Warning: foreach() argument must be of type array|object, bool given in /var/www/html/web/app/themes/studypress-core-theme/template-parts/header/mobile-offcanvas.php on line 20

Give a brief description of Mercury, Include its atmosphere, surface temperature, surface features, and speed of rotation about its axis.

Short Answer

Expert verified
Mercury has a thin atmosphere, severe temperature variations, a cratered surface, and rotates once every 59 Earth days.

Step by step solution

01

Understanding Mercury's Atmosphere

Mercury has a very thin atmosphere composed mostly of oxygen, sodium, hydrogen, helium, and potassium. Because its atmosphere is so tenuous, it cannot retain heat, leading to extreme temperature fluctuations.
02

Analyzing Surface Temperature

The surface temperature on Mercury varies significantly due to its thin atmosphere. Daytime temperatures can soar up to about 430°C (800°F) while nighttime temperatures can drop to -180°C (-290°F).
03

Examining Surface Features

Mercury's surface is heavily cratered, similar to that of the Moon, and has large plains. The planet has features such as cliffs, or "scarps," that are hundreds of kilometers long, formed by the cooling and contracting of the planet over billions of years.
04

Understanding Rotation Speed

Mercury rotates very slowly on its axis. It takes about 59 Earth days to complete one rotation. Interestingly, despite its slow rotation, it orbits the Sun quickly, completing an orbit every 88 Earth days.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Planetary Atmosphere of Mercury
Mercury’s atmosphere is extremely thin, also referred to as an exosphere. Unlike Earth, Mercury's atmosphere doesn't contain enough particles to reflect sunlight or trap heat. It is mainly composed of oxygen, sodium, hydrogen, helium, and potassium. This thin layer is not able to hold heat, which results in the planet experiencing extreme temperature changes immediately as it spins. Such a delicate balance makes Mercury’s environment harsh and dynamic. The tenuous nature of this atmosphere makes it difficult for life as we know it to exist there.
Mercury's Surface Temperature Extremes
Due to the sparse atmosphere, Mercury experiences dramatic swings in temperature from day to night. During the day, temperatures can reach up to 430°C (800°F). This intense heat is a result of its proximity to the Sun and lack of atmospheric protection. At night, the temperature plummets to around -180°C (-290°F). These extremes stem from the planet's inability to retain heat once the sun sets. The swift temperature changes are one of the most distinctive attributes of Mercury, contributing to its unique surface environment.
Surface Features of Mercury
Mercury's surface shares similarities with our Moon, largely characterized by numerous impact craters and smooth plains. This resemblance arises from countless collisions with asteroids and comets over billions of years. Some notable features include vast cliffs known as 'scarps,' which stretch for hundreds of kilometers. These cliffs were formed as Mercury's interior cooled and contracted. Such geological formations reveal much about the planet's history and its cooling process, offering a window into the dynamic past of this rocky world.
Mercury's Slow Planetary Rotation
The rotation of Mercury is intriguingly slow. It requires about 59 Earth days for Mercury to rotate once on its axis. However, despite this lethargic rotation, Mercury is quite fast when orbiting the Sun, completing one full orbit in just 88 Earth days. This means that a single day on Mercury (sunrise to sunrise) lasts for about 176 Earth days due to its unique 3:2 spin-orbit resonance. This slow rotation and rapid orbiting pattern contribute to its extreme temperature variations and have fascinated astronomers who study planetary motion.

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Study anywhere. Anytime. Across all devices.

Sign-up for free