Jove
Visualize
お問い合わせ
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

関連する概念動画

Collisions in Multiple Dimensions: Introduction01:05

Collisions in Multiple Dimensions: Introduction

It is far more common for collisions to occur in two dimensions; that is, the initial velocity vectors are neither parallel nor antiparallel to each other. Let's see what complications arise from this. The first idea is that momentum is a vector. Like all vectors, it can be expressed as a sum of perpendicular components (usually, though not always, an x-component and a y-component, and a z-component if necessary). Thus, when the statement of conservation of momentum is written for a problem,...
Types of Collisions - II01:19

Types of Collisions - II

When two or more objects collide with each other, they can stick together to form one single composite object (after collision). The total mass of the object after the collision is the sum of the masses of the original objects, and it moves with a velocity dictated by the conservation of momentum. Although the system's total momentum remains constant, the kinetic energy decreases, and thus such a collision is an inelastic collision. Most of the collisions between objects in daily life are...
Elastic Collisions: Introduction01:00

Elastic Collisions: Introduction

An elastic collision is one that conserves both internal kinetic energy and momentum. Internal kinetic energy is the sum of the kinetic energies of the objects in a system. Truly elastic collisions can only be achieved with subatomic particles, such as electrons striking nuclei. Macroscopic collisions can be very nearly, but not quite, elastic, as some kinetic energy is always converted into other forms of energy such as heat transfer due to friction and sound. An example of a nearly...
Elastic Collisions: Case Study01:15

Elastic Collisions: Case Study

Elastic collision of a system demands conservation of both momentum and kinetic energy. To solve problems involving one-dimensional elastic collisions between two objects, the equations for conservation of momentum and conservation of internal kinetic energy can be used. For the two objects, the sum of momentum before the collision equals the total momentum after the collision. An elastic collision conserves internal kinetic energy, and so the sum of kinetic energies before the collision equals...
Types Of Collisions - I01:04

Types Of Collisions - I

When two objects come in direct contact with each other, it is called a collision. During a collision, two or more objects exert forces on each other in a relatively short amount of time. A collision can be categorized as either an elastic or inelastic collision. If two or more objects approach each other, collide and then bounce off, moving away from each other with the same relative speed at which they approached each other, the total kinetic energy of the system is said to be conserved. This...
Collisions in Multiple Dimensions: Problem Solving01:06

Collisions in Multiple Dimensions: Problem Solving

In multiple dimensions, the conservation of momentum applies in each direction independently. Hence, to solve collisions in multiple dimensions, we should write down the momentum conservation in each direction separately. To help understand collisions in multiple dimensions, consider an example.
A small car of mass 1,200 kg traveling east at 60 km/h collides at an intersection with a truck of mass 3,000 kg traveling due north at 40 km/h. The two vehicles are locked together. What is the...

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

Compromised white matter integrity in obesity.

Obesity reviews : an official journal of the International Association for the Study of Obesity·2015
Same author

[The functional sport shoe parameter "torsion" within running shoe research--a literature review].

Sportverletzung Sportschaden : Organ der Gesellschaft fur Orthopadisch-Traumatologische Sportmedizin·2010
Same author

Chain extension of sugar delta-lactones with the enolate of tert-butyl bromoacetate and elaboration into functionalized C-ketosides, C-glycosides, and C-glucosyl glycines.

Organic letters·2001
Same author

Combinatorial synthesis of carbohydrates.

Current opinion in chemical biology·1999
Same author

Protein interactions implicated in neurotransmitter release.

Journal of physiology, Paris·1998
Same author

Interaction between the pili of Pseudomonas aeruginosa PAK and its carbohydrate receptor beta-D-GalNAc(1-->4)beta-D-Gal analogs.

Canadian journal of microbiology·1998

関連する実験動画

Updated: Jul 12, 2026

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
09:44

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System

Published on: June 5, 2014

銀河が衝突し合体する.

F Schweizer

    Science (New York, N.Y.)
    |January 17, 1986
    PubMed
    まとめ

    銀河は,宇宙との出会い中に重力によって駆動される相互作用と合併を通じて進化する. これらの出来事は,恒星形成と燃料クエーザーを誘発し,ビッグバン以来の銀河の進行中の進化を明らかにします.

    科学分野:

    • 天文学と天体物理学について
    • コスモロジー・コスモロジーとは

    背景:

    • 銀河は,環境と相互の相互作用によって進化する.
    • 重力によって誘発される銀河の出会いは,永続的な痕跡を残します.
    • これらの相互作用は,銀河の合併につながり,軌道エネルギーを消耗させます.

    研究 の 目的:

    • 銀河の形成と進化のメカニズムを探求する.
    • 宇宙の進化における銀河の相互作用と合併の役割を理解する.
    • 銀河の形成のタイミングと進行中のダイナミックな変化を調査するために.

    主な方法:

    • コンピューター技術の進歩を利用してシミュレーションを行う.
    • 宇宙望遠鏡からの観測データを活用する.
    • 銀河の出会いにおける重力と潮のサインを分析する.

    主要な成果:

    • 銀河の衝突と合併は,銀河の進化の重要な原動力である.
    • これらの出来事は,広範囲にわたる恒星形成を引き起こし,クエーザーを燃料にします.
    • 証拠によると,銀河の一部は,当初考えられていたよりも後に形成され,進化を続けています.

    さらに関連する動画

    Setting Limits on Supersymmetry Using Simplified Models
    07:46

    Setting Limits on Supersymmetry Using Simplified Models

    Published on: November 15, 2013

    Bringing the Visible Universe into Focus with Robo-AO
    10:35

    Bringing the Visible Universe into Focus with Robo-AO

    Published on: February 12, 2013

    関連する実験動画

    Last Updated: Jul 12, 2026

    Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
    09:44

    Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System

    Published on: June 5, 2014

    Setting Limits on Supersymmetry Using Simplified Models
    07:46

    Setting Limits on Supersymmetry Using Simplified Models

    Published on: November 15, 2013

    Bringing the Visible Universe into Focus with Robo-AO
    10:35

    Bringing the Visible Universe into Focus with Robo-AO

    Published on: February 12, 2013

    結論:

    • 銀河の進化は,相互作用や合併によって大きく影響されるダイナミックなプロセスです.
    • 宇宙の出会いは,銀河の性質や現象を形作る上で重要な役割を果たしています.
    • 銀河は静的な存在ではないし,宇宙の時間尺度で重要な動的進化を続けている.