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Noble Gases02:54

Noble Gases

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The elements in group 18 are noble gases (helium, neon, argon, krypton, xenon, and radon). They earned the name “noble” because they were assumed to be nonreactive since they have filled valence shells. In 1962, Dr. Neil Bartlett at the University of British Columbia proved this assumption to be false.
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Schwarzschild Radius and Event Horizon01:21

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No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape...
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Oxygenic Photosynthesis01:26

Oxygenic Photosynthesis

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Oxygenic photosynthesis is a fundamental process in which light energy is harnessed to drive the oxidation of water, leading to the production of molecular oxygen (O₂), adenosine triphosphate (ATP), and nicotinamide adenine dinucleotide phosphate (NADPH). This process is essential for sustaining aerobic life on Earth and is primarily carried out by cyanobacteria, algae, and plants. The core of oxygenic photosynthesis lies in the thylakoid membranes, where chlorophyll pigments facilitate...
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Reduced Mass Coordinates: Isolated Two-body Problem01:12

Reduced Mass Coordinates: Isolated Two-body Problem

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In classical mechanics, the two-body problem is one of the fundamental problems describing the motion of two interacting bodies under gravity or any other central force. When considering the motion of two bodies, one of the most important concepts is the reduced mass coordinates, a quantity that allows the two-body problem to be solved like a single-body problem. In these circumstances, it is assumed that a single body with reduced mass revolves around another body fixed in a position with an...
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Anoxygenic Photosynthesis01:30

Anoxygenic Photosynthesis

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Anoxygenic photosynthesis is a phototrophic process that captures light energy to drive carbon fixation without producing molecular oxygen. Unlike oxygenic photosynthesis, which utilizes water as an electron donor and releases oxygen, anoxygenic phototrophs use alternative electron donors such as hydrogen sulfide (H₂S), elemental sulfur (S⁰), or thiosulfate (S₂O₃²⁻). This process is carried out by diverse groups of bacteria, including purple bacteria, green...
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Emission Spectra02:39

Emission Spectra

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When solids, liquids, or condensed gases are heated sufficiently, they radiate some of the excess energy as light. Photons produced in this manner have a range of energies, and thereby produce a continuous spectrum in which an unbroken series of wavelengths is present.
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Related Experiment Video

Updated: Mar 23, 2026

An Atmospheric Pressure Plasma Setup to Investigate the Reactive Species Formation
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An Atmospheric Pressure Plasma Setup to Investigate the Reactive Species Formation

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A white dwarf with an oxygen atmosphere.

S O Kepler1, Detlev Koester2, Gustavo Ourique3

  • 1Instituto de Física, Universidade Federal do Rio Grande do Sul, 91501-900 Porto Alegre, RS, Brazil. kepler@if.ufrgs.br.

Science (New York, N.Y.)
|April 2, 2016
PubMed
Summary

Astronomers discovered a unique white dwarf star with an atmosphere almost entirely made of oxygen. This finding challenges typical white dwarf atmospheric models and offers insights into stellar evolution.

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Area of Science:

  • Astronomy and Astrophysics
  • Stellar Evolution
  • White Dwarf Stars

Background:

  • White dwarf stars typically have atmospheres dominated by light elements like hydrogen and helium due to gravitational diffusion.
  • Stars with initial masses below approximately 10 solar masses are expected to evolve into white dwarfs.

Purpose of the Study:

  • To report the discovery of an unusual white dwarf, SDSS J124043.01+671034.68.
  • To characterize the atmospheric composition of this unique white dwarf and investigate its implications for stellar evolution.

Main Methods:

  • Spectroscopic analysis of the white dwarf SDSS J124043.01+671034.68.
  • Compositional analysis of the star's atmosphere to determine elemental abundances.

Main Results:

  • The white dwarf SDSS J124043.01+671034.68 exhibits an atmosphere almost entirely composed of oxygen.
  • Neon and magnesium are present but at abundances at least 25 times lower than oxygen.
  • No hydrogen or helium were detected in the star's atmosphere.

Conclusions:

  • The observed atmospheric composition suggests this white dwarf may be an oxygen-neon type.
  • This discovery provides a rare observational test for models of stellar evolution, particularly for stars at the higher-mass end of pre-white dwarf formation.