関連する実験動画
Updated: May 7, 2026

10:35
Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
銀河NGC4258までの距離は,セフェイド変数星の観測から得られた
E Maoz1, J A Newman, L Ferrarese
1NASA Ames Research Center, MS 245-3, Moffett Field, California 94035-1000, USA. maoz@ism.arc.nasa.gov
Nature
|July 25, 2006
まとめ
セフェイド変数星は,宇宙の距離を測る上で極めて重要です. NGC4258の新しい観測は,セフェイド距離とマザーベースの測定の間の不一致を示し,ハッブル定数と宇宙に潜在的に影響を与える可能性があります.
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:
- セフェイド変数星は,銀河外距離測定のための標準的なろうそくとして使用されます.
- 正確な距離は,ハッブル定数と宇宙の年齢を決定するために不可欠です.
研究 の 目的:
- 銀河NGC4258.8までの距離測定の不一致を調査する.
- チェフェイド星変星距離計算における潜在的なシステマティックエラーの影響を評価する.
主な方法:
- NGC4258.8のセフェイド変数星の観測
- ウォーターマザー自身の運動から得られた独立した幾何学的な距離との比較.
主要な成果:
- NGC4258へのセフェイドベースの距離は8.1 ± 0.4 Mpcです.
- ウォーターマザーからの独立した幾何学的な距離は7.2 ± 0.5 Mpcです.
- 2つの測定値の差は1.3シグマである.
結論:
- 改訂されたセフェイド距離スケールは,マザーベースの距離を採用した場合,ハッブル定数を12 ± 9%増加させるでしょう.
- この修正により,計算された宇宙膨張年齢も同じ割合で減少する.
- セフェイドの距離における潜在的な体系的不確実性は,さらなる調査を正当化します.
関連する概念動画
Kepler's Third Law of Planetary Motion
In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. In 1909, he formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe. However, in 1918, he published his third law of planetary motion, which gives a precise mathematical relationship between a planet's average distance from the Sun and the amount of time it takes to revolve around the Sun. It...
Schwarzschild Radius and Event Horizon
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 velocity with the...
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 velocity with the...
Detection of Black Holes
Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Flame Photometry: Overview
Flame photometry, also known as flame emission spectrometry, is a technique used for the qualitative and quantitative analysis of elements present in a sample using a flame as the source of excitation energy. The concept of flame photometry was realized in the early 1860s by Kirchhoff and Bunsen, who discovered that specific elements emit characteristic radiation when excited in flames. The first instrument developed for this purpose was used to measure sodium (Na) in plant ash using a Bunsen...
Flame Photometry: Lab
In a flame photometer, when a solution like potassium chloride is aspirated into the flame, the solvent evaporates, leaving behind dehydrated salt. This salt dissociates into free gaseous atoms in their ground state. Some of these atoms absorb energy from the flame, leading to their excitation. The excited atoms return to the ground state, emitting photons at characteristic wavelengths. Because only electronic transitions are involved, the resulting emission lines are very narrow. The intensity...
Eccentricity of an Ellipse
An ellipse is a fundamental conic section defined by the constant sum of distances from any point on its curve to two fixed points, known as the foci. This geometric property can be physically demonstrated using a pencil, string, and two pins. By anchoring the string at both ends and maintaining it taut with a pencil, one can trace the outline of an ellipse.The shape and extent of the ellipse are determined by its eccentricity, e, defined as the ratio of the distance between the center and a...

