Discovery | |
---|---|
Discovered by | Johann Palisa |
Discovery date | 5 June 1885 |
Designations | |
(248) Lameia | |
Pronunciation | /ləˈmiːə/[1] |
Named after | Lamia |
A885 LA, 1959 LO | |
Main belt | |
Orbital characteristics[2] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 130.86 yr (47,796 d) |
Aphelion | 2.64 AU (394.30 Gm) |
Perihelion | 2.31 AU (345.06 Gm) |
2.47 AU (369.67 Gm) | |
Eccentricity | 0.066588 |
3.88 yr (1,418.9 d) | |
Average orbital speed | 18.95 km/s |
264.207° | |
0° 15m 13.392s / day | |
Inclination | 4.0581° |
246.845° | |
10.782° | |
Physical characteristics | |
Dimensions | 48.66±2.5 km[3] |
11.912 h (0.4963 d) | |
0.0615±0.007 | |
10.2 | |
248 Lameia is a typical main belt asteroid. It was discovered by Austrian astronomer Johann Palisa on 5 June 1885 in Vienna and was named after the Lamia, a lover of Zeus in Ancient Greek mythology. 248 Lameia is orbiting the Sun with a period of 3.88 years and a low eccentricity (ovalness) of 0.067.[2] The semimajor axis of 2.47 AU is slightly inward from the 3:1 Kirkwood Gap.[4] Its orbital plane is inclined by 4° to the plane of the ecliptic.[2]
On 27 June 1998 an occultation of the 8th magnitude star PPM 236753 (HD 188960)[5] by 248 Lameia was timed by five observers near Gauteng, South Africa. The chords produced a rough size estimate of a 62 × 53 km ellipse.[6] The size estimate based on IRAS Minor Planet Survey data is ~49 km. The rotation rate of this object is commensurate with the rotation of the Earth, requiring observations from different locations to build a complete light curve. These yield a rotation estimate of 11.912±0.001 h with a brightness variation of 0.17±0.01 magnitude in amplitude. The same data set gives a size estimate of 47±3 km, in agreement with earlier measurements.[3]
Infrared imaging of this body shows a relatively featureless spectra that suggests materials that are similar to carbonaceous chondrite meteorites.[7]
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