Transit Of Venus Research Paper

Scaled Distance Venus-Sun: 1.08 x 108 Km * (1 meter/2.87 x 108 Km) = 0.38 m

The astronomers who made the discovery said that the real-life Tatooine’s transits are only visible 9 percent of the time because the tilt of the planet’s orbit changes so quickly. They explained that they were lucky that they were able to detect the planet, because transits are usually not visible from Earth.

Like Mercury it is a rocky planet. It's even hotter than its smaller cousin Mercury, with temperatures drastically increased by an unchecked system of greenhouse gasses. The temperatures also varied wildly, from a -364 degree Fahrenheit low to a 870 degree high. Venus also hosts wild winds, blowing at extremely high speeds at the poles while the air at the equator hangs at a standstill. This air is also extremely heavy, and weighs almost 90 times heavier than that on Earth. Venus is constantly covered in thick, sulfurous clouds. These clouds reflect almost 90% of the light that hit them, making Venus the brightest object in the sky besides the sun and the moon. They also contain droplets of sulfuric acid, which occasionally rains down on the planet's surface. These storms even contain

When was it discovered/named: The Babylonians have the earliest recording of the observation of Venus, dating back to around 1581 BC.

Being Earth's sister planet, Venus can be greatly compared to it. They are similar in most aspects but Venus can be distinct from Earth by its atmosphere. Venus' atmosphere consist of carbon dioxide and a small percentage of nitrogen. Its atmospheric mass is 93 times of that of Earth and its atmospheric pressure is 92 times of that of on Earth's surface. Hence, Venus has an extremely dense atmosphere. The abundance of carbon dioxide and thick clouds of sulfur dioxide is responsible for the greatest greenhouse effect in the Solar System. It causes hot surfaces, even hotter than Mercury, and its minimum surface temperature of 735 K. This temperature does not vary or varies only little between day and night in Venus due to thermal inertia and

The book provides information about the planet Venus researched by real scientist and probes. Some of those information include

We have finally arrived at Venus! Did you know a day on Venus is the same as 116 days and 18 hours on Earth. Venus has the longest day in our solar system. Venus is thought to rotate so slowly, because of its dense atmosphere and high speed winds. Wind on Venus can go up to 450 miles per hour. My question is , “Does Venus take longer to orbit the sun because it rotates backwards?”, but scientist are also not sure why Venus rotates backwards.

I have decided since it will take me 43 day to get from Earth to Venus I will write facts about Earth on my way there. Since we are going to the solar system the basic facts about Earth are necessary. Earth is third planet from the Sun, and the fifth largest in our Solar System. 71% of Earth’s surface is covered in water, and the remaining 29% is

Before we arrive to Venus let me inform you that we aren’t actually landing on Venus or any of the planets . Venus can literally kill you in 10 seconds or less. Venus is the second closest planet to the Sun. Which makes Venus 464 oc (867 oF), and it's the hottest planet in our Solar System. The reason why Venus is the hottest planet and not Mercury is because Venus's atmosphere is mostly made up of carbon dioxide. Which is a prevalent greenhouse gas. In my next entry I will get into what a greenhouse effect is.

The Soviet Union was the only country to actually land on the surface of Venus and were the ones to closely examine the atmospheric structure and properties along with the soil components. Though there were some technological failures along the way, their ability to persist paid off in discovering new scientific information from Earth’s sister

Venus, aptly named after the Roman goddess of beauty, shines in our night sky. This is due to the interesting nature of Venus's atmosphere. Though it has some of the same elements as Earth's atmosphere, Venus's is very different. It boasts roughly 96% carbon dioxide and roughly 3% nitrogen. CO2 is very important for any organisms on planets but the CO2 on Venus reveals something very different. The greenhouse effect that muggle scientists believe is happening to Earth right now may have happened to Venus a long time ago. After all Venus and Earth are sister planets, alike in many aspects. The reason that Venus shines so brightly in the night sky is the clouds of sulfuric acid that hover over the layer of CO2 on Venus. The clouds reflect as

The photographs taken were then examined by NASA as well as the Japanese Aerospace Exploration Agency (JAXA) (http://global.jaxa.jp/). The images will give an insight into finer details of the planet which have been unknown to scientists as of yet. This information’s time to shine is now as it could be useful to any future missions to Venus as well as identifying similar planets as they cross in front of distant stars.

Before going into detail, let’s look at some basic statistics and facts of Venus. The second planet from the sun has an average distance of 0.72 AU. It has a similar size to Earth with a radius of 6051 kilometers and a mass 82% that of Earth’s. It is composed of rocks and metals and has an average density of 5.24 g/cm3. Unlike most other planets, Venus has zero moons. Mainly due to its very severe greenhouse effect, Venus has a searing average surface temperature of 740 K or 466.85 C. Venus rotates exceedingly slow,

Above the Troposshere is the Mesosphere, which is about 40 km thick. Above the Mesosphere is the Thermossohere whom I dont know how thick it is, and above that is the Exosphere which is so called because it is the most outher Atmospheric layer. The Exosphere is between an altitude from 220 km to 250 km. 90 % of the atmospheric mass of Venus is at an altitude lower then 28 km. Venus is easily visible even without using a telescope during morning and evening because there are upon the thicknlayer of Carbon dioxyde closest to the surface, layers of clouds of sulfuric acid which reflect over 90 % of the sunlight that hits Venus. Venus must appear as yellow because of the reflection of this layers of clouds. The Greek for example first thought, that Venus would be two diffrent planets/stars as it appered in the morning and evening sky. They so called it Phosphorus and

This is because for a planet to be detected it must have an orbit that transits between the observation point and the star. This means that the planet must orbit in a very specific plane and that the plane becomes smaller for planets that orbit at a greater distance from their host star. So planets that are detected using the transit method are usually planets known as “Hot Jupiters”. To break down this description it means that these planets are comparable to Jupiter because of their size and density, and are described as being hot due to their closeness to their host star (usually between 0.015 and 0.05 AU) and the high surface temperature that comes with that closeness. Also if the host star is small such as a neutron star then the size of the plane that a transit is visible in is also reduced.