Very long baseline radio interferometry (VLBI) with ground-based
observatories is limited by the size of Earth, the geographic distribution of
antennas, and the transparency of the atmosphere. In this whitepaper, we
present Capella, a tentative design of a space-only VLBI system. Using four
small (<500 kg) satellites on two orthogonal polar low-Earth orbits, and
single-band heterodyne receivers operating at frequencies around 690 GHz, the
interferometer is able to achieve angular resolutions of approximately 7
microarcsec. Within a total observing time of three days, a near-complete uv
plane coverage can be reached, with a 1-sigma point source sensitivity as good
as about 6~mJy for an instantaneous bandwidth of 1 GHz. The required downlink
data rates of >10 Gbps can be reached through near-infrared laser
communication; depending on the actual downlink speed, one or multiple ground
communication stations are necessary. We note that all key technologies
required for the Capella system are already available, some of them
off-the-shelf. Data can be correlated using dedicated versions of existing
Fourier transform (FX) software correlators; dedicated routines will be needed
to handle the effects of orbital motion, including relativistic corrections.
With the specifications assumed in this whitepaper, Capella will be able to
address a range of science cases, including: photon rings around supermassive
black holes; the acceleration and collimation zones of plasma jets emitted from
the vicinity of supermassive black holes; the chemical composition of accretion
flows into active galactic nuclei through observations of molecular absorption
lines; mapping supermassive binary black holes; the magnetic activity of stars;
and nova eruptions of symbiotic binary stars - and, like any substantially new
observing technique, has the potential for unexpected discoveries.Comment: 18 pages, 2 figures, 1 table. Whitepaper version 1.0. Living
document, will be updated when necessar