Skip to main content
Log in

Long-Range Reconnaissance Imager on New Horizons

  • Published:
Space Science Reviews Aims and scope Submit manuscript

Abstract

The LOng-Range Reconnaissance Imager (LORRI) is the high-resolution imaging instrument for the New Horizons mission to Pluto, its giant satellite Charon, its small moons Nix and Hydra, and the Kuiper Belt, which is the vast region of icy bodies extending roughly from Neptune’s orbit out to 50 astronomical units (AU). New Horizons launched on January 19, 2006, as the inaugural mission in NASA’s New Frontiers program. LORRI is a narrow-angle (field of view=0.29°), high-resolution (4.95 μrad pixels), Ritchey-Chrétien telescope with a 20.8-cm diameter primary mirror, a focal length of 263 cm, and a three-lens, field-flattening assembly. A 1,024×1,024 pixel (optically active region), thinned, backside-illuminated charge-coupled device (CCD) detector is used in the focal plane unit and is operated in frame-transfer mode. LORRI provides panchromatic imaging over a bandpass that extends approximately from 350 nm to 850 nm. LORRI operates in an extreme thermal environment, situated inside the warm spacecraft with a large, open aperture viewing cold space. LORRI has a silicon carbide optical system, designed to maintain focus over the operating temperature range without a focus adjustment mechanism. Moreover, the spacecraft is thruster-stabilized without reaction wheels, placing stringent limits on the available exposure time and the optical throughput needed to satisfy the measurement requirements.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Subscribe and save

Springer+ Basic
EUR 32.99 /Month
  • Get 10 units per month
  • Download Article/Chapter or Ebook
  • 1 Unit = 1 Article or 1 Chapter
  • Cancel anytime
Subscribe now

Buy Now

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  • A.F. Cheng, L.A. Young, EOS Trans. AGU, 83, 384, 389 (2002).

    Google Scholar 

  • S. Conard, F. Azad, J. Boldt, A. Cheng, K. Cooper, E. Darlington, M. Grey, J. Hayes, P. Hogue, K. Kosakowski, T. Magee, M. Morgan, E. Rossano, D. Sampath, C. Schlemm, H. Weaver, in Astrobiology and Planetary Missions, ed. by G.R. Gladstone. Proc. SPIE 5906, 2005.

  • K. Horne, star-www.stand.ac.uk/kdh1/pub0/ada/woe/woe.ps, University of St. Andrews, 2004.

  • R.L. McNutt et al., Space Sci. Rev. (2007, this issue)

  • F. Morgan, S.J. Conard, H.A. Weaver, O. Barnouin-Jha, A.F. Cheng, H.W. Taylor, K.A. Cooper, R.H. Barkhouser, R. Boucarut, E.H. Darlington, M.P. Grey, I. Kuznetsov, T.J. Madison, M.A. Quijada, D.J. Sahnow, J.M. Stock, in Astrobiology and Planetary Missions, ed. by G.R. Gladstone. Proc. SPIE 5906, 2005.

  • D. Reuter et al., Space Sci. Rev. (2007, this issue)

  • H.A. Weaver, S.A. Stern, M. Mutchler, A. Steffl, M. Buie, W. Merline, J. Spencer, E. Young, L. Young, Discovery of two new satellites of Pluto. Nature 439, 943–946 (2006)

    Article  ADS  Google Scholar 

  • H.A. Weaver et al., Space Sci. Rev. (2007, this issue)

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to A. F. Cheng.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Cheng, A.F., Weaver, H.A., Conard, S.J. et al. Long-Range Reconnaissance Imager on New Horizons. Space Sci Rev 140, 189–215 (2008). https://doi.org/10.1007/s11214-007-9271-6

Download citation

  • Received:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s11214-007-9271-6

Keywords

Navigation