REX (New Horizons)

Diagram of the trajectory of New Horizons, which enables the REX experiment to utilize the occultation of Pluto between the spacecraft and Earth to determine atmospheric data Part of the radio network on Earth, a 70 m antenna at Goldstone, California . REX picks up the signal from Earth during the flyby to record some types of data about the Plutonian system.

REX or Radio Science Experiment is an experiment on the New Horizons space probe to determine various aspects of the atmosphere of Pluto during the 2015 flyby.[1]

## Contents

* 1 Experiment
* 2 Extended mission
* 3 Data from REX
* 4 See also
* 5 References
* 6 External links

## Experiment

Experiment was designed with several goals including determination of pressure and temperature of Plutonian atmosphere, measurements of a possible ionosphere of Pluto and Charon, recording thermal emission temperatures, and taking more accurate chord lengths of Charon and Pluto.

To accomplish the goals, as the spacecraft passed by Pluto, it was targeted on a path that took it behind the dwarf planet in relation to where Earth is, and at that time radio signals from the flyby spacecraft passed through atmosphere of body, and from this various aspects could be determined.[1] REX also is designed to take measurements of the atmospheric conditions at Pluto's moon Charon as part of the mission.[2] REX utilizes an ultrastable oscillator, various electronics, and radio hardware aboard the New Horizons spacecraft.[3] REX utilizes the X-band radio uplink on the spacecraft.[4]

REX hardware weights 160 g (0.16 kg) and consumes 1.6 watts of spacecraft electrical power.[1] It also makes use of other NH hardware, overall key hardware components for REX include:[4]

* high-gain antenna
* low-noise X-band receiver
* ultrastable oscillator

To take the measurements, REX communicates with the Deep Space Network on Earth.[2]

Observation goals:[4]

* temperature profiles of Pluto's atmosphere
* pressure profiles of Pluto's atmosphere
* radiometric temperature
* gravitational moments
* ionosphere structure

## Extended mission

REX is also planned for use in the New Horizon's post Pluto extended mission, including the 486958 Arrokoth flyby.[5] REX will be used to take thermal measurements of the Kuiper belt body during the planned flyby.[5] REX is also used to study the amount of electrons in outer space in the Kuiper belt region.[5] The Kuiper belt is a ring of orbiting bodies between approximately 30 to 55 AU (Earth-Sun distances), home to Pluto and short-period comets it is estimated to consist of hundreds of thousand if not millions of small icy objects.[6] The belt was discovered starting in 1992, and can be studied more closely by the New Horizons mission which is passing through it starting in the late 2010s.[7]

During the post Pluto cruise, REX is usually turned on monthly to measure the electron density of the solar wind between Earth and the spacecraft.[8] When New Horizons flew by Pluto in 2015, it was at about 32.9 AU from the Sun, and about 43.6 AU for the New Year's Day 2019 flyby of Arrokoth.[9][10]

The timing of the Arrokoth flyby was adjusted in part to aid the use of the REX experiment, in particular time it so more radar dishes on Earth could be used for this experiment.[11]

## Data from REX

Using REX radio occultation data the diameter of Pluto was found to be 2376.6±3.2 km in a 2017 paper.[12]

## See also

* Gravity science (Juno) (Experiment aboard Juno Jupiter orbiter that uses radio and time)
* Mariner 4 (radio experiment helped determine more accurate atmospheric conditions about Mars in the 1960s)

## References

1. ↑ 1.0 1.1 1.2 Tyler, G. L.; Linscott, I. R.; Bird, M. K.; Hinson, D. P.; Strobel, D. F.; Pätzold, M.; Summers, M. E.; Sivaramakrishnan, K. (2008-02-21). "The New Horizons Radio Science Experiment (REX)" (in en). Space Science Reviews 140 (1–4): 217–259. doi:10.1007/s11214-007-9302-3. ISSN 0038-6308. Bibcode: 2008SSRv..140..217T. http://www.boulder.swri.edu/pkb/ssr/ssr-rex.pdf.
2. ↑ 2.0 2.1 Linscott, I.; Hinson, D. P.; Bird, M. K.; Stern, A.; Weaver, H. A.; Olkin, C.; Young, L. A.; Ennico Smith, K. (2015). "The New Horizons Radio Science Experiment: Performance and Measurements of Pluto's Atmospheric Structure, Surface Pressure, and Surface Temperature". AGU Fall Meeting Abstracts 2015: P54A–05. Bibcode: 2015AGUFM.P54A..05L.
3. ↑ DeBoy, C. C.; Haskins, C. B.; Brown, T. A.; Schluze, R. C.; Bernacik, M. A.; Jensen, J. R.; Millard, W.; Duven, D. et al. (March 2004). "The RF telecommunications system for the New Horizons mission to Pluto". IEEE Aerospace Conference. doi:10.1109/AERO.2004.1367922.
4. ↑ 4.0 4.1 4.2 Linscott, I. R.; Bird, M. K.; Hinson, D. P.; Pätzold, M.; Tyler, G. L. (2011). "The Radioscience Experiment on New Horizons" (in en-US). IEEE Conference. doi:10.1109/URSIGASS.2011.6051216.
5. ↑ 5.0 5.1 5.2 Stern, S. A.; Weaver, H. A.; Spencer, J. R.; Elliott, H. A.; the New Horizons Team (2018). "The New Horizons Kuiper Belt Extended Mission". Space Science Reviews 214 (4): 77. doi:10.1007/s11214-018-0507-4. Bibcode: 2018SSRv..214...77S.
6. ↑ "Kuiper Belt". Solar System Exploration: NASA Science. https://solarsystem.nasa.gov/solar-system/kuiper-belt/overview/.
7. ↑ "The PI's Perspective: Why Didn't Voyager Explore the Kuiper Belt? – Pluto New Horizons" (in en-US). 28 February 2018. https://blogs.nasa.gov/pluto/2018/02/28/the-pis-perspective-why-didnt-voyager-explore-the-kuiper-belt/.
8. ↑ "Kuiper Belt". https://solarsystem.nasa.gov/solar-system/kuiper-belt/overview/.
9. ↑ Bagenal, F.; Delamere, P. A.; Elliott, H. A.; Hill, M. E.; Lisse, C. M.; McComas, D. J.; McNutt Jr, R. L.; Richardson, J. D. et al. (2015). "Solar wind at 33 AU: Setting bounds on the Pluto interaction for New Horizons". Journal of Geophysical Research: Planets 120 (9): 1497–1511. doi:10.1002/2015JE004880. Bibcode: 2015JGRE..120.1497B.
10. ↑ "New Horizons" (in en). http://pluto.jhuapl.edu/Mission/Where-is-New-Horizons/index.php.
11. ↑ "New Horizons prepares for encounter with 2014 MU69" (in en). http://www.planetary.org/blogs/emily-lakdawalla/2018/0124-new-horizons-prepares-for-2014mu69.html.
12. ↑ Nimmo, Francis (2017). "Mean radius and shape of Pluto and Charon from New Horizons images". Icarus 287: 12–29. doi:10.1016/j.icarus.2016.06.027. Bibcode: 2017Icar..287...12N.

## External links

* NASA - REX

* v
* t
* e

New Horizons

* Exploration of Pluto
* List of New Horizons topics
* New Frontiers program

Targets|

| Flybys|

* 132524 APL
* Jupiter
* Pluto
* 486958 Arrokoth

|

Observations|

* Neptune
* 2011 KW48
* 15810 Arawn
* 50000 Quaoar

Rejected|

* 2011 HM102
* 2014 MT69
* 2014 OS393
* 2014 PN70

Spacecraft|

| Instruments|

* Alice
* Long Range Reconnaissance Imager
* PEPSSI
* Ralph
* REX
* Venetia Burney Student Dust Counter
* SWAP

|

Subsystems|

* GPHS-RTG

Personnel|

| Institutions|

* Applied Physics Laboratory
* Ball Aerospace
* Goddard Space Flight Center
* Jet Propulsion Laboratory
* KinetX
* Southwest Research Institute
* Stanford University
* University of Colorado

|

People|

* Frances Bagenal
* Richard Binzel
* Alice Bowman
* Marc Buie
* Lisa Hardaway
* Brian May
* Cathy Olkin
* Daniel Sarokon
* Mark Showalter
* Alan Stern
* Hal Weaver

Logistics|

* Atlas V (launch vehicle)
* Centaur (upper stage)
* Star 48B (3rd stage)
* Cape Canaveral Air Force Station Space Launch Complex 41 (launch site)
* Deep Space Network

Related|

* Hubble Space Telescope
* Kuiper belt
* New Horizons 2
* Pluto Kuiper Express

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