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HD 23134


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The VLTI PRIMA Facility
The Phase Referenced Imaging and Microarcsecond Astrometry (PRIMA)instrument was recently delivered to the summit of Cerro Paranal andinstalled as part of the Very Large Telescope Interferometer (VLTI)infrastructure. PRIMA is designed to (i) provide phase-referencedinterferometric imaging at milliarcsecond scales, (ii) enable faint starscience several magnitudes fainter than the current atmospheric limitsof the VLTI, and (iii) provide astrometric measurements at the tens ofmicro-arcsecond level. PRIMA has successfully seen first fringes and iscurrently (as of late 2008) undergoing initial commissioning tests.

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Observation and Astrometry data

Constellation:Fluss Eridanus
Right ascension:03h42m01.96s
Declination:-21°14'14.1"
Apparent magnitude:8.318
Distance:158.228 parsecs
Proper motion RA:-19
Proper motion Dec:-20.3
B-T magnitude:9.576
V-T magnitude:8.422

Catalogs and designations:
Proper Names   (Edit)
HD 1989HD 23134
TYCHO-2 2000TYC 5880-1269-1
USNO-A2.0USNO-A2 0675-01262312
HIPHIP 17284

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