Visibility of Venus during the march equinox

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Discussion Overview

The discussion revolves around the visibility of Venus during the March equinox, particularly in relation to its conjunctions with the Sun and how these affect its appearance in the sky from Mesoamerica. Participants explore the astronomical mechanics behind Venus's orbit and its visibility patterns over time.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant notes that Venus may not be very visible during the equinox every four years due to sunlight obscuring it, referencing tables of Venus-Sun conjunctions.
  • Another participant explains the orbital mechanics, stating that Venus completes approximately 1.625 times an orbit around the Sun each year, leading to a near alignment with the Sun every four years.
  • A similar calculation is repeated by another participant, emphasizing the 0.75 degrees shift of Venus's position relative to the Sun over four years.
  • Questions arise regarding the calculation of the 0.75 degrees shift and the assertion of an 80-year interval where Venus is difficult to see.
  • Clarifications are provided about the angle relationships between Venus, the Sun, and Earth, indicating that visibility can vary based on these angles and the relative positions of the planets.
  • Observations from Stellarium suggest that Venus is closer to the Sun in specific years, with predictions about its visibility in years like 2037 and 2017, noting that it may be invisible to the naked eye during certain conjunctions.

Areas of Agreement / Disagreement

Participants express differing views on the visibility of Venus during the March equinox, with some proposing specific years when it may be invisible while others challenge the assumptions behind those predictions. The discussion remains unresolved regarding the exact conditions under which Venus may be seen or obscured.

Contextual Notes

Participants acknowledge the complexity of Venus's visibility due to its orbital mechanics and the angles involved, but there are unresolved aspects regarding the calculations and assumptions made about visibility intervals.

kaleidoscope
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So this weekend I read a little about the Dresden Codex of the Maya (their astronomical log) and played a little bit with Stellarium trying to imagine the sky they saw. I noticed something that I think is interesting, Venus wasn't very visible during the equinox every four years because the sunlight would cover it (from Mesoamerica). I looked for some information about it and found some tables of the Venus-Sun Conjunctions for several centuries, and conjunctions appear to take place around march an repeat about the same date every 4 years. http://www.astropro.com/features/tables/geo/ve-su/ve000su/vesu27.html For instance, Stellarium predict it won't be visible in 2013, 2017, 2021, etc.

So, does Venus really "disappear" in the sky every 4 years during the march equinox?
 
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Venus goes round the sun in 224.701 days and the Earth in 365.256 days, so in one earthyear venus, goes 356.256/224.701 = 1.62550 times round the sun.

In 4 years, venus will go 6.50208 times round the sun, so if venus is exactly in front of the sun at the start of the 4 years, it will be nearly exactly behind the sun at the end of four years (it will shift 0.75 degrees).
There will be a period of 80 years intervals, where venus is within 7.5 degrees of the sun, and very hard to see.
 
willem2 said:
Venus goes round the sun in 224.701 days and the Earth in 365.256 days, so in one earthyear venus, goes 356.256/224.701 = 1.62550 times round the sun.

In 4 years, venus will go 6.50208 times round the sun, so if venus is exactly in front of the sun at the start of the 4 years, it will be nearly exactly behind the sun at the end of four years (it will shift 0.75 degrees).
There will be a period of 80 years intervals, where venus is within 7.5 degrees of the sun, and very hard to see.

Nice. How did you calculte the 0.75 degrees shift and the 80 year interval?
 
kaleidoscope said:
Nice. How did you calculte the 0.75 degrees shift and the 80 year interval?

The 0.75 degrees is from the 0.00208 extra rotations that venus makes in 4 years. This is however not the angle that venus moves as seen from the earth, and therefore the 80 years that I tought venus would remain too close to the sun to see isn't correct.

When the angle venus/sun/earth is 7.5 degrees and venus is close to its inferior conjunction, the angle venus/earth/sun is much larger than 7.5 degrees, so venus will be further away from the sun as seen from the earth.

When Venus is close to its superior conjunction, and the angle venus/earth/sun = 180-7.5 degrees, the angle venus/earth/sun will be smaller than 7.5 degrees.

If venus is above or below the ecliptic, because both orbits aren't exactly in the same plane, the angle between venus and the sun will look much larger when venus is closer to the Earth also.

Looking in stellarium, you can see that venus is much closer to the sun in the years 2013 +- 8n. Venus is almost exactly behind the sun in 2037, but is probably still invisible with the naked eye in in 1941 or 2133, while in 2017+- 8n years, venus never gets closer than about 5 degrees to the sun, and is probably only invisible 5 or 6 times.
 

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