31.5: 天文学的一些有用常数(附录 E)
- Page ID
- 202856
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\(\newcommand{\avec}{\mathbf a}\) \(\newcommand{\bvec}{\mathbf b}\) \(\newcommand{\cvec}{\mathbf c}\) \(\newcommand{\dvec}{\mathbf d}\) \(\newcommand{\dtil}{\widetilde{\mathbf d}}\) \(\newcommand{\evec}{\mathbf e}\) \(\newcommand{\fvec}{\mathbf f}\) \(\newcommand{\nvec}{\mathbf n}\) \(\newcommand{\pvec}{\mathbf p}\) \(\newcommand{\qvec}{\mathbf q}\) \(\newcommand{\svec}{\mathbf s}\) \(\newcommand{\tvec}{\mathbf t}\) \(\newcommand{\uvec}{\mathbf u}\) \(\newcommand{\vvec}{\mathbf v}\) \(\newcommand{\wvec}{\mathbf w}\) \(\newcommand{\xvec}{\mathbf x}\) \(\newcommand{\yvec}{\mathbf y}\) \(\newcommand{\zvec}{\mathbf z}\) \(\newcommand{\rvec}{\mathbf r}\) \(\newcommand{\mvec}{\mathbf m}\) \(\newcommand{\zerovec}{\mathbf 0}\) \(\newcommand{\onevec}{\mathbf 1}\) \(\newcommand{\real}{\mathbb R}\) \(\newcommand{\twovec}[2]{\left[\begin{array}{r}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\ctwovec}[2]{\left[\begin{array}{c}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\threevec}[3]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\cthreevec}[3]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\fourvec}[4]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\cfourvec}[4]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\fivevec}[5]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\cfivevec}[5]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\mattwo}[4]{\left[\begin{array}{rr}#1 \amp #2 \\ #3 \amp #4 \\ \end{array}\right]}\) \(\newcommand{\laspan}[1]{\text{Span}\{#1\}}\) \(\newcommand{\bcal}{\cal B}\) \(\newcommand{\ccal}{\cal C}\) \(\newcommand{\scal}{\cal S}\) \(\newcommand{\wcal}{\cal W}\) \(\newcommand{\ecal}{\cal E}\) \(\newcommand{\coords}[2]{\left\{#1\right\}_{#2}}\) \(\newcommand{\gray}[1]{\color{gray}{#1}}\) \(\newcommand{\lgray}[1]{\color{lightgray}{#1}}\) \(\newcommand{\rank}{\operatorname{rank}}\) \(\newcommand{\row}{\text{Row}}\) \(\newcommand{\col}{\text{Col}}\) \(\renewcommand{\row}{\text{Row}}\) \(\newcommand{\nul}{\text{Nul}}\) \(\newcommand{\var}{\text{Var}}\) \(\newcommand{\corr}{\text{corr}}\) \(\newcommand{\len}[1]{\left|#1\right|}\) \(\newcommand{\bbar}{\overline{\bvec}}\) \(\newcommand{\bhat}{\widehat{\bvec}}\) \(\newcommand{\bperp}{\bvec^\perp}\) \(\newcommand{\xhat}{\widehat{\xvec}}\) \(\newcommand{\vhat}{\widehat{\vvec}}\) \(\newcommand{\uhat}{\widehat{\uvec}}\) \(\newcommand{\what}{\widehat{\wvec}}\) \(\newcommand{\Sighat}{\widehat{\Sigma}}\) \(\newcommand{\lt}{<}\) \(\newcommand{\gt}{>}\) \(\newcommand{\amp}{&}\) \(\definecolor{fillinmathshade}{gray}{0.9}\)| 表\(\PageIndex{1}\):物理常数 | |
|---|---|
| 姓名 | 价值 |
| \ (\ pageIndex {1}\):物理常量名称” data-valign= “top” class= “lt-phys-19716” > 光速 (c) | \ (\ pageIndex {1}\):物理常量值” data-valign= “top” class= “lt-phys-19716” >2.9979 × 10 8 m/s |
| \ (\ pageIndex {1}\):物理常量名称” data-valign= “top” class= “lt-phys-19716” > 引力常数 (G) | \ (\ pageIndex {1}\):物理常量值” data-valign= “top” class= “lt-phys-19716” >6.674 × 10 −11 m 3/(kg s 2) |
| \ (\ pageIndex {1}\):物理常量名称” data-valign= “top” class= “lt-Phys-19716” >Planck 的常量 (h) | \ (\ pageIndex {1}\):物理常量值” data-valign= “top” class= “lt-phys-19716” >6.626 × 10 −34 J-s |
| \ (\ pageIndex {1}\):物理常量名称” data-valign= “top” class= “lt-phys-19716” > 氢原子的质量 (M H) | \ (\ pageIndex {1}\):物理常量值” data-valign= “top” class= “lt-phys-19716” >1.673 × 10 −27 kg |
| \ (\ pageIndex {1}\):物理常量名称” data-valign= “top” class= “lt-phys-19716” > 电子质量 (M e) | \ (\ pageIndex {1}\):物理常量值” data-valign= “top” class= “lt-phys-19716” >9.109 × 10 −31 kg |
| \ (\ pageIndex {1}\):物理常量名称” data-valign= “top” class= “lt-Phys-19716">rydberg 常量 (R ∞) | \ (\ pageIndex {1}\):物理常量值” data-valign= “top” class= “lt-phys-19716” >1.0974 × 10 7 m −1 |
| \ (\ pageIndex {1}\):物理常量名称” data-valign= “top” class= “lt-phys-19716">Stefan-Boltzmann 常量 (α) | \ (\ pageIndex {1}\):物理常量值” data-valign= “top” class= “lt-phys-19716” >5.670×10 −8 J/ (s·m 2 deg 4) 1 |
| \ (\ pageIndex {1}\):物理常量名称” data-valign= “top” class= “lt-phys-19716">维也纳定律常量(λ max T) | \ (\ pageIndex {1}\):物理常量值” data-valign= “top” class= “lt-phys-19716” >2.898 × 10 −3 m K |
| \ (\ pageIndex {1}\):物理常量名称” data-valign= “top” class= “lt-phys-19716” > 电子伏特(能量)(eV) | \ (\ pageIndex {1}\):物理常量值” data-valign= “top” class= “lt-phys-19716” >1.602 × 10 −19 J |
| \ (\ pageIndex {1}\):物理常量名称” data-valign= “top” class= “lt-phys-19716” > 1 吨 TNT 的能量当量 | \ (\ pageIndex {1}\):物理常量值” data-valign= “top” class= “lt-phys-19716” >4.2 × 10 9 J |
| 表\(\PageIndex{2}\):天文常数 | |
|---|---|
| 姓名 | 价值 |
| \ (\ pageIndex {2}\):天文常量名称” data-valign= “top” class= “lt-phys-19716” > 天文单位(澳大利亚) | \ (\ pageIndex {2}\):天文常数值” data-valign= “top” class= “lt-phys-19716” >1.496 × 10 11 m |
| \ (\ pageIndex {2}\):天文常量名称” data-valign= “top” class= “lt-Phys-19716">光年 (ly) | \ (\ pageIndex {2}\):天文常数值” data-valign= “top” class= “lt-phys-19716” >9.461 × 10 15 m |
| \ (\ pageIndex {2}\):天文常量名称” data-valign= “top” class= “lt-phys-19716” >parsec (pc) | \ (\ pageIndex {2}\):天文常数值” data-valign= “top” class= “lt-phys-19716” >3.086 × 10 16 m = 3.262 光年 |
| \ (\ pageIndex {2}\):天文常量名称” data-valign= “top” class= “lt-phys-19716” > 恒星年 (y) | \ (\ pageIndex {2}\):天文常数值” data-valign= “top” class= “lt-phys-19716” >3.156×10 7 s |
| \ (\ pageIndex {2}\):天文常量名称” data-valign= “top” class= “lt-phys-19716” > 地球质量(M E arth) | \ (\ pageIndex {2}\):天文常数值” data-valign= “top” class= “lt-phys-19716” >5.974 × 10 24 kg |
| \ (\ pageIndex {2}\):天文常量名称” data-valign= “top” class= “lt-phys-19716” > 地球赤道半径(R Eart h) | \ (\ pageIndex {2}\):天文常数值” data-valign= “top” class= “lt-phys-19716” >6.378 × 10 6 m |
| \ (\ pageIndex {2}\):天文常量名称” data-valign= “top” class= “lt-phys-19716” > 黄道的倾斜 | \ (\ pageIndex {2}\):天文常数值” data-valign= “top” class= “lt-phys-19716” >23° 26' |
| \ (\ pageIndex {2}\):天文常量名称” data-valign= “top” class= “lt-phys-19716” > 地球的表面重力 (g) | \ (\ pageIndex {2}\):天文常数值” data-valign= “top” class= “lt-phys-19716” >9.807 m/s 2 |
| \ (\ pageIndex {2}\):天文常量名称” data-valign= “top” class= “lt-phys-19716” > 地球逃生速度(v 地球) | \ (\ pageIndex {2}\):天文常数值” data-valign= “top” class= “lt-phys-19716” >1.119 × 10 4 m/s |
| \ (\ pageIndex {2}\):天文常数名称” data-valign= “top” class= “lt-phys-19716” > 太阳质量(M Sun) | \ (\ pageIndex {2}\):天文常数值” data-valign= “top” class= “lt-phys-19716” >1.989×10 30 kg |
| \ (\ pageIndex {2}\):天文常量名称” data-valign= “top” class= “lt-phys-19716” > 太阳(R Sun)的赤道半径 | \ (\ pageIndex {2}\):天文常数值” data-valign= “top” class= “lt-phys-19716” >6.960 × 10 8 m |
| \ (\ pageIndex {2}\):天文常量名称” data-valign= “top” class= “lt-phys-19716” > 太阳(L Sun)的亮度 | \ (\ pageIndex {2}\):天文常数值” data-valign= “top” class= “lt-phys-19716” >3.85 × 10 26 W |
| \ (\ pageIndex {2}\):天文常量名称” data-valign= “top” class= “lt-phys-19716” > 太阳常数(地球接收的能量通量)(S) | \ (\ pageIndex {2}\):天文常数值” data-valign= “top” class= “lt-phys-19716” >1.368 × 10 3 W/m 2 |
| \ (\ pageIndex {2}\):天文常量名称” data-valign= “top” class= “lt-Phys-19716">哈勃常数 (H 0) | \ (\ pageIndex {2}\):天文常数值” data-valign= “top” class= “lt-phys-19716” > 每百万光年大约 20 km/s,或每兆帕秒大约 70 km/s |
脚注
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