Discovery [1] | |
---|---|
Discovered by | F. Mallia |
Discovery site | Campo Catino Obs. |
Discovery date | 29 September 1999 |
Designations | |
(21795) Masi | |
Named after |
Gianluca Masi
[1] (Italian astronomer) |
1999 SN9 · 1988 UE 1993 BZ1 | |
main-belt
[1]
[2] · (
inner) Nysa [3] | |
Orbital characteristics [2] | |
Epoch 23 March 2018 ( JD 2458200.5) | |
Uncertainty parameter 0 | |
Observation arc | 64.45 yr (23,541 d) |
Aphelion | 2.8409 AU |
Perihelion | 1.9222 AU |
2.3815 AU | |
Eccentricity | 0.1929 |
3.68 yr (1,342 d) | |
337.35 ° | |
0° 16m 5.52s / day | |
Inclination | 1.8376° |
337.09° | |
81.681° | |
Physical characteristics | |
2.45
km (calculated)
[4] 3.150±0.164 km [5] [6] | |
13.862±0.0121 h [7] | |
0.20 (assumed)
[4] 0.235±0.037 [5] [6] | |
S (assumed) [4] | |
14.7
[6] 14.9 [2] 14.970±0.004 (R) [7] 15.41±0.14 [8] 15.42 [4] | |
21795 Masi ( provisional designation 1999 SN9) is a Nysian asteroid from the inner regions of the asteroid belt, approximately 3 kilometers (2 miles) in diameter. It was discovered on 29 September 1999, by Italian amateur astronomer Franco Mallia at the Campo Catino Astronomical Observatory in Lazio, Italy. [1] The likely S-type asteroid has a rotation period of 13.86 hours. [4] It was named for Italian astronomer Gianluca Masi. [1]
Masi is member of the Nysa family ( 405), [3] located in the Nysa–Polana complex and one of the largest asteroid families of the asteroid belt, named after 44 Nysa. [9] It orbits the Sun in the inner main-belt at a distance of 1.9–2.8 AU once every 3 years and 8 months (1,342 days; semi-major axis of 2.38 AU). Its orbit has an eccentricity of 0.19 and an inclination of 2 ° with respect to the ecliptic. [2] The body's observation arc begins with a precovery published by the Digitized Sky Survey and taken at the Palomar Observatory in April 1954, more than 45 years prior to its official discovery observation at Campo Catino. [1]
Masi is an assumed, stony S-type asteroid, [4] which is also the overall spectral type for members of the Nysa family of asteroids. [9]: 23
In September 2010, a rotational lightcurve of Masi was obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 13.862 hours with a relatively high brightness amplitude of 0.68 magnitude ( U=2). [7]
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Masi measures 3.150 kilometers in diameter and its surface has an albedo of 0.235, [5] [6] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20, and calculates a diameter of 2.45 kilometers based on an absolute magnitude of 15.42. [4]
This minor planet was named after Italian astrophysicist and astronomer, Gianluca Masi (born 1972), a researcher and discoverer of minor planets and variable stars, who became an avid amateur astronomer when he was 8 years old. [1] The official naming citation was published by the Minor Planet Center on 9 May 2001 ( M.P.C. 42679). [10]
Discovery [1] | |
---|---|
Discovered by | F. Mallia |
Discovery site | Campo Catino Obs. |
Discovery date | 29 September 1999 |
Designations | |
(21795) Masi | |
Named after |
Gianluca Masi
[1] (Italian astronomer) |
1999 SN9 · 1988 UE 1993 BZ1 | |
main-belt
[1]
[2] · (
inner) Nysa [3] | |
Orbital characteristics [2] | |
Epoch 23 March 2018 ( JD 2458200.5) | |
Uncertainty parameter 0 | |
Observation arc | 64.45 yr (23,541 d) |
Aphelion | 2.8409 AU |
Perihelion | 1.9222 AU |
2.3815 AU | |
Eccentricity | 0.1929 |
3.68 yr (1,342 d) | |
337.35 ° | |
0° 16m 5.52s / day | |
Inclination | 1.8376° |
337.09° | |
81.681° | |
Physical characteristics | |
2.45
km (calculated)
[4] 3.150±0.164 km [5] [6] | |
13.862±0.0121 h [7] | |
0.20 (assumed)
[4] 0.235±0.037 [5] [6] | |
S (assumed) [4] | |
14.7
[6] 14.9 [2] 14.970±0.004 (R) [7] 15.41±0.14 [8] 15.42 [4] | |
21795 Masi ( provisional designation 1999 SN9) is a Nysian asteroid from the inner regions of the asteroid belt, approximately 3 kilometers (2 miles) in diameter. It was discovered on 29 September 1999, by Italian amateur astronomer Franco Mallia at the Campo Catino Astronomical Observatory in Lazio, Italy. [1] The likely S-type asteroid has a rotation period of 13.86 hours. [4] It was named for Italian astronomer Gianluca Masi. [1]
Masi is member of the Nysa family ( 405), [3] located in the Nysa–Polana complex and one of the largest asteroid families of the asteroid belt, named after 44 Nysa. [9] It orbits the Sun in the inner main-belt at a distance of 1.9–2.8 AU once every 3 years and 8 months (1,342 days; semi-major axis of 2.38 AU). Its orbit has an eccentricity of 0.19 and an inclination of 2 ° with respect to the ecliptic. [2] The body's observation arc begins with a precovery published by the Digitized Sky Survey and taken at the Palomar Observatory in April 1954, more than 45 years prior to its official discovery observation at Campo Catino. [1]
Masi is an assumed, stony S-type asteroid, [4] which is also the overall spectral type for members of the Nysa family of asteroids. [9]: 23
In September 2010, a rotational lightcurve of Masi was obtained from photometric observations in the R-band by astronomers at the Palomar Transient Factory in California. Lightcurve analysis gave a rotation period of 13.862 hours with a relatively high brightness amplitude of 0.68 magnitude ( U=2). [7]
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Masi measures 3.150 kilometers in diameter and its surface has an albedo of 0.235, [5] [6] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20, and calculates a diameter of 2.45 kilometers based on an absolute magnitude of 15.42. [4]
This minor planet was named after Italian astrophysicist and astronomer, Gianluca Masi (born 1972), a researcher and discoverer of minor planets and variable stars, who became an avid amateur astronomer when he was 8 years old. [1] The official naming citation was published by the Minor Planet Center on 9 May 2001 ( M.P.C. 42679). [10]