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JadeStar
If a mod can let me know its ok to post this as its own new thread I will
JadeStar
As you can see habitable planets larger than the Earth but smaller than the large planets of our own solar system seem to be more plentiful than planets like the Earth.
Ross 54
A problem here is that most of the short ETs are said to be gracile, thin, or lightly constructed. This would suggest their origin on worlds with less than terrestrial gravity.
As small, red M class stars have become recognized as promising abodes for life, we might consider these in this context. As quite small stars, they seem likely to produce, on average, relatively small planets, with comparatively weak gravity.
We also have numerous descriptions of extraterrestrials with conspicuously large eyes. These could be a good adaptation to the limited, long wavelength light on a tidally locked planet of a red dwarf star.
Galileo400
Ross 54
A problem here is that most of the short ETs are said to be gracile, thin, or lightly constructed. This would suggest their origin on worlds with less than terrestrial gravity.
As small, red M class stars have become recognized as promising abodes for life, we might consider these in this context. As quite small stars, they seem likely to produce, on average, relatively small planets, with comparatively weak gravity.
We also have numerous descriptions of extraterrestrials with conspicuously large eyes. These could be a good adaptation to the limited, long wavelength light on a tidally locked planet of a red dwarf star.
I could not agree more. And if it is true that the greys come from such a world, I bet they hate that on Earth they are so heavy and the Sun is so bright. I bet their skin would sunburn like a redhead's.
You may be correct about the general superiority of planets of Sun-like stars as abodes of sentient life. We know too little about such matters to say anything in more than speculative terms. And, yes, I agree that a planet brightly lit by a G class star could still have low light environments-- jungles, dense forests, and perpetually overcast skies all being possibilities.
tanka418
Galileo400
Ross 54
A problem here is that most of the short ETs are said to be gracile, thin, or lightly constructed. This would suggest their origin on worlds with less than terrestrial gravity.
As small, red M class stars have become recognized as promising abodes for life, we might consider these in this context. As quite small stars, they seem likely to produce, on average, relatively small planets, with comparatively weak gravity.
We also have numerous descriptions of extraterrestrials with conspicuously large eyes. These could be a good adaptation to the limited, long wavelength light on a tidally locked planet of a red dwarf star.
I could not agree more. And if it is true that the greys come from such a world, I bet they hate that on Earth they are so heavy and the Sun is so bright. I bet their skin would sunburn like a redhead's.
Actually; it is highly improbable that advanced sentient life would evolve around a class "M" star, even the bright ones.
It is a far better bet that these large eyed people from Reticuli are from a "G" class star. Its actually pretty easy to evolve in a "reduced" light environment even near a "G" star.
Ross 54
You may be correct about the general superiority of planets of Sun-like stars as abodes of sentient life. We know too little about such matters to say anything in more than speculative terms. And, yes, I agree that a planet brightly lit by a G class star could still have low light environments-- jungles, dense forests, and perpetually overcast skies all being possibilities.
2009 Post: A nearby Sun-like star in the constellation Andromeda regarded as a promising candidate for habitability if it possesses any Earth-like planets within its habitable zone. It ranks in the top five stars most likely to support life in a shortlist drawn up in 2006 by astrobiologist Margaret Turnbull, one of the authors of HabCat (Catalog of Nearby Habitable Systems).]/i]
The presence of a moderately close companion could disrupt the orbit of a hypothetical planet in HD 10307's habitable zone. However, the uncertainty of the orbital parameters makes it equally uncertain exactly where stable orbits would be in this system.
It was transmitted from Eurasia's largest radar, 70-meter Eupatoria Planetary Radar. The message was named Cosmic Call 2, it was sent on July 6, 2003, and it will arrive at HD 10307 in September 2044.
2009 Post: Not a lot of information found on this star. However, data indicates it is a F5V or F6V star, most likely aged between 4 and 6 billions of years. That is potentially a "sun like" star.
2009 Post: The most Sun-like of the 30 nearest stars to the Sun.
It is not known if the star is accompanied by any planets – its low metallicity makes it questionable whether the nebula from which it condensed had sufficient heavy element content to allow planet-sized objects to form). However, if any planets are present, (...) they are likely to be subjected to a much more intense bombardment than anything the Earth has experienced, making the survival of any life problematic.
2009 Quote No large substellar companion has been found thus far (Murdoch et al, 1993). However, the distance from 82 Eridani A where an Earth-type planet would be "comfortable" with liquid water is centered around 0.80 AU -- midway between the orbital distances of Venus and Earth in the Solar System. At that distance from the star, such a planet would have an orbital period of almost 275 days, or over two thirds of an Earth year. Astronomers are hoping to use NASA's Terrestrial Planet Finder (TPF) and the ESA's Darwin planned groups of observatories to search for a rocky inner planet in the so-called "habitable zone" (HZ) around 82 Eridani. As currently planned, the TPF will include two complementary observatory groups: a visible-light coronagraph to launch around 2014; and a "formation-flying" infrared interferometer to launch before 2020, while Darwin will launch a flotilla of three mid-infrared telescopes and a fourth communications hub beginning in 2015.Furthermore, this star is estimated over 10 billions years old. This leaves a lot of time for any potential life around it to be much more advanced than we are! .
On August 17, 2011, European astronomers announced the discovery of three planets orbiting 82 G. Eridani. The mass range of these planets classifies them as super-Earths; objects with only a few times the Earth's mass. These planets were discovered by precise measurements of the radial velocity of the star, with the planets revealing their presence by their gravitational displacement of the star during each orbit. None of the planets display a significant orbital eccentricity. However, their orbital periods are all 90 days or less, indicating that they are orbiting close to the host star. The equilibrium temperature for the most distant planet, based on an assumed Bond albedo of 0.3, would be about 388 K (115 °C); significantly above the boiling point of water.
The number of planets in the system is slightly uncertain. At the time of planet c's detection, it exerted the lowest gravitational perturbation. There was also a similarity noted between its orbital period and the rotational period of the star. For these reasons the discovery team were somewhat more cautious regarding the verity of its candidate planet status than for the other two.Continued observation of the star will be required to determine the exact nature of the planetary system.
Ross 54
Found this image, which gives an idea of the three dimensional space occupied by the group of stars selected by Marjorie Fish as most closely resembling the Betty Hill star map. www.ufoconspiracy.com/images/zbetty.gif
They seem to have gone a long trip (37 light years), without any stops along the way, to visit Earth. A longer voyage, by far, than to any other single star.
Perhaps we should feel flattered.edit on 27-10-2013 by Ross 54 because: added information