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My intuition suggests that a planet far out and small would be very difficult to detect by its occlusion. This page calculates that Pluto for instance spans on
by foota 9y ago
My intuition suggests that a planet far out and small would be very difficult to detect by its occlusion.
This page calculates that Pluto for instance spans only 3 pixels at the Hubble space telescopes resolution: http://www.planetary.org/blogs/emily-lakdawalla/2013/02141014-hubble-galaxy-pluto.html http://www.planetary.org/blogs/emily-lakdawalla/2013/0214101...
- PhasmaFelis 9y agoIndeed. The article says that the hypothetical planet would be 2 pixels.
- BurningFrog 9y agoThe pixel size isn't what determines if occlusion happens. The planet and the star can both be much smaller than a pixel, as long as the planet is big enough to cover the star.
- 1024core 9y agoIf Hubble can barely see Pluto, how the heck did terrestrial telescopes find it in the first place?
- brobinson 9y agoWasn't the presence of a Pluto-like body _known_ because the orbits of other planets didn't match expectations based on the gravitational pulls of all the other known bodies in our solar system?
- simias 9y agoNot exactly. It's true that Neptune was discovered that way and that people found Pluto while looking for a "Planet X" that would explain other gravitational discrepancies: In the 1840s, Urbain Le Verrier used Newtonian mechanics to predict the position of the then-undiscovered planet Neptune after analyzing perturbations in the orbit of Uranus. Subsequent observations of Neptune in the late 19th century led astronomers to speculate that Uranus's orbit was being disturbed by another planet besides Neptune.[1] However it turned out that Pluto was not Planet X after all. After all Neptune and Uranus are respectively about 7900 and 6700 times more massive than Pluto. In 1978, the discovery of Pluto's moon Charon allowed the measurement of Pluto's mass for the first time: roughly 0.2% that of Earth, and far too small to account for the discrepancies in the orbit of Uranus. Subsequent searches for an alternative Planet X, notably by Robert Sutton Harrington, failed. In 1992, Myles Standish used data from Voyager 2's flyby of Neptune in 1989, which had revised the estimates of Neptune's mass downward by 0.5%—an amount comparable to the mass of Mars—to recalculate its gravitational effect on Uranus. With the new figures added in, the discrepancies, and with them the need for a Planet X, vanished. Today, the majority of scientists agree that Planet X, as Lowell defined it, does not exist. Lowell had made a prediction of Planet X's orbit and position in 1915 that was fairly close to Pluto's actual orbit and its position at that time; Ernest W. Brown concluded soon after Pluto's discovery that this was a coincidence, a view still held today.[2] [1] https://en.wikipedia.org/wiki/Pluto#Discovery https://en.wikipedia.org/wiki/Pluto#Discovery [2] https://en.wikipedia.org/wiki/Pluto#Planet_X_disproved https://en.wikipedia.org/wiki/Pluto#Planet_X_disproved
- Dylan16807 9y agoTo see something that acts like a point of light, size doesn't matter at all. Glowing objects are visible even when their area is a small fraction of a pixel. But your chances of noticing occlusion are much lower.