Possible dwarf planets 1970-01-01
Dwarf planets are celestial bodies that orbit the Sun and are similar to planets but do not meet all the criteria to be classified as such. The International Astronomical Union (IAU) defines a dwarf planet as a body that: 1. Orbits the Sun 2. Is not a satellite (i.e., it is not a moon of another body) 3.
Sednoids 1970-01-01
Sednoids refers to a group of trans-Neptunian objects (TNOs) that have orbits significantly influenced by the gravitational pull of a distant, yet-to-be-identified planet, often referred to as "Planet Nine" or "Planet X." The name is derived from the first known member of this group, Sedna, which was discovered in 2003 and has a highly elliptical orbit that takes it far beyond the typical Kuiper Belt.
ASASSN-V J213939.3-702817.4 1970-01-01
ASASSN-V J213939.3-702817.4 is a designation given to a variable star or astronomical object observed by the All-Sky Automated Survey for SuperNovae (ASAS-SN). The ASAS-SN project is focused on detecting transients, such as supernovae and other variable stellar phenomena, across the entire sky. The designation includes the coordinates of the object in the sky, with "J213939.3-702817.
BLC1 1970-01-01
BLC1, or "Bacteria Living in the Clouds," refers to a specific type of bacteria that has been identified in the atmosphere, particularly in clouds. These microorganisms are of interest in various fields, including microbiology, environmental science, and climate studies, because they can influence cloud formation and precipitation processes. In some studies, BLC1 is specifically associated with certain strains of bacteria that are capable of ice nucleation, which means they can promote the formation of ice crystals in cloud droplets.
Baldwin effect (astronomy) 1970-01-01
In the context of astronomy, the "Baldwin effect" refers to a correlation observed in the properties of quasars, particularly the relationship between the luminosity of a quasar and the equivalent width of certain emission lines, such as the magnesium II line. This effect suggests that more luminous quasars tend to have weaker emission lines, which can be interpreted as a result of different physical processes occurring in these high-energy environments. The phenomenon is named after the astronomer James A.
Diffuse extragalactic background radiation 1970-01-01
Diffuse Extragalactic Background Radiation (DEBR) refers to the faint, overall glow of electromagnetic radiation that permeates the universe outside our galaxy. This radiation is not concentrated in individual sources like stars or galaxies but is instead the cumulative output from numerous cosmic phenomena across vast distances.
Diffuse interstellar bands 1970-01-01
Diffuse interstellar bands (DIBs) are a set of absorption lines observed in the spectra of stars that are located behind interstellar dust clouds. These absorption features are seen in the ultraviolet, visible, and near-infrared portions of the electromagnetic spectrum. They are believed to arise from the presence of large, complex molecules or species that exist in the interstellar medium, though their precise nature has not yet been conclusively identified.
Disrupted planet 1970-01-01
The term "disrupted planet" is not a widely recognized or specific scientific term in astronomy or planetary science. However, it might refer to a planet that has experienced significant alterations to its surface, atmosphere, or orbital characteristics due to various factors such as collisions, gravitational interactions, or other cosmic events.
EPIC 204376071 1970-01-01
EPIC 204376071 is a star cataloged in the Kepler Input Catalog, and is particularly notable for being the host star of an exoplanet discovered by the Kepler space telescope. This star is located in the constellation Cygnus and is part of the Kepler field of view, which was monitored for transiting exoplanets.
Extraterrestrial life 1970-01-01
Extraterrestrial life refers to any form of life that exists beyond Earth. This concept encompasses a wide range of possibilities, from simple microorganisms to advanced, intelligent civilizations. The search for extraterrestrial life is a significant area of interest in fields such as astrobiology, astronomy, and planetary science.
Faint young Sun paradox 1970-01-01
The Faint Young Sun Paradox refers to an apparent contradiction in our understanding of the early Earth's climate and the evolution of life. According to astrophysical models of the Sun's evolution, the Sun was significantly less luminous during its early years—about 30% dimmer—as it was a younger star in the process of fusing hydrogen into helium. If the Sun was indeed fainter, it raises questions about how early Earth maintained liquid water on its surface and supported life.
Fast blue optical transient 1970-01-01
Fast Blue Optical Transients (FBOTs) are a type of astronomical phenomenon characterized by a rapid rise and decline in brightness, typically occurring in the optical wavelengths. These events are often linked to cataclysmic occurrences such as supernovae, neutron star mergers, or the collapse of massive stars. FBOTs are distinguished by their exceptionally fast light curves, which reach their peak brightness within just a few days and then fade away quickly, often within weeks.
Fast radio burst 1970-01-01
Fast Radio Bursts (FRBs) are brief but intense bursts of radio waves from distant galaxies. They are characterized by their extremely high energy, typically lasting only a few milliseconds, yet they can emit as much energy in that short time as the Sun emits in an entire day. FRBs were first discovered in 2007, and their origins remain a topic of active research.
Fermi paradox 1970-01-01
The Fermi Paradox is the apparent contradiction between the high probability of extraterrestrial life in the universe and the lack of evidence or contact with such civilizations. The paradox is named after physicist Enrico Fermi, who famously asked, "Where is everybody?" during a discussion about the possibility of intelligent life beyond Earth.
G-dwarf problem 1970-01-01
The G-dwarf problem is a phenomenon in astrophysics and astronomy related to the abundance of certain types of stars, specifically G-type main-sequence stars (often referred to as "G-dwarfs"). These stars are similar to our Sun and are characterized by certain characteristics, such as their temperature and luminosity. The problem arises when astronomers try to account for the number of G-dwarf stars in the Milky Way galaxy.
Galactic Center GeV excess 1970-01-01
The Galactic Center GeV excess refers to an observed excess of gamma-ray radiation in the vicinity of the center of our galaxy, the Milky Way, particularly in the GeV (giga-electronvolt) energy range. This excess was first noted in gamma-ray data collected by the Fermi Gamma-ray Space Telescope and has become a subject of significant interest in astrophysics and particle physics.
Greisen–Zatsepin–Kuzmin limit 1970-01-01
The Greisen–Zatsepin–Kuzmin (GZK) limit refers to a fundamental limit on the energy of cosmic rays, particularly protons, due to interactions with the cosmic microwave background (CMB) radiation. This limit is named after three physicists: Kenneth Greisen, Georgiy Zatsepin, and Vitaly Kuzmin, who independently identified this phenomenon in the early 1960s.
HD 139139 1970-01-01
HD 139139 is a star located in the constellation of Centaurus, approximately 60 light-years away from Earth. It is a solar-type star, similar in characteristics to our Sun, and is often of interest for studies involving stellar properties, exoplanet research, and astrobiology. In addition to its basic stellar characteristics, HD 139139 has also gained attention due to the discovery of one or more exoplanets in its orbit.
IPTF14hls 1970-01-01
IPTF14hls is a designation for a specific astronomical object, identified as a supernova. It was discovered as part of the Intermediate Palomar Transient Factory (iPTF) survey, which focuses on transient astronomical events. The "IPTF" stands for the "Intermediate Palomar Transient Factory," while "14hls" indicates that the supernova was discovered in the year 2014.
List of fast radio bursts 1970-01-01
Fast Radio Bursts (FRBs) are brief, intense bursts of radio waves originating from outside our galaxy. They are typically only a few milliseconds long and carry massive amounts of energy. The exact sources of FRBs are still not completely understood, but they have intrigued astronomers since they were first discovered in 2007. The list of FRBs includes both repeating and non-repeating bursts.