J/A+AS/128/179      Precision meteor orbits (Betlem+ 1998)

Precision meteor orbits obtained by the Dutch Meteor Society - Photographic Meteor Survey (1981-1993) Betlem H., ter Kuile C.R., de Lignie M., van't Leven J., Jobse K., Miskotte K., Jenniskens P. <Astron. Astrophys. Suppl. Ser. 128, 179 (1998)> =1998A&AS..128..179B 1998A&AS..128..179B (SIMBAD/NED BibCode)
ADC_Keywords: Solar system ; Positional data ; Space velocities Keywords: meteoroids Description: Orbital elements, encounter data and other relevant information of 359 photographic meteors (Table 2 of the paper). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2a 128 359 *Photographic orbital data of 359 multi station meteors table2b 100 359 *Trajectory data of 359 multi station meteors -------------------------------------------------------------------------------- Note to table2a and table2b: Data obtained by the Dutch Meteor Society between 1981 and 1993 -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2a -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Code DMS sequential numbering starting with the year 7- 8 I2 --- Month Month 10- 16 F7.4 d Day Day and time (UT) in decimal days 18 I1 --- Nstat Number of multi-station components 20- 24 A5 --- Stream Meteor stream identification 26- 28 I3 mag Mv Absolute visual magnitude at a distance of 100km 30- 34 F5.3 AU q Perihelion distance 36- 40 F5.3 AU e_q rms uncertainty on q 42- 48 F7.2 AU a Semi-major axis 50- 55 F6.3 AU-1 1/a Inverse semi-major axis 57- 61 F5.3 AU-1 e_1/a rms uncertainty on 63- 67 F5.3 --- e Eccentricity 69- 73 F5.3 --- e_e rms uncertainty on e 75- 80 F6.2 deg i Inclination of the orbit with respect to the ecliptic (Eq. 2000) 82- 86 F5.2 deg e_i rms uncertainty on i 88- 93 F6.2 deg omega Argument of perihelion (Eq. 2000) 95- 99 F5.2 deg e_omega rms uncertainty on omega 101-108 F8.4 deg Node Ascensing node (Eq. 2000) 110-115 F6.4 deg e_Node rms uncertainty on Node 117-122 F6.2 deg pi Longitude of perihelion (Eq. 2000) 124-128 F5.2 deg e_pi rms uncertainty on pi -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2b -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- Code DMS sequential numbering starting with the year 7- 11 F5.2 km/s Vg Geocentric velocity 13- 17 F5.2 km/s Vh Heliocentric velocity 19- 23 F5.2 km/s Vinf Apparent pre-atmospheric velocity 25- 29 F5.2 km/s Vel Average velocity along trajectory 31- 33 F3.1 km/s e_Vel rms uncertainty on Vel 35- 39 F5.1 km Hbeg ? Beginning height 41- 45 F5.1 km Hmax ? Height of brightest point on meteor track 47- 50 F4.1 km Hend ? End height of meteor 52- 57 F6.2 deg RAdeg Apparent right ascension of radiant (J2000) 59- 63 F5.2 deg e_RAdeg ? Error due to uncertainty in time of meteor, or spread in solutions for all possible sets of two stations 65- 70 F6.2 deg DEdeg Apparent declination of radiant (J2000) 72- 75 F4.2 deg e_DEdeg ? Error due to uncertainty in time of meteor, or spread in solutions for all possible sets of two stations 77- 82 F6.2 deg RAgeo Geocentric right ascension of radiant (J2000) 84- 89 F6.2 deg DEgeo Geocentric declination (J2000) 91- 95 F5.3 --- CosZR Cosine of zenith angle of radiant at time of meteor 97-100 F4.1 deg Qmax Convergence angle between planes through meteor and photographic station, maximum value of all combinations -------------------------------------------------------------------------------- Acknowledgements: Hans Betlem References: A subset of these data are available through the IAU Meteor Data Center in Lund, Sweden. For further information see the website of the Dutch Meteor Society http://www.pi.net/~terkuile/meteors/dms.htm
(End) Patricia Bauer [CDS] 11-Jul-1997
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line