(42301) 2001 UR163 is a small celestial body classified as a centaur, which is a type of object located between the orbits of Jupiter and Neptune. Centaurs are considered transitional objects because they share characteristics of both asteroids and comets. Discovered in 2001, (42301) 2001 UR163 has an irregular orbit and is believed to be composed of ice and rock.
(523639) 2010 RE64 is a trans-Neptunian object (TNO) that is part of the Kuiper Belt, a region of the solar system beyond the orbit of Neptune filled with many small and icy bodies. This particular object was discovered in 2010 and has characteristics typical of other Kuiper Belt objects, such as being relatively small and composed mainly of frozen materials.
(523645) 2010 VK201 is the designation of a significant asteroid that is part of the asteroid belt. It was discovered in November 2010. It's categorized as a near-Earth object (NEO), specifically an Atira asteroid, meaning its orbit lies entirely within that of Earth's orbit.
(612533) 2002 XV93 is a designation for a trans-Neptunian object (TNO) located in the outer solar system, specifically in the Kuiper Belt. TNOs are celestial bodies that orbit the Sun beyond Neptune.
(84522) 2002 TC302 is a near-Earth asteroid discovered on October 1, 2002. It is classified as an Apollo-type asteroid, which means it has an orbit that crosses Earth's orbit. These types of asteroids can come quite close to Earth but are not necessarily on a collision course with our planet.
19521 Chaos refers to a specific numerical value associated with a particular chaotic dynamical system or a mathematical phenomenon known as "chaos theory." However, without more context, it’s difficult to determine the precise significance of "19521 Chaos." In mathematics and physics, chaos theory studies systems that appear to be disordered or random, but are actually governed by underlying patterns and deterministic laws. These systems are sensitive to initial conditions, which is often illustrated with examples like the butterfly effect.
2014 FC72 is a specific fluid used in various applications, primarily known for its properties as a coolant and dielectric fluid. It is a perfluorinated compound, which means it consists of carbon and fluorine atoms. FC72 is often utilized in electronics cooling, particularly in applications where traditional cooling methods (like water cooling) may not be suitable. FC72 offers several advantages, such as excellent thermal conductivity, high chemical stability, and low toxicity.
2014 UZ224 is a trans-Neptunian object (TNO) that was discovered in 2014. It is part of the Kuiper Belt, a region of the solar system beyond the orbit of Neptune that contains many small icy bodies. 2014 UZ224 is classified as a scattered disk object, which means it has an elliptical and tilted orbit that can be influenced by the gravitational pull of the giant planets, particularly Neptune.
U is a designation for a specific trans-Neptunian object (TNO) that was discovered in the outer solar system. TNOs are icy bodies that orbit the Sun at a greater distance than Neptune. They are part of a larger group of objects known as the Kuiper Belt, which contains many similar bodies. The designation "U" is used here for clarity, as there can be multiple objects with similar naming conventions.
90377 Sedna is a distinct and distant object in the solar system, classified as a trans-Neptunian object (TNO). It was discovered in 2003 and is notable for its unusually large size and highly eccentric orbit, which takes it far beyond the orbit of Neptune. Sedna is believed to be one of the largest known TNOs, with an estimated diameter of about 1,000 kilometers (620 miles).
ESPRESSO can refer to different concepts depending on the context. Here are a few possibilities: 1. **Coffee**: Espresso is a concentrated coffee beverage brewed by forcing a small amount of nearly boiling water through finely-ground coffee beans. It is characterized by its rich flavor and thick crema (the golden layer that forms on top of a well-prepared espresso).
SCIAMACHY, which stands for SCanning Imaging Absorption spectroMeter for Atmospheric CHartographY, is an instrument that was launched aboard the European Space Agency's (ESA) ENVISAT satellite in March 2002. The primary purpose of SCIAMACHY is to measure the Earth's atmospheric composition and monitor various trace gases, aerosols, and other atmospheric constituents through spectral analysis.
The High Accuracy Radial velocity Planet Searcher (HARPS) is an advanced spectrograph designed for the precise measurement of the radial velocities of stars. Located at the La Silla Observatory in Chile, HARPS is particularly renowned for its capability to detect exoplanets through the radial velocity method. This technique involves observing the slight wobble of a star caused by the gravitational influence of orbiting planets, which leads to shifts in the star's spectral lines.
The Swiss 1.2-metre Leonhard Euler Telescope (SELT) is an astronomical telescope located at the La Silla Observatory in Chile, which is operated by the European Southern Observatory (ESO). It is named after the Swiss mathematician and astronomer Leonhard Euler. The telescope has a primary mirror with a diameter of 1.2 meters and is primarily used for research in astrophysics and for observations of celestial objects.
A Bonner sphere is a type of neutron detection and measurement device used in radiation physics. It consists of a sphere made of a hydrogenous material, such as polyethylene, that is surrounded by a layer of neutron moderator or shielding material, often containing boron or other neutron-absorbing substances. The primary purpose of the Bonner sphere is to measure neutron flux or dose rates in a radiation field.
A push broom scanner is a type of optical imaging system used primarily in remote sensing and aerial imaging. Unlike traditional scanners that use a moving mechanism to capture images line-by-line, a push broom scanner captures an entire line of data simultaneously. Here’s how it works: ### Key Features of Push Broom Scanners: 1. **Linear Array**: Push broom scanners use a linear array of sensors (often CCD or CMOS sensors) arranged in a line.
Gammasphere is a sophisticated gamma-ray detection system used in nuclear and particle physics research. It is primarily designed to study the structure of atomic nuclei by detecting the gamma rays emitted during nuclear reactions and decays. The system consists of an array of high-purity germanium (HPGe) detectors that are arranged in a spherical configuration, allowing for efficient detection of gamma radiation from various angles.
Global-scale Observations of the Limb and Disk (GOLD) is a NASA mission aimed at studying the Earth's upper atmosphere, particularly the region known as the ionosphere and the thermosphere. Launched on January 25, 2018, aboard an experimental satellite called the International Space Station (ISS), GOLD's primary objective is to obtain detailed observations of the Earth's limb and disk, which means the edge and the surface of the Earth as seen from space.
Pinned article: ourbigbook/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!
Intro to OurBigBook
. Source. We have two killer features:
- 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-calculusArticles 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/derivativeVideo 2. OurBigBook Web topics demo. Source. - 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.
- to OurBigBook.com to get awesome multi-user features like topics and likes
- as HTML files to a static website, which you can host yourself for free on many external providers like GitHub Pages, and remain in full control
Figure 2. You can publish local OurBigBook lightweight markup files to either OurBigBook.com or as a static website.Figure 3. Visual Studio Code extension installation.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. - Infinitely deep tables of contents:
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