The position of the Sun refers to its location in the sky at any given time, which can vary based on several factors, including geographical location (latitude and longitude), the time of day, and the time of year (season). 1. **Time of Day:** The Sun appears to move across the sky from east to west due to the Earth's rotation. It rises in the east, reaches its highest point around noon (solar noon), and sets in the west.
A permanently shadowed crater refers to a lunar or planetary crater where sunlight never reaches the floor due to the angle of the solar rays and the geometry of the crater's walls. On bodies like the Moon, there are regions near the poles where the Sun never rises high enough in the sky to illuminate certain areas of the surface.
The Peak of Eternal Light is a location on the Moon in the game "Destiny." Specifically, it is a point of interest in the game's expansive open-world setting, known for its unique and haunting beauty. The area is characterized by its perpetual sunlight, which gives it a distinctive appearance compared to other regions that are more shadowy or desolate.
The orbit of Venus refers to the path that the planet Venus takes around the Sun. Here are some key details about Venus's orbit: 1. **Orbital Period**: Venus takes approximately 225 Earth days to complete one orbit around the Sun. This is known as its orbital period. 2. **Orbital Distance**: Venus is the second planet from the Sun, and it orbits at an average distance of about 108 million kilometers (about 67 million miles).
The orbit of Mars refers to the path that the planet Mars takes around the Sun. Mars has an elliptical orbit, meaning it is not a perfect circle, but rather an elongated shape. Here are some key characteristics of Mars' orbit: 1. **Average Distance from the Sun**: Mars is, on average, about 227.9 million kilometers (141.6 million miles) from the Sun. This distance is referred to as its semi-major axis.
The March equinox, also known as the vernal equinox, occurs around March 20th or 21st in the Northern Hemisphere. During this time, day and night are approximately equal in length as the sun crosses the celestial equator moving northward. This event marks the beginning of spring in the Northern Hemisphere and autumn in the Southern Hemisphere. The March equinox is significant for various cultural and agricultural reasons.
Libration is a phenomenon observed in celestial mechanics, particularly in the context of the Moon's orbit around the Earth. It refers to the oscillating motion that allows us to see slightly more than half of the Moon's surface from Earth over time. This effect occurs due to the Moon's elliptical orbit and its axial tilt. There are two primary types of libration: 1. **Libration in Longitude**: This occurs because the Moon's orbital speed varies as it travels along its elliptical path.
The "Jupiter Barrier" is a term that may refer to the gravitational influence of Jupiter in the solar system, particularly its role in shaping the dynamics of the asteroid belt and other celestial bodies. Jupiter is the largest planet in our solar system and has a strong gravitational field that can affect the orbits of nearby objects. One specific context where the term may be used is in discussions about the stability of the asteroid belt.
The term "invariable plane" is commonly used in celestial mechanics and can refer to the concept of a plane that remains fixed in space during the orbital motion of a celestial body, such as a satellite or a planet. Specifically, in the context of celestial mechanics, the invariable plane is defined as the plane that contains the total angular momentum vector of a system of bodies. For a system of celestial bodies, the invariable plane is often considered with respect to the center of mass of the system.
The First Point of Aries, also known as the Aries Point, is an important astronomical marker in the celestial coordinate system. It is defined as the point in the sky where the ecliptic (the path that the Sun appears to take through the stars) intersects the celestial equator. This intersection occurs at the vernal equinox, which is the point in spring when day and night are approximately equal in length.
"Equinox" can refer to a few different concepts depending on the context: 1. **Astronomy**: An equinox is an astronomical event that occurs twice a year when the sun is directly above the equator, resulting in nearly equal lengths of day and night across the globe. The two equinoxes are the vernal (spring) equinox, occurring around March 20 or 21, and the autumnal equinox, occurring around September 22 or 23.
The ecliptic is the apparent path that the Sun takes across the sky over the course of a year, as observed from Earth. It represents the plane of Earth's orbit around the Sun and is an essential concept in astronomy and celestial navigation. Here are a few key points about the ecliptic: 1. **Zodiac**: The ecliptic is divided into twelve sections known as the zodiac signs, which correspond to different constellations.
Earth's rotation refers to the spinning of the planet around its axis, which is an imaginary line that runs from the North Pole to the South Pole. This rotation is responsible for the cycle of day and night. Earth completes one full rotation approximately every 24 hours, which results in the diurnal cycle that we experience as daylight when the side of the Earth facing the Sun is illuminated, and nighttime when that side rotates away from the Sun.
The celestial equator is an imaginary great circle on the celestial sphere that lies directly above the Earth's equator. It divides the celestial sphere into the northern and southern celestial hemispheres. In more detail: 1. **Celestial Sphere**: The celestial sphere is an abstract representation where all celestial objects (like stars, planets, and galaxies) are projected onto an imaginary sphere surrounding the Earth.
The Spring Equinox, also known as the Vernal Equinox, occurs around March 20 or 21 each year in the Northern Hemisphere. It marks the moment when the sun crosses the celestial equator, moving northward. On this day, day and night are approximately equal in length, which is why it's called an equinox (from Latin, meaning "equal night").
Solstices are astronomical events that occur twice a year when the Sun reaches its highest or lowest point in the sky at noon, resulting in the longest and shortest days of the year. There are two solstices: 1. **Summer Solstice**: In the Northern Hemisphere, this occurs around June 21, when the Sun is directly overhead at the Tropic of Cancer. This day has the longest period of daylight and marks the beginning of summer.
Solar System dynamic theories refer to the mathematical and physical frameworks that explain the motions and gravitational interactions of celestial bodies within the Solar System. These theories encompass a wide range of topics, including the movements of planets, moons, asteroids, comets, and the Sun itself. Here are some key aspects: 1. **Newtonian Mechanics**: Sir Isaac Newton's laws of motion and the law of universal gravitation laid the groundwork for understanding the dynamics of celestial bodies.
Equinoxes are astronomical events that occur twice a year when the Sun reaches its highest or lowest point in the sky at noon, resulting in nearly equal amounts of daylight and darkness. The two equinoxes are known as the vernal equinox and the autumnal equinox. 1. **Vernal Equinox**: This occurs around March 20 or 21 in the Northern Hemisphere, marking the beginning of spring.
The Autumn Equinox, also known as the Fall Equinox or September Equinox, is an astronomical event that occurs when the Sun crosses the celestial equator, making day and night approximately equal in length. This event typically takes place around September 22 or 23 in the Northern Hemisphere and is one of two equinoxes that occur each year; the other being the Spring Equinox, which happens around March 20 or 21.
Sylvie Roke is a fictional character from the animated series "Carmen Sandiego." She is depicted as a young, intelligent, and resourceful woman who is often seen working alongside the series' main character, Carmen. The show revolves around Carmen's adventures as a master thief who steals from thieves to right wrongs and expose the corruption of organizations like V.I.L.E.

Pinned article: Introduction to the OurBigBook Project

Welcome to the OurBigBook Project! Our goal is to create the perfect publishing platform for STEM subjects, and get university-level students to write the best free STEM tutorials ever.
Everyone is welcome to create an account and play with the site: ourbigbook.com/go/register. We belive that students themselves can write amazing tutorials, but teachers are welcome too. You can write about anything you want, it doesn't have to be STEM or even educational. Silly test content is very welcome and you won't be penalized in any way. Just keep it legal!
We have two killer features:
  1. topics: topics group articles by different users with the same title, e.g. here is the topic for the "Fundamental Theorem of Calculus" ourbigbook.com/go/topic/fundamental-theorem-of-calculus
    Articles of different users are sorted by upvote within each article page. This feature is a bit like:
    • a Wikipedia where each user can have their own version of each article
    • a Q&A website like Stack Overflow, where multiple people can give their views on a given topic, and the best ones are sorted by upvote. Except you don't need to wait for someone to ask first, and any topic goes, no matter how narrow or broad
    This feature makes it possible for readers to find better explanations of any topic created by other writers. And it allows writers to create an explanation in a place that readers might actually find it.
    Figure 1.
    Screenshot of the "Derivative" topic page
    . View it live at: ourbigbook.com/go/topic/derivative
  2. local editing: you can store all your personal knowledge base content locally in a plaintext markup format that can be edited locally and published either:
    This way you can be sure that even if OurBigBook.com were to go down one day (which we have no plans to do as it is quite cheap to host!), your content will still be perfectly readable as a static site.
    Figure 5. . You can also edit articles on the Web editor without installing anything locally.
    Video 3.
    Edit locally and publish demo
    . Source. This shows editing OurBigBook Markup and publishing it using the Visual Studio Code extension.
  3. https://raw.githubusercontent.com/ourbigbook/ourbigbook-media/master/feature/x/hilbert-space-arrow.png
  4. Infinitely deep tables of contents:
    Figure 6.
    Dynamic article tree with infinitely deep table of contents
    .
    Descendant pages can also show up as toplevel e.g.: ourbigbook.com/cirosantilli/chordate-subclade
All our software is open source and hosted at: github.com/ourbigbook/ourbigbook
Further documentation can be found at: docs.ourbigbook.com
Feel free to reach our to us for any help or suggestions: docs.ourbigbook.com/#contact