Explore Westonci.ca, the premier Q&A site that helps you find precise answers to your questions, no matter the topic. Join our Q&A platform to get precise answers from experts in diverse fields and enhance your understanding. Connect with a community of professionals ready to provide precise solutions to your questions quickly and accurately.

the conditions on the surface of venus are; mars has a period and direction of rotation that are; the clouds in the atmosphere of venus consist primarily of; an earth-based telescopic view of venus shows; when venus is at its brightest as seen from the earth (near greatest elongation) it is; the internal structure of mercury is most likely a; mercury looks very similar to which planet or satellite in our solar system; the most common surface features on venus are

Sagot :

Craters, volcanoes, mountains, and vast lava plains characterize the terrain. Consequently, Mars and Earth both rotate in the same way (counterclockwise if you look down on the solar system from North of the ecliptic). On Mars, the Sun will always rise in the East, using the same definition of East as on Earth.

In several ways, Mercury common to the moon of Earth. Venus' atmosphere is 96% carbon dioxide. Sulfuric acid is used to make thick clouds between 30 and 60 kilometers in altitude, and the greenhouse effect of CO2 keeps the surface temperature high. The Sun-Earth-Venus angle allows us to observe the planet at its brightest at two points during its orbit. When Venus is at an elongation of 39°, roughly 36 days before and after inferior conjunction, these phenomena—known as peak brilliancy—occur.

Around 85% of the planet's radius, or 1,289 miles (2,074 kilometers), is made up of a substantial metallic core. It appears to be partially molten or liquid based on the evidence. Similar to the mantle and crust of Earth, Mercury's outer layer is only around 400 kilometers (250 miles) thick. Despite Mercury being closer to the Sun, it is the planet with the highest temperature in our solar system. Venus's surface reaches temperatures of roughly 900 °F (475 °C), which are hot enough to melt lead.

The surface is rust-colored, covered in thousands of massive volcanoes, strongly crushed mountains, and other geological features. Venus's surface is obscured by dense clouds, so we can't see it from Earth. But as our understanding of Venus has grown, we now know that the planet's surface is dotted with craters, volcanoes, mountains, and enormous lava plains.

Learn more about venus visit: brainly.com/question/28479993

#SPJ4

Thanks for using our platform. We aim to provide accurate and up-to-date answers to all your queries. Come back soon. Thanks for using our service. We're always here to provide accurate and up-to-date answers to all your queries. We're here to help at Westonci.ca. Keep visiting for the best answers to your questions.