It looks like you're using an Ad Blocker.
Please white-list or disable AboveTopSecret.com in your ad-blocking tool.
Some features of ATS will be disabled while you continue to use an ad-blocker.
You know we’ve found something new and interesting when scientists don’t really know how to classify it. Using the Subaru Telescope an international team of astronomers has discovered a “super-Jupiter” so massive that it seems they’re not quite sure whether to call it a planet or a low-mass brown dwarf (in other words, a star that failed to fire). Located roughly 170 light-years from Earth, the host star is roughly 2.5 times more massive than the sun and its planet is about 13 times larger than Jupiter, making this the highest-mass star to ever host a directly imaged orbital companion--especially one of this size. Kappa Andromedae is part of what’s known as the Columba stellar moving group, and at just 30 million years old it is relatively young (our Sun is estimated to be more like five billion hears old). That’s significant if only for the mode of discovery--young stars are good targets for directly imaging exoplanets because their planets (also young) tend to retain more heat leftover from the formation process and thus reveal themselves more readily via infrared emissions. That’s how the researchers were able to zero in on Kappa And b, the super-Jupiter orbiting Kappa Andromedae at a distance about 1.8 times Neptune’s distance from the Sun, over the glare of its host star. RELATED ARTICLES Largest Known Exoplanet Discovered Astronomers Capture First Images of an Exoplanet Orbiting Its Star Freshly Discovered Earth-Like Planet Orbiting Nearby Star Could Be the First Truly Habitable Exoplanet TAGS Technology, Clay Dillow, exoplanets, kappa and b, kappa andromedae, Space, super-jupiterAll of this is scientifically significant because according to the way we understand both star formation and planetary formation there are parameters that determine whether objects of certain masses can do certain things, and both Kappa Andromedae and its orbiting super-object sit at interesting places within these parameters. In theory, Kappa And b probably falls just shy of being massive enough to trigger internal fusion--it is right on the brink of potentially becoming a star (hence the speculation that it might be better classified as a brown dwarf). And as for Kappa Andromedae, its 2.5 solar masses demonstrate that stars its size are capable of producing these huge orbiting bodies--super-planets relative to those found in our solar system--in their planetary discs. That’s something that some theorists thought impossible due to the massive amount of radiation these stars put off (the idea is that this radiation would interfere with the normal planet formation process that takes place around smaller stars like the Sun). So the strange case of Kappa Andromedae and super-Jupiter Kappa And b gives astronomers some things to think about. The team that discovered it plans to keep the Subaru Telescope trained on it for awhile to better defines the planet’s chemistry and orbital characteristics, which will further their understanding of exactly what is going on over there.
Currently, the International Astronomical Union considers an object with a mass above the limiting mass for thermonuclear fusion of deuterium (currently calculated to be 13 Jupiter masses for objects of solar metallicity) to be a brown dwarf, whereas an object under that mass (and orbiting a star or stellar remnant) is considered a planet.
Originally posted by inverslyproportional
... its planet is about 13 times larger than Jupiter
A remarkable property of brown dwarfs is that they are all roughly the same radius as Jupiter. At the high end of their mass range (60–90 Jupiter masses), the volume of a brown dwarf is governed primarily by electron-degeneracy pressure, as it is in white dwarfs; at the low end of the range (10 Jupiter masses), their volume is governed primarily by Coulomb pressure, as it is in planets. The net result is that the radii of brown dwarfs vary by only 10–15% over the range of possible masses. This can make distinguishing them from planets difficult.
It may be semantics.
People are still arguing about calling Pluto a "dwarf planet". So is it a planet or isn't it? If dwarf is an adjective, doesn't that still mean it's a planet, just a type of planet? And if it's not a planet, why are we still calling it a (insert adjective here) planet? Saying a dwarf planet isn't a planet is like saying a grizzly bear isn't a bear. I don't think we've heard the last of that.
Researchers on both sides of the debate gathered on August 14–16, 2008, at The Johns Hopkins University Applied Physics Laboratory for a conference that included back-to-back talks on the current IAU definition of a planet. Entitled "The Great Planet Debate", the conference published a post-conference press release indicating that scientists could not come to a consensus about the definition of a planet. Just before the conference, on June 11, 2008, the IAU announced in a press release that the term "plutoid" would henceforth be used to describe Pluto and other objects similar to Pluto which have an orbital semimajor axis greater than that of Neptune and enough mass to be of near-spherical shape.