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Two Earth-size planets that orbit each other might exist around distant stars, researchers say.
The solar system has many examples of moons orbiting planets; Jupiter and Saturn both possess more than 60 satellites. However, these moons are usually much smaller than their planets — Earth is nearly four times wider than its moon and more than 80 times its mass.
Still, some moons are as large as planets. For instance, Ganymede, Jupiter's largest moon, is larger than Mercury, and three-quarters the diameter of Mars. Also, moons at times are nearly as large as their worlds; Pluto's largest moon, Charon, is about half the diameter of the dwarf planet itself. This raises the intriguing possibility that planets of equal size could orbit each other.
The scientists ran about two dozen simulations. However, these simulations often resulted in the planets colliding, typically merging or accreting together into a larger planet and sometimes leaving behind a disk of debris from which a moon could form. Also, in some simulations, the planets collided in a grazing manner at high speeds, resulting in "hit and run" interactions in which the worlds escaped from one another.
Still, about one-third of the simulations resulted in binary planets forming. These involved relatively slow, grazing collisions.
"Previously, the only expected outcomes of large-body impacts of this sort were escape or accretion — that is, either the two bodies do not stay together or they merge into one, occasionally with a disk of debris," study co-author Keegan Ryan, an undergraduate student at the California Institute of Technology in Pasadena, told Space.com. "Our findings suggest the possibility of another outcome — binary planets. The bodies stay mostly intact, but end in a bound orbit with one another."
These binary planets would loom extraordinarily close to one another, separated by a distance of about half the diameter of each of the worlds. Over time, the rate at which both planets spin would fall into lockstep, with each world only turning one face toward its partner.
Such binaries can persist for billions of years, researchers say, provided they form at least half an astronomical unit or more away from their parent stars — far enough away for the star's gravitational pull to not disrupt the binary planet system. (One astronomical unit, or AU, is the average distance between the sun and Earth, about 93 million miles, or 150 million kilometers.)
originally posted by: swanne
a reply to: JadeStar
Regarding the possibility of life there, I am more concerned about the gravitational pull on one planet over the other and how this could affect the shape of the planets, if not their water distribution or period of rotation.
Extraordinary find nevertheless, a definitive S&F from me!
originally posted by: Iamschist
a reply to: JadeStar
Wonderful thread, and wow. The tides on a planet with a binary planet companion. Surfs up! lol I wonder what kind of civilizations would develop? I agree the inhabitants learn flight early to get to the other planet. Could two separate life forms develop? I hope the resources on each planet are equal.
For some reason I keep thinking of that Star Trek episode with the two races of half black and half white people, just on opposite sides and how they hated each other. Hopefully it would all be nice and peaceful.
Our moon stabilizes our planet's spin around its orbital access. Two relatively equally sized planets would do the same for each other.
originally posted by: intrptr
a reply to: JadeStar
Our moon stabilizes our planet's spin around its orbital access. Two relatively equally sized planets would do the same for each other.
I thought hey would pull into each other, slowly closing the distance and then joining in a cataclysm?
Isn't that why all "moons' are smaller than their "planets"?
If unequal in mass the pull of gravity finds a Lagrange point to settle into. If equal in mass they both pull each other together?
I don't really know what I'm talking about, just not seeing any body in our solar system with an equal "partner".
I asked this question once in high school physics class and my teacher told me in no uncertain terms that a double planet system would be nearly impossible because of that.
originally posted by: intrptr
a reply to: JadeStar
Our moon stabilizes our planet's spin around its orbital access. Two relatively equally sized planets would do the same for each other.
I thought hey would pull into each other, slowly closing the distance and then joining in a cataclysm? Isn't that why all "moons' are smaller than their "planets"?
If unequal in mass the pull of gravity finds a Lagrange point to settle into. If equal in mass they both pull each other together?
I don't really know what I'm talking about, just not seeing any body in our solar system with an equal "partner".
in our moons case it's the tidal forces and "sloshing" that are actually pushing the moon away. when it first formed it would have filled a huge portion of the sky. trying to remember the figure… i wanna say it moves away about an inch a year?
originally posted by: stormbringer1701
related topic: Did you read the article about scientists have figured out a way to characterize the magnetic fields of exo-planets. this is important in determining if a exo-earth is protected from stellar and cosmic rays like earth is. it is one more thing that would be used to determine potential probe targets, additional scope time, and even colonization targets.
www.sciencedaily.com...
im way to multi-tasked to do it now. we'll see who gets to it. i only have a little to say about it beyond the article, anyway.
originally posted by: JadeStar
originally posted by: stormbringer1701
related topic: Did you read the article about scientists have figured out a way to characterize the magnetic fields of exo-planets. this is important in determining if a exo-earth is protected from stellar and cosmic rays like earth is. it is one more thing that would be used to determine potential probe targets, additional scope time, and even colonization targets.
www.sciencedaily.com...
Yes! I was just about to post something about this but please go ahead and post it up and talk about it cause i'm kinda snowed under with work.
in the past an astronomer thought he detected a gas giant at barnards star. (the same thing happened with proxima as well) so for a while everyone thought banard's star was the place to go. unfortunately subsequent searchers ruled out anything larger than neptune i believe and no wobble or transit was observed above statistical noise level. still that does not mean barnard's star does not have smaller planets. it will be interesting in the next decade to see which of the abundant dwarf stars in our neigborhood turn out to have planets. i mean there are a lot of them.
originally posted by: PrinceRupertsDog
a reply to: JadeStar
There is a sci-fi novel from the 1980s calledFlight of the Dragonfly, where a mission to Barnard's Star is undertaken. They arrive and discover a binary planetary system. The original version of tbe book was interesting. The author later updated the book, added some sex scenes that was written by his wife. Still, it was/is an interesting premise. It would actually make a good movie.
M dwarfs such as Barnard's Star are more easily studied than larger stars in this regard because their lower masses render perturbations more obvious.[42] Gatewood was thus able to show in 1995 that planets with 10 times the mass of Jupiter (the lower limit for brown dwarfs) were impossible around Barnard's Star,[38] in a paper which helped refine the negative certainty regarding planetary objects in general.[43] In 1999, work with the Hubble Space Telescope further excluded planetary companions of 0.8 times the mass of Jupiter with an orbital period of less than 1,000 days (Jupiter's orbital period is 4,332 days),[4] while Kuerster determined in 2003 that within the habitable zone around Barnard's Star, planets are not possible with an "M sin i" value[44] greater than 7.5 times the mass of the Earth, or with a mass greater than 3.1 times the mass of Neptune (much lower than van de Kamp's smallest suggested value).[18]
Even though this research has greatly restricted the possible properties of planets around Barnard's Star, it has not ruled them out completely; terrestrial planets would be difficult to detect. NASA's Space Interferometry Mission, which was to begin searching for extrasolar Earth-like planets, was reported to have chosen Barnard's Star as an early search target.[23] However, this mission was shut down in 2010.[45] ESA's similar Darwin interferometry mission had the same goal, but was stripped of funding in 2007.[46]
Proxima Centauri b?
Using data collected up to early 1994, astronomers using the Hubble Space Telescope discerned a 77-day variation in the proper motion of Proxima (Benedict et al, 1994). The astrometric perturbations found could be due to the gravitational pull of a large planet with about 80 percent of Jupiter's mass at a 1994 separation from Proxima of about 0.17 AUs -- 17 percent of Earth's orbital distance in the Solar System from the distance, or less than half Mercury's orbital distance. The Hubble astrometry team calculated that the chance of a false positive reading from their data -- same perturbations without a planet -- to be around 25 percent.
© Estate of John Whatmough -- larger image
(Artwork from Extrasolar Visions, used with permission from Whatmough)
Glowing red through gravitational contraction, the candidate brown dwarf companion
to Proxima Centauri is depicted with two moons (one eclipsing the flare star) with
distant Alpha Centauri A and B at upper right, as imagined by Whatmough.
In 1996, another group of astronomers using the Hubble Space Telescope discovered that they might have directly observed a companion to Proxima with the implied brightness of a brown dwarf and an apparent visual separation of only about half the Earth-Sun distance -- 0.5 AU (Schultz et al, 1998). A substellar companion at that distance would imply an orbital period of around a year, or it could be in a highly eccentric orbit with a much greater average distance from Proxima. However, later observations by other astronomers using interferometric astrometry and recent radial velocity data found no evidence to support the existence of a companion greater than 0.8 Jupiter mass with an orbital period around Proxima Centauri of between one and about 2.7 years (Benedict et al, 1999). Proxima has been selected to be one of the Tier 1 target stars for NASA's Space Interferometry Mission (SIM) -- which is planned for launch as early as 2011 -- to detect a planet as small as three Earth-masses within two AUs of its host star.