02037+2556 STF 208 AB (10 Ari)
02h 03m 39.26s +25° 56' 07.6" P.A. 349.00 sep 1.3 mag 5.82,7.87 Sp F8IV dist. 48.71 pc (158.89 l.y.)
Coord 2000 |
02037+2556 |
|
Discov num |
STF 208 |
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Comp |
AB |
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Coord arcsec 2000 |
02 03 39.26 +25 56 07.6 |
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Date first |
1821 |
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Date last |
2018 |
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Obs |
238 |
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Pa first |
23 |
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Pa last |
348.6 |
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P.A. Now (θ) |
350.2° |
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Sep first |
2.0 |
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Sep last |
1.31 |
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Sep. Now (ρ) |
1.608" |
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Mag pri |
5.82 |
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Mag sec |
7.87 |
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delta mag (ΔM) |
2.05 |
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Spectral class |
F8IV (yellow-white) |
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Pri motion ra |
+134 |
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Sec motion ra |
+134 |
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Pri motion dec |
+010 |
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Sec motion dec |
+010 |
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Notes |
N
O
(See Notes, Orbital solution) |
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This double is physical.
02037+2556 SYSTEM COMPONENTS
Show |
name |
SAO |
coord |
wds_name |
last |
obs |
pa |
sep |
mag1 |
mag2 |
d_mag |
orb |
current |
Show |
10 Ari |
75114 |
02 03 39 +25 56 08 |
STF 208 AB |
2018 |
238 |
349 |
1.3 |
5.82 |
7.87 |
2.05 |
Y |
<=== |
Show |
|
75114 |
02 03 39 +25 56 08 |
STF 208 AB,C |
2001 |
3 |
150 |
95.3 |
5.67 |
13.50 |
7.83 |
|
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Triple system
4 estimated visually detectable stars in this system
OTHER CATALOGS AND DESIGNATIONS
Name |
10 Ari |
|
Constellation |
Aries |
|
SAO |
75114 |
|
HIP |
9621 |
|
Tycho2 |
1761-02538-1 |
|
Gaia DR2 |
105599987245304192 |
|
HD |
12558 |
|
HR |
605 |
|
GC |
2476 |
|
ADS |
1631 |
|
BD |
BD+25 341 |
|
Flamsteed |
10 Arietis |
|
Flamsteed name |
10 Ari |
|
Distance |
48.71 |
|
Distance ly |
158.89 |
|
ORBITAL ELEMENTS
Period (P) | 325y | |
Periastron (T) | 1931.6y | |
Semi-major axis (a) | 1.39a | |
Eccentricity (e) | 0.59 | |
Inclination (i) | 51° | |
Longitude of periastron (ω) | 165° | |
Node (Ω) | 20.5° | |
Notes | n | |
Reference | Hei1996a | |
Equinox | | |
Last observation | | |
Grade | 3 | (1=Definitive, 9=Indet.) |
label |
theta |
rho |
2000 |
338.0 |
1.261 |
2001 |
338.6 |
1.277 |
2002 |
339.3 |
1.294 |
2003 |
339.9 |
1.310 |
2004 |
340.6 |
1.326 |
2005 |
341.2 |
1.342 |
2006 |
341.8 |
1.358 |
2007 |
342.4 |
1.374 |
2008 |
342.9 |
1.389 |
2009 |
343.5 |
1.405 |
2010 |
344.0 |
1.420 |
2011 |
344.6 |
1.436 |
2012 |
345.1 |
1.451 |
2013 |
345.6 |
1.466 |
2014 |
346.1 |
1.481 |
2015 |
346.6 |
1.495 |
2016 |
347.1 |
1.510 |
2017 |
347.5 |
1.524 |
2018 |
348.0 |
1.538 |
2019 |
348.5 |
1.553 |
2020 |
348.9 |
1.567 |
2021 |
349.3 |
1.580 |
2022 |
349.8 |
1.594 |
2023 |
350.2 |
1.608 |
2024 |
350.6 |
1.621 |
2025 |
351.0 |
1.634 |
2026 |
351.4 |
1.647 |
2027 |
351.8 |
1.660 |
2028 |
352.2 |
1.673 |
2029 |
352.6 |
1.685 |
2030 |
353.0 |
1.698 |
2031 |
353.4 |
1.710 |
2032 |
353.7 |
1.722 |
2033 |
354.1 |
1.734 |
2034 |
354.5 |
1.746 |
2035 |
354.8 |
1.758 |
2036 |
355.2 |
1.769 |
2037 |
355.5 |
1.781 |
2038 |
355.8 |
1.792 |
2039 |
356.2 |
1.803 |
2040 |
356.5 |
1.814 |
2041 |
356.8 |
1.825 |
2042 |
357.2 |
1.835 |
2043 |
357.5 |
1.846 |
2044 |
357.8 |
1.856 |
2045 |
358.1 |
1.866 |
2046 |
358.4 |
1.876 |
2047 |
358.7 |
1.886 |
2048 |
359.0 |
1.895 |
2049 |
359.3 |
1.905 |
2050 |
359.6 |
1.914 |
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Note: Theta is PA, Rho is Sep. For yearly orbits, data refer to Jan 1st.
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Measures: green=micrometric, blue=interferometric, purple=photographic |
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