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tabellen:uranus_de200

Uranus

mittlere Anomalien

Tabelle 1
$M_5 =$ $20\overset{\circ}{.}320992 + 2880\overset{\circ}{.}0 \cdot T + 154\overset{\circ}{.}904004 \cdot T$
$M_6 =$ $317\overset{\circ}{.}865996 + 1080\overset{\circ}{.}0 \cdot T + 142\overset{\circ}{.}112988 \cdot T$
$M_7 =$ $142\overset{\circ}{.}816212 + 360\overset{\circ}{.}0 \cdot T + 68\overset{\circ}{.}502564 \cdot T$
$M_8 =$ $259\overset{\circ}{.}805988 + 0\overset{\circ}{.}0 \cdot T + 218\overset{\circ}{.}467008 \cdot T$

Tabellen

\[\begin{align} dl &= \sum_{n=1}^{10} T^{t_n} (a_n \cos(p_n \ M_p + s_n \ M_s) + b_n \sin(p_n \ M_p + s_n \ M_s)) \\ db &= \sum_{n=1}^{10} T^{t_n} (c_n \cos(p_n \ M_p + s_n \ M_s) + d_n \sin(p_n \ M_p + s_n \ M_s)) \\ dr &= \sum_{n=1}^{10} T^{t_n} (e_n \cos(p_n \ M_p + s_n \ M_s) + f_n \sin(p_n \ M_p + s_n \ M_s)) \end{align}\tag{1}\]

Tabelle 2: Keplerterme
n $a_n['']$ $b_n['']$ $c_n['']$ $d_n['']$ $e_n['']$ $f_n['']$ $p_n$ $s_n$ $t_n$
$01$ $-78.1$ $19518.1$ $2759.5$ $-311.9$ $-90718.2$ $-334.7$ $1 $ $0 $ $0 $
$02$ $-81.6$ $107.7 $ $-2.8 $ $-43.7 $ $-497.4 $ $-379.5$ $1 $ $0 $ $1 $
$03$ $-6.6 $ $-3.1 $ $-0.4 $ $-0.5 $ $14.4 $ $-30.6 $ $1 $ $0 $ $2 $
$04$ $0.0 $ $-0.5 $ $0.0 $ $0.0 $ $2.4 $ $0.0 $ $1 $ $0 $ $3 $
$05$ $-2.4 $ $586.1 $ $130.6 $ $-14.3 $ $-2145.2 $ $-15.3 $ $2 $ $0 $ $0 $
$06$ $-4.5 $ $6.6 $ $0.7 $ $-1.6 $ $-24.2 $ $-17.8 $ $2 $ $0 $ $1 $
$07$ $-0.4 $ $0.0 $ $0.0 $ $0.0 $ $0.1 $ $-1.4 $ $2 $ $0 $ $2 $
$08$ $0.0 $ $24.5 $ $7.0 $ $-0.7 $ $-76.2 $ $-0.6 $ $3 $ $0 $ $0 $
$09$ $-0.2 $ $0.4 $ $0.1 $ $-0.1 $ $-1.4 $ $-0.8 $ $3 $ $0 $ $1 $
$10$ $0.0 $ $1.1 $ $0.4 $ $0.0 $ $-3.0 $ $0.1 $ $4 $ $0 $ $0 $

\[\begin{align} dl &= \sum_{n=11}^{61} T^{t_n} (a_n \cos(p_n \ M_p + s_n \ M_s + t_n \ M_t) + b_n \sin(p_n \ M_p + s_n \ M_s + t_n \ M_t)) \\ db &= \sum_{n=11}^{61} T^{t_n} (c_n \cos(p_n \ M_p + s_n \ M_s + t_n \ M_t) + d_n \sin(p_n \ M_p + s_n \ M_s + t_n \ M_t)) \\ dr &= \sum_{n=11}^{61} T^{t_n} (e_n \cos(p_n \ M_p + s_n \ M_s + t_n \ M_t) + f_n \sin(p_n \ M_p + s_n \ M_s + t_n \ M_t)) \end{align}\tag{2}\]

Tabelle 3: Störterme der Planeten
Störungen durch den Jupiter
n $a_n['']$ $b_n['']$ $c_n['']$ $d_n['']$ $e_n['']$ $f_n['']$ $p_n$ $s_n$ $t_n$
$11$ $0.0 $ $0.0 $ $-0.1 $ $0.0 $ $-0.1 $ $1.7 $ $-1$ $-1$ $0 $
$12$ $0.5 $ $-1.2 $ $-0.9 $ $0.1 $ $18.9 $ $9.1 $ $0 $ $-1$ $0 $
$13$ $-21.2$ $48.7 $ $0.0 $ $0.0 $ $-455.5 $ $198.8 $ $1 $ $-1$ $0 $
$14$ $-0.5 $ $1.2 $ $0.0 $ $0.0 $ $-10.9 $ $-4.8 $ $1 $ $-2$ $0 $
$15$ $-1.3 $ $3.2 $ $0.3 $ $0.1 $ $-23.2 $ $-11.1 $ $2 $ $-1$ $0 $
$16$ $-0.2 $ $0.2 $ $0.0 $ $0.0 $ $1.1 $ $1.5 $ $2 $ $-2$ $0 $
$17$ $0.0 $ $0.2 $ $0.0 $ $0.0 $ $-1.8 $ $0.4 $ $3 $ $-1$ $0 $
Störungen durch den Saturn
n $a_n['']$ $b_n['']$ $c_n['']$ $d_n['']$ $e_n['']$ $f_n['']$ $p_n$ $s_n$ $t_n$
$18$ $1.4 $ $-0.5 $ $-0.4 $ $-0.8 $ $-6.4 $ $9.0 $ $0 $ $-1$ $0 $
$19$ $-18.6$ $-12.6 $ $1.0 $ $0.3 $ $36.7 $ $-336.8$ $1 $ $-1$ $0 $
$20$ $-0.7 $ $-0.3 $ $0.1 $ $0.0 $ $0.5 $ $-7.5 $ $1 $ $-2$ $0 $
$21$ $20.0 $ $-141.6 $ $3.1 $ $-0.8 $ $-587.1 $ $-107.0$ $2 $ $-1$ $0 $
$22$ $1.0 $ $1.4 $ $0.0 $ $0.0 $ $5.8 $ $-4.0 $ $2 $ $-1$ $1 $
$23$ $1.6 $ $-3.8 $ $0.0 $ $0.0 $ $-35.6 $ $-16.0 $ $2 $ $-2$ $0 $
$24$ $75.3 $ $-100.9 $ $-0.8 $ $0.1 $ $128.9 $ $77.5 $ $3 $ $-1$ $0 $
$25$ $0.2 $ $1.8 $ $0.0 $ $0.0 $ $-1.9 $ $0.3 $ $3 $ $-1$ $1 $
$26$ $2.3 $ $-1.3 $ $0.0 $ $0.1 $ $-9.5 $ $-17.9 $ $3 $ $-2$ $0 $
$27$ $-0.7 $ $-0.5 $ $0.0 $ $0.0 $ $-4.9 $ $6.8 $ $3 $ $-3$ $0 $
$28$ $3.4 $ $-5.0 $ $-0.8 $ $-0.5 $ $21.6 $ $14.3 $ $4 $ $-1$ $0 $
$29$ $1.9 $ $0.1 $ $0.0 $ $0.0 $ $1.2 $ $-12.1 $ $4 $ $-2$ $0 $
$30$ $-0.1 $ $-0.4 $ $0.0 $ $0.0 $ $-3.9 $ $1.2 $ $4 $ $-3$ $0 $
$31$ $-0.2 $ $0.1 $ $0.0 $ $0.0 $ $1.6 $ $1.8 $ $4 $ $-4$ $0 $
$32$ $0.2 $ $-0.3 $ $-0.1 $ $0.0 $ $1.0 $ $0.6 $ $5 $ $-1$ $0 $
$33$ $-2.2 $ $-2.2 $ $0.0 $ $0.0 $ $-7.7 $ $8.5 $ $5 $ $-2$ $0 $
$34$ $0.1 $ $-0.2 $ $0.0 $ $0.0 $ $-1.4 $ $-0.4 $ $5 $ $-3$ $0 $
$35$ $-0.1 $ $0.0 $ $0.0 $ $0.0 $ $0.1 $ $1.2 $ $5 $ $-4$ $0 $
$36$ $-0.2 $ $-0.6 $ $0.0 $ $0.0 $ $1.4 $ $-0.7 $ $6 $ $-2$ $0 $
Störungen durch den Neptun
n $a_n['']$ $b_n['']$ $c_n['']$ $d_n['']$ $e_n['']$ $f_n['']$ $p_n$ $s_n$ $t_n$
$37$ $-0.2 $ $0.2 $ $-0.1 $ $0.0 $ $0.7 $ $0.7 $ $-1$ $-1$ $0 $
$38$ $-2.8 $ $2.5 $ $-0.4 $ $-0.1 $ $8.7 $ $10.5 $ $0 $ $-1$ $0 $
$39$ $-28.4$ $20.3 $ $0.0 $ $0.0 $ $-51.4 $ $-72.0 $ $1 $ $-1$ $0 $
$40$ $-0.6 $ $-0.1 $ $0.2 $ $0.4 $ $4.2 $ $-14.6 $ $1 $ $-2$ $0 $
$41$ $0.2 $ $0.5 $ $-0.1 $ $0.1 $ $3.4 $ $-1.6 $ $1 $ $-3$ $0 $
$42$ $-1.8 $ $1.3 $ $0.0 $ $0.3 $ $-5.5 $ $-7.7 $ $2 $ $-1$ $0 $
$43$ $29.4 $ $10.2 $ $0.0 $ $0.0 $ $-29.0 $ $83.2 $ $2 $ $-2$ $0 $
$44$ $8.8 $ $17.8 $ $-0.1 $ $-0.3 $ $-41.9 $ $21.5 $ $2 $ $-3$ $0 $
$45$ $0.0 $ $0.1 $ $0.1 $ $0.0 $ $-2.1 $ $-0.9 $ $2 $ $-4$ $0 $
$46$ $1.5 $ $0.5 $ $0.1 $ $-0.2 $ $-1.7 $ $5.1 $ $3 $ $-2$ $0 $
$47$ $4.4 $ $14.6 $ $0.1 $ $-0.1 $ $-84.3 $ $-25.2 $ $3 $ $-3$ $0 $
$48$ $2.4 $ $-4.5 $ $0.0 $ $0.0 $ $12.0 $ $6.2 $ $3 $ $-4$ $0 $
$49$ $2.9 $ $-0.9 $ $0.0 $ $0.0 $ $2.1 $ $6.2 $ $3 $ $-5$ $0 $
$50$ $0.3 $ $1.0 $ $0.1 $ $-0.1 $ $-4.0 $ $1.1 $ $4 $ $-3$ $0 $
$51$ $2.1 $ $-2.7 $ $0.0 $ $0.0 $ $17.9 $ $14.0 $ $4 $ $-4$ $0 $
$52$ $3.0 $ $-0.4 $ $-0.1 $ $-0.1 $ $2.3 $ $17.6 $ $4 $ $-5$ $0 $
$53$ $-0.6 $ $-0.5 $ $0.0 $ $0.0 $ $1.1 $ $-1.6 $ $4 $ $-6$ $0 $
$54$ $0.2 $ $-0.2 $ $0.0 $ $0.0 $ $1.0 $ $0.8 $ $5 $ $-4$ $0 $
$55$ $-0.9 $ $-0.1 $ $0.0 $ $0.0 $ $0.6 $ $-7.1 $ $5 $ $-5$ $0 $
$56$ $-0.5 $ $-0.6 $ $0.0 $ $0.0 $ $3.8 $ $-3.6 $ $5 $ $-6$ $0 $
$57$ $0.0 $ $-0.5 $ $0.0 $ $0.0 $ $3.0 $ $0.1 $ $5 $ $-7$ $0 $
$58$ $0.2 $ $0.3 $ $0.0 $ $0.0 $ $-2.7 $ $1.6 $ $6 $ $-6$ $0 $
$59$ $-0.1 $ $0.2 $ $0.0 $ $0.0 $ $-2.0 $ $-0.4 $ $6 $ $-7$ $0 $
$60$ $0.1 $ $-0.2 $ $0.0 $ $0.0 $ $1.3 $ $0.5 $ $7 $ $-7$ $0 $
$61$ $0.1 $ $0.0 $ $0.0 $ $0.0 $ $0.4 $ $0.9 $ $7 $ $-8$ $0 $

\[\begin{align} dl &= \sum_{n=62}^{70} a_n \cos(p_n \ M_p + s_n \ M_s + t_n \ M_t) + b_n \sin(p_n \ M_p + s_n \ M_s + t_n \ M_t) \\ db &= \sum_{n=62}^{70} c_n \cos(p_n \ M_p + s_n \ M_s + t_n \ M_t) + d_n \sin(p_n \ M_p + s_n \ M_s + t_n \ M_t) \\ dr &= \sum_{n=62}^{70} e_n \cos(p_n \ M_p + s_n \ M_s + t_n \ M_t) + f_n \sin(p_n \ M_p + s_n \ M_s + t_n \ M_t) \end{align}\tag{3}\]

Tabelle 3: Störungen durch den Jupiter und den Saturn
n $a_n['']$ $b_n['']$ $c_n['']$ $d_n['']$ $e_n['']$ $f_n['']$ $p_n$ $s_n$ $t_n$
$62$ $-0.7 $ $0.4 $ $0.0 $ $0.0 $ $-1.5 $ $-2.5 $ $-2$ $2 $ $-4$
$63$ $-0.1 $ $-0.1 $ $0.0 $ $0.0 $ $-2.2 $ $1.0 $ $-1$ $2 $ $-4$
$64$ $0.1 $ $-0.4 $ $0.0 $ $0.0 $ $1.4 $ $0.2 $ $1 $ $0 $ $-5$
$65$ $0.4 $ $0.5 $ $0.0 $ $0.0 $ $-0.8 $ $-0.8 $ $1 $ $0 $ $-6$
$66$ $5.7 $ $6.3 $ $0.0 $ $0.0 $ $28.5 $ $-25.5 $ $2 $ $0 $ $-6$
$67$ $+0.1\cdot T$ $-0.2\cdot T$ $+0.0\cdot T$ $+0.0\cdot T$ $-1.1\cdot T$ $-0.6\cdot T$ $2$ $0$ $-6$
$68$ $-1.4 $ $29.2$ $0.0$ $0.0$ $-11.4$ $1.1$ $3$ $0$ $-6$
$69$ $+0.8\cdot T$ $-0.4\cdot T$ $+0.0\cdot T$ $+0.0\cdot T$ $+0.2\cdot T$ $+0.3\cdot T$ $3$ $0$ $-6$
$70$ $0.0$ $1.3$ $0.0$ $0.0$ $-6.0$ $-0.1$ $4$ $0$ $-6$

Heliozentrische Koordinaten

\[\begin{align} l_7 &= M_7 + 170\overset{\circ}{.}454348 + (5082\overset{''}{.}3\cdot T + 34\overset{''}{.}2\cdot T^2 + \text{dl})/3600'' \\ b_7 &= (- 130\overset{''}{.}61 - 0\overset{''}{.}54\cdot T + 0\overset{''}{.}04\cdot T^2 + \text{db})/3600'' \\ r_7 &= 19.211991\text{ AE} - 3.33 \cdot 10^{-4}\text{ AE} \cdot T - 5.0 \cdot 10^{-6}\text{ AE} \cdot T^2 + 10^{-5}\text{ AE dr} \end{align}\tag{4}\]

tabellen/uranus_de200.txt · Zuletzt geändert: 2024/05/11 14:54 von hcgreier