Determining the Beginning of Space
Author: SpacePedia
Theme: General Space
Subject: Kármán Line - The Beginning of Space
Article Summary: The Kármán line is an imaginary boundary accepted at approximately 100 kilometers above Earth's surface and used to define the transition between atmospheric flight and movement in space. The atmosphere does not suddenly end at this altitude; its density gradually decreases as altitude increases. The altitude of approximately 100 kilometers is used to define the region where the atmosphere becomes extremely sparse and the characteristics of aerodynamic flight change significantly.
Date: 14-08-2026
The Mysterious World of the Red Planet
Author: SpacePedia
Theme: Planets
Subject: Mars Planet - Our Red Neighbor
Article Summary: Mars is one of the planets in the Solar System that most closely resembles Earth and is known as the "Red Planet." It gets this color from iron oxide (rust) on its surface. With its thin atmosphere, massive volcanoes, and deep canyons, Mars is one of the most studied planets by scientists because it may have once contained water. Today, Mars is considered a potential candidate for future human life.
Date: 18-03-2026
The Critical Mass Limit Determining the Collapse of Neutron Stars into Black Holes
Author: SpacePedia
Theme: Neutron Stars
Subject: Stability limit of neutron stars and collapse into black holes
Article Summary: Neutron stars are extremely dense celestial objects left behind after the supernova explosions of massive stars. While their masses can be similar to or several times that of the Sun, their diameters are only about 20–25 kilometers. The main factor supporting matter at this extraordinary density is the quantum mechanical pressure and the strong forces generated by the dense nuclear matter inside the neutron star. However, there is an upper limit to the mass a neutron star can sustain. This limit is known as the Tolman–Oppenheimer–Volkoff (TOV) limit. Its exact value is still being researched today, as it depends on the equation of state of neutron star matter at extremely high densities; observations show that neutron stars with several solar masses can exist. If a neutron star exceeds the maximum mass it can support, it cannot withstand its own gravity and, according to general relativity, will begin to collapse, forming a black hole. Therefore, the critical mass is of great importance for understanding the physical boundary between a neutron star and a black hole.
Date: 19-09-2026
The Late Heavy Bombardment Period in the Early Solar System
Author: SpacePedia
Theme: General Space
Subject: Late Heavy Bombardment
Article Summary: The early periods of the Solar System were much more dynamic and filled with collisions than today. Asteroids and comets left over from the formation of planets and small celestial bodies struck the surfaces of young planets much more frequently. The most significant traces of this intense bombardment period are the numerous craters found on the surfaces of the Moon, Mercury, and other rocky bodies.
Date: 20-09-2026
The Sizes Reached by the Largest Stars Compared to the Sun
Author: SpacePedia
Theme: Stars
Subject: Sizes of stars
Article Summary: The sizes of stars can differ greatly from one another. While the Sun is considered a medium-sized star, some giant and especially red supergiant stars can reach hundreds of times, or in some cases much more, the Sun's diameter. This comparison is one of the easiest ways to understand how large stars can be. However, a star's size is not the same as its mass. A star can have a very large volume while its density may be extremely low. This situation becomes especially apparent in giant stars in the later stages of their lives.
Date: 19-09-2026
The Effect of Tidal Locking on the Moon's Rotation
Author: SpacePedia
Theme: General Space
Subject: Tidal locking
Article Summary: The Moon's rotation period on its own axis is equal to its orbital period around the Earth. Therefore, the same side of the Moon is always visible from Earth. This has not always been the case; gravitational interaction between the Earth and the Moon has gradually slowed the Moon's rotation over billions of years, leading it to become tidally locked.
Date: 20-09-2026
Estimating the Ages of Stars from Their Rotation Speeds
Author: SpacePedia
Theme: Different Methods
Subject: Stellar age
Article Summary: It is not possible to directly measure the age of stars. Instead, strong estimates about their age are made using the star's physical properties. Rotation speed is one of these methods. Especially in Sun-like stars, the rotation speed decreases as they age. Therefore, measuring how fast a star rotates provides an important indicator that can be used to determine its age.
Date: 20-09-2026
The Effects of Microgravity on Astronauts' Human Bodies
Author: SpacePedia
Theme: General Space
Subject: Microgravity
Article Summary: Microgravity causes the human body to adapt to a physical environment different from conditions on Earth. With the significant reduction in gravity, muscles and bones bear less load, the distribution of body fluids changes, and the balance system begins to receive different signals. As the duration of stay in space increases, these changes become more pronounced.
Date: 20-09-2026
New Lunar Missions for Humanity within the Artemis Program
Author: SpacePedia
Theme: New Developments
Subject: Artemis Program
Article Summary: The Artemis Program is advancing to restart human lunar exploration and lay the foundation for long-term exploration activities around the Moon. Artemis II paved the way for crewed Artemis missions by passing around the Moon with four astronauts in April 2026. According to the current plan, Artemis III is set to conduct critical docking and landing system tests in Earth orbit in 2027, while Artemis IV aims to land humans on the lunar surface in 2028.
Date: 11-09-2026
The Interstellar Long Journey of the Voyager Spacecraft
Author: SpacePedia
Theme: Spacecraft
Subject: Voyager's Interstellar Journey
Article Summary: The Voyager spacecraft were launched in 1977 to explore the outer regions of the Solar System. After passing by Jupiter and Saturn, Voyager 2 also flew close to Uranus and Neptune, making important observations about these distant worlds. Their journey was not limited to the planets; the spacecraft became human-made exploration vehicles advancing toward the outer boundaries of the Solar System and into interstellar space. The source notes that even at Voyager 2's speed of over 55,000 kilometers per hour, it would still take tens of thousands of years to approach another star.
Date: 11-09-2026
The Icy Reservoir at the Outer Edge of the Solar System: The Oort Cloud
Author: SpacePedia
Theme: Comets
Subject: Oort Cloud
Article Summary: The Oort Cloud is a hypothetical spherical region thought to surround the very distant outer regions of the Solar System, containing billions of icy small bodies. This structure, believed to lie far beyond Neptune's orbit, has not been directly observed. The existence of the Oort Cloud is inferred from the orbits of very long-period comets and orbital calculations suggesting that these objects may originate from the farthest regions of the Solar System. It is thought that some of the icy bodies ejected from the regions where planets formed during the Sun's formation were captured by the Sun's gravity in very distant orbits. Passing stars and the gravitational effects of the Milky Way can alter the orbits of these objects and send some of them toward the Sun. Thus, the Oort Cloud represents a reservoir of icy bodies in the most distant regions of the Solar System, serving as a possible source of long-period comets.
Date: 18-09-2026
What Happened in the First Minutes of the Universe After the Big Bang
Author: SpacePedia
Theme: General Space
Subject: Early Universe
Article Summary: Immediately after the Big Bang, the universe was much hotter, denser, and smaller than it is today. As expansion continued, temperature and density rapidly decreased. While interactions between fundamental particles took place in the first seconds, by the first minutes, protons and neutrons began to come together to form light atomic nuclei. This process is called Big Bang nucleosynthesis. By the end of the first minutes, the universe mostly contained hydrogen nuclei and helium nuclei, with smaller amounts of light nuclei such as deuterium and helium-3 also forming. However, the universe did not yet have the structures we see today, such as stars, galaxies, or neutral atoms.
Date: 18-09-2026