ULTRASAT

A model of the planned ULTRASAT satellite

ULTRASAT (Ultraviolet Transient Astronomy Satellite) is a proposed astronomical satellite mission whose wide-angle UV telescope will detect and monitor transient astrophysical phenomena in the near-ultraviolet spectral region. ULTRASAT will observe a large patch of sky, more than 200 square degrees, alternating every six months between the southern and northern hemisphere. The satellite will orbit the Earth from an altitude of about 300 km above the geosynchronous orbit, getting a ‘ride’ as a secondary payload in the fairing of the rocket carrying a communications satellite. Upon detection of a transient event, ULTRASAT will provide alerts to other ground-based and space telescopes to be directed to the source for further observation of the event in other wavelength bands. A joint American-Israeli proposal for this project was submitted to NASA by a team from Caltech/JPL (Jet Propulsion Laboratory), the Weizmann Institute of Science and Israel Aerospace Industries (IAI). The Israeli contribution will be funded by the Israel Space Agency[1] and launch is expected before 2021.

Background

The ULTRASAT initiative was born in 2010 in discussions between Weizmann Institute (WIS) and Caltech scientists together with the Israel Space Agency (ISA) to meet the need for a wide field space telescope for studying transient astronomical events, in a small satellite such as those suitable for SMEX. In the preliminary investigation phase, various other bands were considered, including X-ray. The ultraviolet was selected due to the technology maturity, the higher chances of successful implementation and the need to continue exploring this wavelength region.[2] The importance of this project is confirmed in [3] which says that the discovery rate for UV variable sources and UV transients could increase by several orders of magnitude with the launch of a space-based UV mission with a wide field of view (several deg2) and [4] which states that "The proposed ULTRASAT mission could discover hundreds of tidal disruption events per year in the UV.

The project, originally called LIMSAT, was renamed ULTRASAT - Ultraviolet TRansient Astronomy SATellite in 2011 when a proposal was submitted to NASA for the [Explorers program] 2012 Mission of Opportunity section, in collaboration with NASA's Ames Research Center. Due to the sequester and NASA budget cuts, no proposal was selected that year. Following considerable changes in the configuration of the telescope, the planned orbit and the satellite bus, a new proposal was submitted in December 2014 in collaboration with JPL. From a concept of eight small refractive UV telescopes on a satellite in low earth orbit, ULTRASAT evolved to a single wide-field Schmidt telescope in super-geosynchronous orbit.

Science

Time domain astronomy has potential for making unusual discoveries. Specifically the ultraviolet (UV) variable sky is relatively poorly explored, even though it offers exciting scientific prospects. Welsh, 2005, describes the discoveries made by GALEX, which would be vastly increased by ULTRASAT[5] One field where short cadence UV observations can make a big difference is the explosion marking the death of a star, known as a supernova (plural: Supernovae, abbreviated to SNe). In the article by Ganot, 2015[6] it is estimated that ULTRASAT would detect more that 100 SNe per year. The UV signals from SNe precede the optical signal, enabling discovery of the SN at an early stage when the light curve is uncontaminated by later processes. Since for a transient event there is typically no early warning and the event’s position in the sky is of statistical nature, most transients are discovered by ground telescopes with limited fields of view, often long after the start of the event, although dedicated surveys are reducing this to around one day. In order to detect transients in large numbers, near continuous observations of large patches of the sky are required. Based on the volume of space monitored and the measured SNe rate (from ground surveys) it is expected that at least 100 such events per year will be detected by ULTRASAT within less than a day of the explosion. The wide field of view and the advanced UV detectors will enable the discovery and monitoring of transient sources within a cosmic volume 300 times larger than that of the most powerful UV satellite to date, GALEX [7]). Analysis of the early light curve provides valuable information (stellar radius and surface chemical composition) on the progenitor star (before it exploded) that cannot be found by other means. In supernovae, an initial burst of high intensity in the UV is followed by radiation in longer wavelengths as the ejected material cools. UV can only be observed from space satellites, because of the blocking effect of the ozone; ground telescopes see only the later stages of the event. ULTRASAT has been designed to cover an unprecedentedly large field of view with a highly sensitive UV camera, with repeat image times as short as 5 minutes. To maximize the number of detected events, ULTRASAT will point to regions at high celestial latitudes, avoiding the Milky Way with its high concentration of "nearby" stars, diffuse background and galactic dust blocking much of the light from distant galaxies where these events occur.

Combined space-UV and ground-based optical observations triggered by a UV transient explorer would yield a wealth of data about massive star explosions, going beyond the stellar radius (and thus the stellar class of the progenitor: red or blue supergiant, or W-R star).

In addition to detecting early supernovae, ULTRASAT will measure UV light from the large number of stars in its field of view at high temporal resolution, possibly enabling the detection of planetary transits.[8] [9]

Other astrophysical sources yielding a transient UV signal are:

Gamma-ray burst afterglows (GRB). A wide field UV transient explorer may find the much sought after “orphan” afterglows.
The signal from a tidal disruption event is expected to peak in the UV.
The mass and environments of massive black holes in the centers of galaxies.
Detection of the electromagnetic counterpart of a gravity wave of a high-energy neutrino event would be highly significant.

References

  1. ↑ Israel Space Agency, “ULTRASAT project”
  2. ↑ Barstow, M., 2004 "Does ultraviolet astronomy have a future?", Astronomy and Geophysics Oct 2004
  3. ↑ Gezari et al, 2013,"The GALEX Time Domain Survey", The Astrophysical Journal, Volume 766, Issue 1, article id. 60
  4. ↑ Arcavi et al, 2014, "A Continuum of H- to He-rich Tidal Disruption Candidates With a Preference for E+A Galaxies", The Astrophysical Journal, Volume 793, Issue 1, article id. 38
  5. ↑ Welsh et al, 2005, The Astronomical Journal 130 825 doi:10.1086/431222
  6. ↑ Ganot et al, 2015, “The detection rate of early UV emission from supernovae: A dedicated GALEX/PTF survey and calibrated theoretical estimates”
  7. ↑ Martin et al, 2005, “The Galaxy Evolution Explorer: A Space Ultraviolet Survey Mission”, The Astrophysical Journal, Volume 619, Issue 1, pp. L1-L6
  8. ↑ Gottesman et al, 2012, "Exoplanets detection in the UV: ULTRASAT - The first Israeli space research mission", Israel Physical Society Conference 2012
  9. ↑ Ofir et al, 2015, "Finding unique exoplanets with ULTRASAT", International Astronautical Congress 2015, Session B4.2.3

Further reading

Sagiv et al, October 2015, "ULTRASAT - the Ultraviolet Transient Astronomy Satellite" IAC 2015, Session B4.2.2

Sagiv et al, April 2014, “Science with a wide-field UV transient explorer”, Astronomical Journal, Vol. 147:79

Soumagnac et al, October 2015, "A survey of eclipsing binaries with the Ultraviolet Transient Astronomy Satellite (ULTRASAT)", IAC 2015, Session A7.2.1

Mahabal et al, March 2008, “Automated probabilistic classification of transients and variables”, Astronomische Nachrichten, Volume 329, Issue 3

Lecture by Prof. Carolin Crawford, 2014, “The Transient Universe”

www.weizmann.ac.il/astrophysics/ultrasat

Wikipedia/ULTRASAT (in Hebrew)

This article is issued from Wikipedia - version of the Saturday, October 24, 2015. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.