the other data that suggests 4 planets not 6, it seems a bit early to come to conclusions about the planet being tidally locked.
Strictly speaking, it's not a burst of something, it's spectroscopic data.

One uses spectroscopy to measure a star's radial velocity, repeating the measurements over several hours or days or weeks or months or years. One then tries to fit the effect of an orbiting planet to what one observes.

The problem with Gliese 581g is that it does not produce a very strong effect, if it exists. It's barely above the noise.
 
  • #65
Vanadium 50 said:
Before we get too excited, red dwarfs have some problems. One is that many of them - perhaps half - are UV Ceti variables, also called flare stars. They have sporadic flares which are much more dangerous than solar flares - both because they are more energetic (especially in X-rays) and because their planets are closer.

Unfortunately, Gl 581 falls into this category. (When looking it up, it's also NSV 7023. NSV stands for New Suspected Variable)

Unfortunately, the closest star to earth, Proxima Centauri, also falls under that unpredictable red dwarf variable category.
 
  • #66
Emphasis added in quote.
GlieseWorm said:
Thus, DaveC426913, with all due respect, it appears that you are quoting the wrong article in your criticism of the conclusions about the nature of the planet, as you have referenced Camilo et al (2000). I can't see how it could be referring to any planets as there have yet to be any planets detected in this entire galaxy, again according to Wikipedia today.


Huh? We've already detected hundreds of exoplanets in the Milky Way, starting in 1992.
http://en.wikipedia.org/wiki/Exoplanet_detection
http://en.wikipedia.org/wiki/PSR_B1257+12
http://en.wikipedia.org/wiki/Extrasolar_Planet
Wikipedia said:
There are 538 such planets that have been confirmed as of March 11, 2011.
Of course, the number of known exoplanets was lower at the time of your post, but much higher than 0.
 
  • #67
FtlIsAwesome said:
Huh?
Yeah. Who knows what he means...
 

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