How much is a trillion dollars? | IHTD

How Long Ago Is a Trillion Seconds? If you count backward, then:
1 million seconds = 12 days ago
1 billion seconds = 31 years ago
1 trillion seconds = 30,000 B.C.
(give or take a decade or two)

How high is a trillion in $1000 bills?

If you stack a trillion-worth of $1000 bills together, then: 1 million dollars = 4 inches high 1 billion dollars = 364 feet high 1 trillion dollars = 63 miles high (give or take a foot or two) Note that this is a STACK, not laid end-to-end.
Source: How much is a trillion dollars? | IHTD

The Evening and Morning Star

Evening and Morning Star. The earth is shown at the bottom of the illustration, and for our purposes, consider it to be at rest. So let's look at Venus at different places in the orbit. It is orbiting around the sun counterclockwise in this illustration, and the earth is rotating on its axis in that same direction, causing night and day. When Venus is on the left side of the illustration between positions 3 and 5, it appears as an evening star, when it is on the right side between positions 6 and 2, it is a morning star. In the other positions on the near and far side of the orbits, it is too near the sun to be seen. The periods as evening and morning star each average about 263 days, the disappearance on the near side of the sun is about 8 days, and on the far side is about 50 days, for a total of 584 days for the entire cycle.
The Feathered Serpent. Native Americans of Central America had a legend about Venus which is still useful to help remember where Venus is in its orbit. The equated Venus, which they called the Dawn Star, with their god Quetzalcoatl, the "Feathered Serpent." They believe he came to earth and lived as a man and that the evening star represented his life. Thus, point 3 in the orbit when Venus first rises in the west as an evening star would represent the "birth" of Venus. It is then on the far side of its orbit, and so it is at about its faintest at birth. It then grows a little brighter every day as an evening star in the west, like a child growing up, until it gets to point 4 in the orbit. That point is called the greatest eastern elongation because it is as far east of the sun as it can get. By this time, Venus is in its "prime" of life, and is very bright. It then continues to get even brighter for about another month until it is so bright it can cast a shadow on a moonless night and is often the cause of flying saucer reports from someone who looked at the sky for the first time. Because it is at this time so near the earth, it seems to plunge surprisingly quickly into the earth and "die" at point 5 in the illustration.
Source: The Evening and Morning Star