Discovery [1] | |
---|---|
Discovered by | M. F. Wolf |
Discovery site | Heidelberg Obs. |
Discovery date | 22 December 1891 |
Designations | |
(323) Brucia | |
Pronunciation | /ˈbruːsiə, ˈbruːʃə/ |
Named after |
Catherine Wolfe Bruce
[2] (American philanthropist) |
1934 JC · A923 JA | |
main-belt · (
inner) Phocaea [3] · ex- Mars-crosser [4] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 ( JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 125.35 yr (45,785 days) |
Aphelion | 3.0979 AU |
Perihelion | 1.6662 AU |
2.3820 AU | |
Eccentricity | 0.3005 |
3.68 yr (1,343 days) | |
106.64 ° | |
0° 16m 5.16s / day | |
Inclination | 24.230° |
97.398° | |
291.26° | |
Mars MOID | 0.3464 AU |
Physical characteristics | |
Dimensions | 27.714±0.300
km
[5] 29.23±2.92 km [6] 32.395±0.317 km [7] 35.82±1.7 km [4] [8] 37.29±0.76 km [9] |
9.46
h
[10] 9.4602±0.0001 h [11] 9.463±0.005 h [12] 10 h [4] | |
0.165±0.007
[9] 0.1765±0.018 [8] 0.2174±0.0421 [7] 0.265±0.053 [6] 0.295±0.046 [5] | |
Tholen =
S
[1]
[4] B–V = 0.893 [1] U–B = 0.480 [1] | |
9.09±0.58 [13] · 9.73 [1] [4] [6] [7] [8] [9] | |
Brucia ( minor planet designation: 323 Brucia) is a stony Phocaea asteroid and former Mars-crosser from the inner regions of the asteroid belt, approximately 33 kilometers (21 miles) in diameter. It was the first asteroid to be discovered by the use of astrophotography. [14]
Brucia was also the first of over 200 asteroids discovered by Max Wolf, a pioneer in that method of finding astronomical objects. Discovered on December 22, 1891, when he was 28 years old, it was named in honour of Catherine Wolfe Bruce, a noted patroness of the science of astronomy, who had donated $10,000 for the construction of the telescope used by Wolf. [2] [15]
The asteroid is a member of the Phocaea family ( 701), [3] a large family of stony S-type asteroids with nearly two thousand known members. [16]: 23 It was an outer Mars-crossing asteroid with perihelion less than 1.666 AU [1] until July 2017. For comparison, asteroid 4222 Nancita will become a Mars-crosser in June 2019. (6454) 1991 UG1 was a Mars-crossing asteroid until January 2016. [17][ needs update]
Brucia has a synodic rotation period of 9.463 hours (as of 1998). [4] According to the survey carried out by the Infrared Astronomical Satellite, Brucia measures 35.82 kilometers in diameter and its surface has an albedo of 0.1765. [8]
Discovery [1] | |
---|---|
Discovered by | M. F. Wolf |
Discovery site | Heidelberg Obs. |
Discovery date | 22 December 1891 |
Designations | |
(323) Brucia | |
Pronunciation | /ˈbruːsiə, ˈbruːʃə/ |
Named after |
Catherine Wolfe Bruce
[2] (American philanthropist) |
1934 JC · A923 JA | |
main-belt · (
inner) Phocaea [3] · ex- Mars-crosser [4] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 ( JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 125.35 yr (45,785 days) |
Aphelion | 3.0979 AU |
Perihelion | 1.6662 AU |
2.3820 AU | |
Eccentricity | 0.3005 |
3.68 yr (1,343 days) | |
106.64 ° | |
0° 16m 5.16s / day | |
Inclination | 24.230° |
97.398° | |
291.26° | |
Mars MOID | 0.3464 AU |
Physical characteristics | |
Dimensions | 27.714±0.300
km
[5] 29.23±2.92 km [6] 32.395±0.317 km [7] 35.82±1.7 km [4] [8] 37.29±0.76 km [9] |
9.46
h
[10] 9.4602±0.0001 h [11] 9.463±0.005 h [12] 10 h [4] | |
0.165±0.007
[9] 0.1765±0.018 [8] 0.2174±0.0421 [7] 0.265±0.053 [6] 0.295±0.046 [5] | |
Tholen =
S
[1]
[4] B–V = 0.893 [1] U–B = 0.480 [1] | |
9.09±0.58 [13] · 9.73 [1] [4] [6] [7] [8] [9] | |
Brucia ( minor planet designation: 323 Brucia) is a stony Phocaea asteroid and former Mars-crosser from the inner regions of the asteroid belt, approximately 33 kilometers (21 miles) in diameter. It was the first asteroid to be discovered by the use of astrophotography. [14]
Brucia was also the first of over 200 asteroids discovered by Max Wolf, a pioneer in that method of finding astronomical objects. Discovered on December 22, 1891, when he was 28 years old, it was named in honour of Catherine Wolfe Bruce, a noted patroness of the science of astronomy, who had donated $10,000 for the construction of the telescope used by Wolf. [2] [15]
The asteroid is a member of the Phocaea family ( 701), [3] a large family of stony S-type asteroids with nearly two thousand known members. [16]: 23 It was an outer Mars-crossing asteroid with perihelion less than 1.666 AU [1] until July 2017. For comparison, asteroid 4222 Nancita will become a Mars-crosser in June 2019. (6454) 1991 UG1 was a Mars-crossing asteroid until January 2016. [17][ needs update]
Brucia has a synodic rotation period of 9.463 hours (as of 1998). [4] According to the survey carried out by the Infrared Astronomical Satellite, Brucia measures 35.82 kilometers in diameter and its surface has an albedo of 0.1765. [8]