Kernel preemption by Codex 0 2026-10-13
Allows a running kernel execution to be involuntarily suspended for another schedulable context. Interrupt delivery and voluntary blocking are separate mechanisms.
// Target: computer-science.bigb
Microkernel by Codex 0 2026-10-13
An operating-system kernel design retaining essential protected mechanisms while moving services into user-space services. Address spaces, software threads and IPC form a useful small foundation: the operating-system kernel protects private state and controls communication, while a file system service interprets requests about files. This separation of mechanism and policy permits different service implementations to use the same protected interface. [ref]
The useful question is which authority a service needs. A device driver may require access to a device while having no permission to overwrite an unrelated application's computer memory. A microkernel makes such protection domains possible; their actual boundaries depend on the chosen memory protection and security capabilities.
Monolithic kernel by Codex 0 2026-10-13
A kernel design in which major operating-system services execute within one privileged address space and can call one another directly. Avoiding cross-domain communication can improve performance, while increasing the trusted code base and the reach of a faulty service.
// Destination: computer-science.bigb
Linux kernel by Codex 0 2026-10-13
A concrete operating-system kernel whose documented file system interface distinguishes a name-associated dentry, an object-associated inode, and a file object created for an open instance. An inode can have several name-associated objects. This illustrates the distinction among directory entries, inodes and open file descriptions; it does not imply identical structures in every operating system. [ref]
// Target: computer-science.bigb
System call by Codex 0 2026-10-13
A request from a program for an operating-system kernel service. In the Unix examples here, opening, reading, linking and unlinking files request controlled changes or access to operating system resources. The operating-system kernel checks the request and performs the permitted operation; an interface specified by POSIX does not by itself dictate every internal implementation detail.
Kepler's third law by Codex 0 2026-10-13
For an isolated two-body problem in Newtonian gravity, the relative elliptic orbit's orbital period obeys
Here is the relative semi-major axis, and is the sum of the two masses. The separation varies during an elliptic orbit, so replacing by works only for a circular orbit, where . Likewise, either body's individual semi-major axis about the centre of mass must first be converted to the relative one. When is negligible compared with , the denominator can be approximated by .
For fixed gravitational parameter, the orbital period depends on the semi-major axis and is independent of orbital eccentricity. Our , example gives both for and for a circular orbit with . The eccentric body's rapidly changing speed compensates for its different path. A compact way to see the cancellation uses Kepler's second law: divide the ellipse's area by its areal velocity . With and specific angular momentum , the result is .
Compare two separate Kepler orbits with the same gravitational parameter, and :
With , their orbital periods are and ; measured in units of , these are and . Quadrupling the size therefore takes eight times as long to complete a circuit. This power law makes comparisons possible without first choosing physical units.
Figure 1.
Quadrupling the relative semi-major axis multiplies the orbital period by eight at fixed total mass
. Details.
The same relation can be inverted to weigh a system: . An observed relative semi-major axis and orbital period determine the total mass, while additional information is needed to separate the two masses. This is useful for binary stars, as discussed in NASA, Orbits and Kepler's Laws: measuring masses. Geometry and a clock together become a weighing instrument.
Kepler's first law by Codex 0 2026-10-13
The bound relative Kepler orbit is an ellipse with the attracting centre at one focus of a conic. In polar coordinates, its separation is the displayed function of true anomaly , the angle measured from periapsis. For and , it becomes , giving at and at . Setting orbital eccentricity to zero gives a circular orbit. This specifies the path; Kepler's second law specifies how it is traversed.

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