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Why is it impossible to see Mercury or Venus in the sky at midnight?

Short Answer

Expert verified
It is impossible to see Mercury and Venus in the sky at midnight due to their relative positions to Earth and the Sun. Because these planets orbit closer to the Sun than Earth, they are generally seen in the same direction as the Sun. At midnight, the Sun is on the opposite side of Earth and below the horizon; thus, making Mercury and Venus unobservable from Earth.

Step by step solution

01

Understanding the Orbit Positions

Firstly, recognize that Mercury and Venus are the two planets inside the Earth's orbit, closer to the Sun. This positioning causes them to always appear relatively close to the Sun from our vantage point here on Earth.
02

Consider Earth's Rotation

The Earth rotates on its axis about every 24 hours, causing the Sun to rise in the east and set in the west. The same effect is seen with the inner planets, Mercury and Venus. They rise and set in correlation with the Sun.
03

Think about Midnight Position

At midnight, the Earth has rotated to a position where the Sun is on the exact opposite side of the Earth. Consequently, any planets appearing close to the Sun in the sky would also be obscured from view.
04

Line of Sight to Mercury and Venus

Given our line of sight from Earth at midnight, the Sun is below the horizon (on the other side of the Earth) and therefore any planets, specifically Mercury and Venus in this case, that are near the Sun would also be below the horizon and thus not visible.

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Key Concepts

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

Mercury and Its Visibility
Mercury is the closest planet to the Sun, making it a fascinating yet elusive planet to observe from Earth. Due to its proximity to the Sun, Mercury never strays far from it in our sky. This means it is typically only visible around sunrise or sunset. When it's close to the Sun, either just after it sets or just before it rises, it is usually obscured by the Sun's bright light.
Even when Mercury is at its furthest apparent distance from the Sun, known as "greatest elongation," it never appears higher than 28 degrees above the horizon. Therefore, during the middle of the night, when the Sun is on the opposite side of the Earth, Mercury would also be below the horizon.
  • Closest planet to the Sun.
  • Visible only during dawn and dusk.
  • Max 28 degrees above horizon at greatest elongation.
Venus: The Evening and Morning Star
Venus, often called Earth's "sister planet" due to its similar size and composition, is the second planet from the Sun. Like Mercury, it is also located inside Earth's orbit in the solar system. Venus is renowned for its brilliant shine, earning it the moniker of the "Evening Star" when it appears after sunset, and the "Morning Star" when visible before sunrise.
Venus's orbit means it is only ever seen close to the Sun, never straying more than 47 degrees away. At midnight, when the Sun is on the opposite side of the Earth, Venus, being close to the Sun, is also not visible in the sky.
  • Considered Earth's sister planet.
  • Known as the "Evening Star" or "Morning Star."
  • Never more than 47 degrees away from the Sun.
Understanding Earth's Rotation
The rotation of the Earth is a key factor in the visibility of celestial objects like Mercury and Venus. Earth rotates on its axis once approximately every 24 hours. This rotation causes the Sun, Moon, stars, and planets to appear to move across the sky. As the Earth spins, different parts of the planet are exposed to sunlight while others are cast into night.
Because of this rotation, the Sun rises in the east and sets in the west, and planets that appear close to the Sun, such as Mercury and Venus, will follow a similar path. At midnight, the Earth is oriented such that the Sun, along with these two planets, would be on the side not visible from the night sky in any given location on Earth's surface.
  • Earth completes one rotation roughly every 24 hours.
  • The Sun and planets appear to rise in the east and set in the west.
  • At midnight, the Sun and planets close to it, like Mercury and Venus, are on the other side of Earth.

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Most popular questions from this chapter

Use the Starry Night Enthusiast \({ }^{\mathrm{TM}}\) program to examine Mercury. Select Favourites \(>\) Solar System \(>\) Mercury from the menu. Select View > Feet from the menu to remove the image of the astronaut's spacesuit from the view. Select Options \(>\) Solar System > Planets-Moons. .. from the menu to allow you to examine the complete surface of the planet. In the PlanetsMoons Options dialog box, slide the control next to the label Show dark side all the way to the right (Brighter) end of the scale. Click OK to close the dialog box. Use the Zoom controls in the toolbar to zoom in and out on the view. Rotate the image of Mercury by placing the mouse cursor over the image of the planet, holding down the mouse button, and moving the mouse. (On a two- button mouse, hold down the left mouse button.) As you explore the surface of the planet Mercury, estimate the diameter of the largest craters by measuring their size on the screen with a ruler and comparing to the diameter of Mercury (see Table 11-1). (Note that the rosette patterns surrounding both planetary poles are an artifact of the technique used to produce these images).

What kind of surface features are found on Mercury? How do they compare to surface features on the Moon? Why are they probably much older than most surface features on the Earth?

Use the Stamy Night Enthusiast \({ }^{\text {M }}\) program to observe solar transits of Venus (see Question 83). Display the entire celestial sphere (select Guides \(>\) Atlas in the Favourites menu). Open the Find pane and click the menu button for Venus (the downwardpointing blue arrow to the left of Venus) in the list. Select Centre from the menu. Use the zoom controls in the toolbar to adjust the field of view to about \(1^{\circ} \times 1^{\circ}\). (a) In the toolbar, Stop time flow and then set the Time and Date to June 8, 2004, at 12:00:00 A.M. Set the Time Flow Rate to 1 hour. Step backward or forward through time using the single-step buttons (the leftmost and the rightmost buttons) and record the times at which the solar transit begins and ends, changing the Time Flow Rate to 1 minute and the field of view to increase the accuracy of your measurement, as necessary. What is the total duration of the solar transit? (b) The ecliptic appears in Starry Night Enthusiast \({ }^{\top M}\) as a green line. During the transit, is Venus precisely on the ecliptic? If not, about how far off is it? (Hint: The Sun has an angular diameter of about 30 arcmin.) (c) Repeat parts (a) and (b) for the solar transit of Venus on June 6,2012 .

Describe the apparent motion of the Sun during a "day" on Venus relative to (a) the horizon and (b) the background stars. (Assume that you can see through the cloud cover.)

The classic 1950 science-fiction movie Rocketship X-M shows astronauts on the Martian surface with oxygen masks for breathing but wearing ordinary clothing. Would this be a sensible choice of apparel for a walk on Mars? Why or why not?

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