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Celestial calendar Visibility of asteroids |
Name |
Opposition |
Magnitude |
Diameter |
Mean |
Eccentricity |
Daily |
|---|---|---|---|---|---|---|
(1) Ceres |
May 8 |
7.0m |
957 |
2.77 |
0.08 |
0.21o |
(2) Pallas |
Mar. 23 |
7.1m |
524 |
2.77 |
0.23 |
0.21o |
(3) Juno |
Dec. 9 |
7.6m |
274 |
2.67 |
0.26 |
0.23o |
(4) Vesta |
Jan. 5, 2006 |
6.2m |
512 |
2.36 |
0.09 |
0.27o |
(6) Hebe |
Apr. 13 |
9.9m |
190 |
2.43 |
0.20 |
0.26o |
(7) Iris |
June 3 |
9.2m |
211 |
2.39 |
0.23 |
0.27o |
(8) Flora |
Jan. 14 |
8.4m |
138 |
2.20 |
0.16 |
0.30o |
(11) Parthenope |
Dec. 9 |
9.8m |
153 |
2.45 |
0.10 |
0.26o |
(15) Eunomia |
Apr. 30 |
9.8m |
320 |
2.64 |
0.19 |
0.23o |
(18) Melpomene |
June 18 |
9.5m |
138 |
2.29 |
0.22 |
0.28o |
(20) Massalia |
Aug. 24 |
9.7m |
145 |
2.41 |
0.14 |
0.26o |
(29) Amphitrite |
Mar. 30 |
9.2m |
212 |
2.56 |
0.07 |
0.24o |
(39) Laetitia |
July 24 |
9.6m |
150 |
2.77 |
0.11 |
0.21o |
(1) Ceres
Date |
Apparent |
Apparent |
Visual |
True |
|---|---|---|---|---|
Apr. 10 |
15h 35.7m |
-9o 00' |
7.5m |
1.78 |
May 10 |
15h 12.1m |
-8o 30' |
7.0m |
1.69 |
June 9 |
14h 48.6m |
-9o 07' |
7.6m |
1.83 |
(2) Pallas
Date |
Apparent |
Apparent |
Visual |
True |
|---|---|---|---|---|
Feb. 19 |
12h 44.2m |
-2o 46' |
7.7m |
1.46 |
Mar. 21 |
12h 29.8m |
8o 25' |
7.1m |
1.37 |
Apr. 20 |
12h 11.1m |
17o 30' |
7.9m |
1.55 |
(3) Juno
Date |
Apparent |
Apparent |
Visual |
True |
|---|---|---|---|---|
Nov. 6, 2005 |
5h 33.3m |
1o 20' |
7.9m |
1.14 |
Dec. 6, 2005 |
5h 17.0m |
-1o 54' |
7.5m |
1.06 |
Jan. 5, 2006 |
4h 56.1m |
0o 17' |
7.9m |
1.17 |
(4) Vesta
Date |
Apparent |
Apparent |
Visual |
True |
|---|---|---|---|---|
Dec. 6, 2005 |
7h 34.8m |
20o 34' |
7.0m |
1.70 |
Jan. 5, 2006 |
7h 08.4m |
22o 46' |
6.3m |
1.55 |
Feb. 4, 2006 |
6h 39.5m |
24o 42' |
6.9m |
1.65 |
|
Glossary Eccentricity: a parameter that specifies the shape of a conic section; one of the standard elements used to describe an elliptic orbit. Mean Distance: the semimajor axis of an elliptic orbit. Opposition: a configuration of the Sun, Earth and a planet in which the apparent geocentric longitude of the planet differs by 180o from the apparent geocentric longitude of the Sun. Semimajor Axis: half the length of the major axis of an ellipse; a standard element used to describe an elliptical orbit. Astronomical Unit (AU): middle distance from Earth to Sun, equal 149.6 millions km. |
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Note: All the times
in this page are expressed in universal time (UT). |