Jove
Visualize
お問い合わせ

関連する概念動画

Noble Gases02:54

Noble Gases

23.3K

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.
23.3K
Schwarzschild Radius and Event Horizon01:21

Schwarzschild Radius and Event Horizon

2.9K
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...
2.9K
Oxygenic Photosynthesis01:26

Oxygenic Photosynthesis

950
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...
950
Reduced Mass Coordinates: Isolated Two-body Problem01:12

Reduced Mass Coordinates: Isolated Two-body Problem

2.5K
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...
2.5K
Anoxygenic Photosynthesis01:30

Anoxygenic Photosynthesis

1.6K
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...
1.6K
Emission Spectra02:39

Emission Spectra

78.1K
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.
78.1K

こちらも読む

関連記事

共著者、ジャーナル、引用グラフによってこの研究に関連する記事。

並び替え
Same author

A hot white dwarf merger remnant revealed by an ultraviolet detection of carbon.

Nature astronomy·2025
Same author

Accretion of a giant planet onto a white dwarf star.

Nature·2019
Same author

A planetesimal orbiting within the debris disc around a white dwarf star.

Science (New York, N.Y.)·2019
関連記事をすべて見る
JoVE
x logofacebook logolinkedin logoyoutube logo
JoVEについて
概要リーダーシップブログJoVEヘルプセンター
著者向け
出版プロセス編集委員会範囲と方針査読よくある質問投稿
図書館員向け
推薦の声購読アクセスリソース図書館諮問委員会よくある質問
研究
JoVE JournalMethods CollectionsJoVE Encyclopedia of Experimentsアーカイブ
教育
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab Manual教員リソースセンター教員サイト
利用規約
プライバシーポリシー
ポリシー

関連する実験動画

Updated: Mar 23, 2026

An Atmospheric Pressure Plasma Setup to Investigate the Reactive Species Formation
08:36

An Atmospheric Pressure Plasma Setup to Investigate the Reactive Species Formation

Published on: November 3, 2016

10.6K

酸素 の 大気 を 持つ 白い 矮星

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
まとめ

天文学者は,大気はほぼ完全に酸素で出来ているユニークな白矮星を発見しました. この発見は典型的な白矮星の大気モデルに 異議を唱え 恒星の進化の洞察を与えてくれます

科学分野:

  • 天文学と天体物理学
  • 星の進化について
  • 白い矮星

背景:

  • 白い矮星は通常,重力拡散により,水素やヘリウムのような軽い元素が支配する大気を有します.
  • 初期質量が約10太陽質量未満の星は白矮星に進化すると予想されます.

研究 の 目的:

  • SDSS J124043.01+671034.68という 珍しい白矮星を発見しました
  • このユニークな白矮星の大気組成を特徴付け 恒星の進化への影響を調査する

主な方法:

  • 白い矮星SDSS J124043.01+671034.68のスペクトル解析について
  • 星の大気の組成分析 元素の豊富さを決定する

主要な成果:

  • 白い矮星SDSS J124043.01+671034.68は,ほぼ完全に酸素で構成された大気を表しています.
  • ネオンとマグネシウムは存在するが,酸素よりも少なくとも25倍少ない.
  • 星の大気には水素やヘリウムが検出されませんでした

結論:

  • 観測された大気組成は この白矮星が酸素ネオン型である可能性を示唆しています

さらに関連する動画

Creating Defined Gaseous Environments to Study the Effects of Hypoxia on C. elegans
11:07

Creating Defined Gaseous Environments to Study the Effects of Hypoxia on C. elegans

Published on: July 20, 2012

12.6K
Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

11.1K

関連する実験動画

Last Updated: Mar 23, 2026

An Atmospheric Pressure Plasma Setup to Investigate the Reactive Species Formation
08:36

An Atmospheric Pressure Plasma Setup to Investigate the Reactive Species Formation

Published on: November 3, 2016

10.6K
Creating Defined Gaseous Environments to Study the Effects of Hypoxia on C. elegans
11:07

Creating Defined Gaseous Environments to Study the Effects of Hypoxia on C. elegans

Published on: July 20, 2012

12.6K
Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

11.1K
  • この発見は,恒星の進化のモデル,特に白矮星形成前の高質量終端の恒星のための珍しい観測テストを提供します.