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The objects, left to right are: 1 dwarf planet Ceres, 2 Pallas, 3 Juno, 4 Vesta, 5 Astraea, 6 Hebe, 7 Iris, 8 Flora, 9 Metis, and 10 Hygiea. The scale is 10 km/px on the original image, though not necessarily on the repro here.
At most oppositions, however, Juno only reaches a magnitude of around +8.7 [24] —only just visible with binoculars—and at smaller elongations a 3-inch (76 mm) telescope will be required to resolve it. [25] It is the main body in the Juno family. Juno was originally considered a planet, along with 1 Ceres, 2 Pallas, and 4 Vesta. [26]
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Both Vesta and Pallas have assumed the title of second-largest asteroid from time to time. [47] At 513 ± 3 km in diameter, [ 9 ] Pallas is slightly smaller than Vesta ( 525.4 ± 0.2 km [ 48 ] ). The mass of Pallas is 79% ± 1% that of Vesta, 22% that of Ceres, and a quarter of one percent that of the Moon .
dmoz page for Solar System; Origin of the Solar System (outline) A Cosmic History of the Solar System; A Tediously Accurate Map of the Solar System (web based scroll map scaled to the Moon being 1 pixel) NASA/JPL Solar System main page. NASA's Solar System Simulator; Solar System Profile by NASA's Solar System Exploration
The next largest are 4 Vesta and 2 Pallas, both with diameters of just over 500 km (300 mi). Vesta is the brightest of the four main-belt asteroids that can, on occasion, be visible to the naked eye. [70] On some rare occasions, a near-Earth asteroid may briefly become visible without technical aid; see 99942 Apophis.
The timeline of discovery of Solar System planets and their natural satellites charts the progress of the discovery of new bodies over history. Each object is listed in chronological order of its discovery (multiple dates occur when the moments of imaging, observation, and publication differ), identified through its various designations (including temporary and permanent schemes), and the ...
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