As Dawn approaches, new image of dwarf planet Ceres



Dwarf planet Ceres as captured by Dawn spacecraft on December 1, 2014. Dawn will arrive at Ceres in March, 2015.

View larger. | Dwarf planet Ceres seen by Dawn spacecraft on December 1. A smaller, correctly exposed image has been enlarged. Resolution 108 kilometers. Image via NASA / JPL DAWN spacecraft.



Here, the 976-kilometer-wide / 606-mile-wide main belt asteroid / protoplanet / dwarf planet 1 Ceres is seen by the approaching Dawn spacecraft from a distance of 1.2 million kilometers / 745,000 miles, on December 1, 2014. Dawn begins its approach phase toward Ceres on December 26 and will arrive at Ceres in March, 2015.


These are test images and 1 Ceres appears only nine pixels wide at this point, perfect for a far-encounter camera calibration.


The main image shows 1 Ceres overexposed with a few background stars within the constellation of Ophiuchus the Serpent Bearer.


Click here for full sized image.


Click here for original uncropped correctly exposed view.


1 Ceres is the largest and most massive of all of the members of the main asteroid belt between the orbits of Mars and Jupiter. 1 Ceres orbits the sun at an average distance of 414 million kilometers / 257 million miles once every 4 years and 218 days.


1 Ceres appears to have a density of 2.09 g/cm3, suggesting 70% rock and 30% ice in composition, very similar ratios to KBOs / Dwarf planets Eris and Pluto.


There have been suggestions that 1 Ceres did indeed originate in the Kuiper Belt then was ejected inwards and was sent into an orbit within the asteroid belt by Jupiter. Myself, I do not think that is the case. I think 1 Ceres formed close to the current orbit, when the infant sun was approximatelyt 30% dimmer than now, so that region was much colder than now, and that Jupiter prevented 1 Ceres from forming into a fully-fledged planet. Jupiter may also had stunted the growth of Mars and asteroids / protoplanets 2 Pallas, 4 Vesta and 10 Hygeia.


A recent discovery made by the Hubble Space Telescope suggests minor plume activity when 1 Ceres is at perihelion, closest point to the sun, at 382.5 million kilometers / 237.5 million miles with plume activity lining up with two large impact craters, showing that two relatively recent impacts have exposed ice rich materials. We’ll see in March, 2015.


1 Ceres rotates once ever 9 hours 4 minutes in a prograde west to east direction.


The surface gravity of 1 Ceres is 0.029 or 1/34th that on Earth.






from EarthSky http://ift.tt/1w9LOXZ

Dwarf planet Ceres as captured by Dawn spacecraft on December 1, 2014. Dawn will arrive at Ceres in March, 2015.

View larger. | Dwarf planet Ceres seen by Dawn spacecraft on December 1. A smaller, correctly exposed image has been enlarged. Resolution 108 kilometers. Image via NASA / JPL DAWN spacecraft.



Here, the 976-kilometer-wide / 606-mile-wide main belt asteroid / protoplanet / dwarf planet 1 Ceres is seen by the approaching Dawn spacecraft from a distance of 1.2 million kilometers / 745,000 miles, on December 1, 2014. Dawn begins its approach phase toward Ceres on December 26 and will arrive at Ceres in March, 2015.


These are test images and 1 Ceres appears only nine pixels wide at this point, perfect for a far-encounter camera calibration.


The main image shows 1 Ceres overexposed with a few background stars within the constellation of Ophiuchus the Serpent Bearer.


Click here for full sized image.


Click here for original uncropped correctly exposed view.


1 Ceres is the largest and most massive of all of the members of the main asteroid belt between the orbits of Mars and Jupiter. 1 Ceres orbits the sun at an average distance of 414 million kilometers / 257 million miles once every 4 years and 218 days.


1 Ceres appears to have a density of 2.09 g/cm3, suggesting 70% rock and 30% ice in composition, very similar ratios to KBOs / Dwarf planets Eris and Pluto.


There have been suggestions that 1 Ceres did indeed originate in the Kuiper Belt then was ejected inwards and was sent into an orbit within the asteroid belt by Jupiter. Myself, I do not think that is the case. I think 1 Ceres formed close to the current orbit, when the infant sun was approximatelyt 30% dimmer than now, so that region was much colder than now, and that Jupiter prevented 1 Ceres from forming into a fully-fledged planet. Jupiter may also had stunted the growth of Mars and asteroids / protoplanets 2 Pallas, 4 Vesta and 10 Hygeia.


A recent discovery made by the Hubble Space Telescope suggests minor plume activity when 1 Ceres is at perihelion, closest point to the sun, at 382.5 million kilometers / 237.5 million miles with plume activity lining up with two large impact craters, showing that two relatively recent impacts have exposed ice rich materials. We’ll see in March, 2015.


1 Ceres rotates once ever 9 hours 4 minutes in a prograde west to east direction.


The surface gravity of 1 Ceres is 0.029 or 1/34th that on Earth.






from EarthSky http://ift.tt/1w9LOXZ

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