Bilingual edition: English is preserved and Chinese follows each unit. Terminology uses the confirmed v20260916 glossary; automated semantic review remains traceable.
中英双语版:英文原文完整保留,中文紧随对应单元;术语采用 v20260916 确认表,自动语义审校结果可追溯。

Ceres

谷神星

Image credit: NASA Dawn site

The Dawn spacecraft reached Ceres on March 6, 2015 and as of this writing in August 2015, it remains in orbit around Ceres.

Ceres is the largest of the asteroids and orbits the Sun in the main asteroid belt between the orbits of Mars and Jupiter. It is 940 kilometers in diameter and has about 1/10000 the mass of the Earth. With over 7000 asteroids catalogued, the total number may exceed 100,000. However, their combined mass is less than 1/10 that of the Earth's Moon. The Dawn spacecraft's measurement of Ceres' mass is 9.39 x 1020kg, which would suggest that it contains about a third of the estimated mass of the asteroid belt, but amounts to about 4% of the mass of the Earth's moon. Reference Dawn Journal, 5/28/15

谷神星是最大的小行星,其轨道位于火星和木星之间的主小行星带中。它的直径为940公里,质量约为地球的1/10000。目前已 catalogued 超过7000颗小行星,总数可能超过100,000颗。然而,它们的总质量不到地球月球质量的1/10。Dawn探测器测量出谷神星的质量为9.39 x 10²⁰ kg,这表明它包含估计小行星带总质量的大约三分之一,但仅占月球质量的约4%。参考Dawn Journal,5/28/15

The feature that immediately drew attention were these bright spots in a crater named Occator. At least eight spots can be seen next to the largest bright area, which scientists think is approximately 6 miles (9 kilometers) wide. A highly reflective material is responsible for these spots -- ice and salt are leading possibilities, but scientists are considering other options, too.

最引人注目的特征是位于名为Occator的撞击坑中的这些明亮斑点。在最大的明亮区域旁边至少可以看见八个斑点,科学家认为该区域大约宽6英里(9公里)。这些斑点的成因是一种高反射率的物质——冰和盐是可能的解释,但科学家也考虑了其他可能性。

This enhanced image of the Occator crater is exaggerated by a factor of 5 in the vertical dimension.

这张增强的Occator撞击坑图像在垂直方向上被放大了5倍。

"In addition to the bright spots, the latest images also show a mountain with steep slopes protruding from a relatively smooth area of the dwarf planet's surface. The structure rises about 3 miles (5 kilometers) above the surface." NASA

除明亮的斑点外,最新图像还显示了一座山峰从矮行星表面相对平滑的区域突起,山体坡度陡峭。该结构高出表面约3英里(5公里)。NASA

Maybe that bump on the bottom side of this photo doesn't look all that impressive, but it is a 3-mile-high mountain!

也许这张照片底部的那座山看起来并不那么壮观,但它高达3英里!
Dawn探测器于2015年3月6日抵达谷神星,并截至2015年8月本文写作时,它仍围绕谷神星运行。

Ceres was discovered on Jan. 1, 1801 by Giuseppe Piazzi of Italy. Ceres may have formed later than Vesta, and with a cooler interior. Current evidence suggests that Vesta only retained a small amount of water because it formed earlier, when radioactive material was more abundant, which would have produced more heat. Ceres, in contrast, has a thick ice mantle and may even have an ocean beneath its icy crust. Ceres, with an average diameter of 590 miles (950 kilometers), is also the largest body in the asteroid belt, the strip of solar system real estate between Mars and Jupiter. By comparison, Vesta has an average diameter of 326 miles (525 kilometers), and is the second most massive body in the belt.

谷神星于1801年1月1日由意大利的吉useppe皮亚齐发现。谷神星可能比灶神星形成得更晚,且内部更冷。目前的证据表明,灶神星由于形成时放射性物质更丰富,因此只保留了少量的水,这会使其在形成时产生更多的热量。相比之下,谷神星拥有厚厚的冰层,甚至可能在其冰壳之下有海洋。谷神星的平均直径为590英里(950公里),也是小行星带中最大的天体,位于火星和木星之间的太阳系区域。相比之下,灶神星的平均直径为326英里(525公里),是小行星带中第二大的天体。
图片版权:NASA Dawn 网站
Index

Solar System Illustration

Solar System Concepts

Reference
Chaisson and McMillan
Ch 14
索引 太阳系图示 太阳系概念 参考 Chaisson 和 McMillan 第14章
 
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HyperPhysics ********** 天体物理学
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