Pluto's New Moon and Potential Collision Risks for New Horizons Probe

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SUMMARY

The New Horizons probe faces minimal collision risks during its flyby of Pluto, with a calculated probability of about 1 in 10 million for hitting small objects, primarily due to the vast distances involved and the limitations of real-time communication. The spacecraft operates using a radioisotope thermoelectric generator (RTG) with a power loss of approximately 0.8% annually, which restricts its ability to capture images of distant Kuiper Belt objects. Observations with the Long-Range Reconnaissance Imager (LORRI) and Ralph instruments will commence six months prior to closest approach, achieving better resolution than the Hubble Space Telescope 70 days before the flyby. Concerns regarding a potential ring system around Pluto are dismissed, as the planet's atmosphere would exceed the Roche limit, making ring formation unlikely.

PREREQUISITES
  • Understanding of spacecraft propulsion and trajectory adjustments
  • Familiarity with radioisotope thermoelectric generators (RTGs)
  • Knowledge of astronomical imaging techniques, specifically LORRI and Ralph instruments
  • Basic concepts of celestial mechanics, including Roche limits
NEXT STEPS
  • Research the capabilities and limitations of radioisotope thermoelectric generators (RTGs)
  • Explore the imaging capabilities of the Long-Range Reconnaissance Imager (LORRI) and Ralph instruments
  • Study the dynamics of small celestial bodies in the Kuiper Belt
  • Investigate the implications of Roche limits on planetary ring formation
USEFUL FOR

Astronomers, aerospace engineers, and space mission planners will benefit from this discussion, particularly those involved in deep space exploration and the study of celestial mechanics.

jarroe
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Is there any chance the New Horizons probe could collide with an unseen or unknown object while making its flyby? I would assume the odds are astronmical, but if such a small body such as pluto has 5 moons, smaller icy bodies might be more frequent/common than we expected? Does anyone know if they can adjust the trajectory of the probe in time if needed?
 
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The possibility always exist with anything in spaceflight. We have virtually no chance of turning the probe in time, as real time communication is impossible due to the vast distance from Earth the probe has reached. We would have to see it coming several days out at least most likely.
 
Objects with a size of ~1mm to 10cm are the most dangerous objects, as they are much more frequent than moons. And we have no way to detect them in this distance.

The small pluto moons have an objectradius/orbitalradius ratio of ~1/3000. The relative area is this number squared. Therefore, a random flight through the system has a probability of about 1 in 10 million to hit them (depends a bit on the parameters). This is negligible compared to all the other risks in space missions.
 
Thanks for the good info. I guess at the speed its moving an object the size of a dime could cripple the mission. Cant imagine the dissapointment for the team if it fails after such a long wait.

Wondering why they don't try to capture some images further out right now or even next year? Must be able to get a better picture than Hubble by now? I know Kuiper belt objects are in the future, perhaps energy must be conserved and energy limits this option? Annual power loss of 0.8%. Couldn't it snap some pics now? Perhaps the resolution wouldn't be enough to accomplish anything yet? Thoughts?

The spacecraft electrical power source is a
radioisotope thermoelectric generator (RTG) with a design baseline of 10.9 kilograms of plutonium-238 dioxide,
housed in 18 general purpose heat source (GPHS) modules3, Fig. 4. The nuclear fuel provides a source thermal
energy that is converted to electrical power using silicon-germanium thermoelectric devices (solid state unicouples).
The efficiency for a GPHS style RTG is 6.4%5 and has an annual power loss of approximately 0.8% due to the
radioactive decay of the isotope fuel6.
 
It is currently about 1 billion km away from Pluto, while Hubble is ~6 billion km away. At this distance ratio, Hubble is better, and there are already a lot of low-resolution images.

According to Wikipedia:
Observations of Pluto, with LORRI plus Ralph, will begin about 6 months prior to closest approach. The targets will be only a few pixels across. 70 days out, resolution will exceed the Hubble Space Telescope's resolution,http://pluto.jhuapl.edu/mission/mission_timeline.php lasting another two weeks after the flyby.
 
Last edited by a moderator:
Thanks for the info. I figured if they had the resolution now, they would've tried it already, but now I know the rest of the story. Thanks again!
 
They might want to avoid all the Lagrangian spots in the Pluto system too.

Don't think a ring system around Pluto would be much of a possibility, I suspect the height of the atmosphere (despite it's low density) would exceed the Roche limit for rings, and any atmosphere at all over the age of the solar system would collapse a ring a very long time ago.
 

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