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The space probes Pioneer 10, Pioneer 11, Voyager 1 and Voyager 2 are the-man made material that escaped from our solar system.

The main problem they face is the lack of power source in them.

So they are not able to contact Earth correctly....

Is there any way to find or track these probes with any of the newest technologies?

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3 Answers 3

up vote 16 down vote accepted

Voyagers are still active, and albeit they don't have the power required to run all the scientific equipment onboard and some of it stopped working by now, they still transmit telemetry data streams towards the Earth that is picked up by NASA JPL's 70-meter antenna at Goldstone, California, part of the Deep Space Network. Quoting from Wikipedia on Voyager program:

The two Voyager spacecraft continue to operate, with some loss in subsystem redundancy, but retain the capability of returning scientific data from a full complement of Voyager Interstellar Mission (VIM) science instruments.

Both spacecraft also have adequate electrical power and attitude control propellant to continue operating until around 2025, after which there may not be available electrical power to support science instrument operation. At that time, science data return and spacecraft operations will cease.

Pioneer probes are however not transmitting anything any more. Well, they might be but their signal is too weak at the distance to the Earth they are at (currently, Pioneer 10 is roughly 110 AU, and Pioneer 11 roughly 89 AU away) and due to deterioration of the thermocouple junctions in their RTGs, they don't generate enough power required to operate their transceivers and their signals being picked up by even the most powerful radio antennas. According to NASA, Pioneer 10's last, very weak signal was received on Jan. 22, 2003, and the last time a Pioneer 10 contact returned telemetry data was April 27, 2002. For Pioneer 11, NASA assessed that its transmitter will fall silent altogether some time in late 1996 and in September 29, 1995 announced they're ending Pioneer 11 operations.

Before Pioneer probes went completely silent on us, SETI used to use Pioneer 10 as a test target during their Phoenix Project, serving as a good approximation target for an ETI signal. Problem with detecting Pioneer probes now is their distance and the power of their transmissions, if they still transmit at all (likely not, and their RTG thermocouple junctions deteriorated beyond supplying required power to transmit anything by now). So even moving much closer to the probes and listening in likely wouldn't result in success.

For example, for omnidirectional transmissions at 120 AU, the required transmission power is 1.6 kW using EIRP isotropic antennas, defining detection range of a 305 meter diameter circular aperture receiver antenna, similar to the Arecibo radio telescope. Pioneer probes of course used directional 2.74 meter diameter parabolic dish high-gain transceiver antennas, so the total power required would be much smaller, but their 8 W output simply wouldn't be enough for the very faint signals not to be lost in the background noise.

Direct optical imaging would of course also be impossible from Earth or its vicinity, with Hubble Space Telescope (HST) resolving Pluto at roughly 16 x 16 pixels, and all these probes are far more distant to us than Pluto is, and of course, Pluto is a dwarf planet, that's orders of magnitude larger imaging target.

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suppose an antena or receiver from nearest place, that may be from nearest planet towards the probe can able to access the week signal from it. am i right. –  ReNiSh A R Feb 4 at 9:30
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No, I don't think so. Because of the deterioration of the thermocouple junctions in Pioneer RTGs, they likely don't generate enough power (for Pioneer 10, by 2005 the total power output was only 65 W) required for their 8 W transceivers. According to Wiki: "The final, very weak signal from Pioneer 10 was received on January 23, 2003 when it was 12 billion kilometers (80 AU) from Earth." –  TildalWave Feb 4 at 9:46
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Nothing I've read about the Pioneers suggests that they could still be found after their radio transmitters failed. I'd be very interested to see more information on this. –  Hobbes Feb 4 at 10:26
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@Hobbes I rewrote the part regarding detection of radioisotope decay at such distances. I'm not in possession of mentioned Stargazing Live episodes and sleeping on it find it extremely unlikely such feat would be possible and signature not lost in the background noise. Since it's entirely possible I just remember what was mentioned there wrong and my memory went haywire, I think it's better to not base any conclusions on that and give someone false impressions. If I'll watch reruns of that episode at a later date, I'll update the answer. ;) –  TildalWave Feb 5 at 10:21
    
I've just finished watching all of the most recent season of Stargazing Live, no mention of tracking the Pioneers or Voyagers. Was this in an earlier season? –  Hobbes Feb 9 at 20:04

We currently cannot track Pioneer 10 or 11.

Someone on the XKCD forum calculated how much radiation the Voyager probes emit besides their radio transmissions. The heat they give off is emitted as infrared light:

We have a power source of 420 W at 1.78×10¹⁰ km, which gives a brightness of 1×10⁻¹⁹ Wm⁻², or an apparent magnitude of 28. That is just visible for a big ground-based telescope....

Note that the radiation we're talking about would be in the infrared frequencies, not visible light. Still, an apparent magnitude of 30 is about the limit for the biggest ground-based IR telescopes.

But this discounts the angular resolution of a telescope. The Pioneers and Voyagers are much too small to be resolved. For example, here's a Hubble image of Pluto and its moons. Pluto is only a few pixels across:
Hubble image of Pluto and its moons

So a space probe at that distance would fill only a fraction of a pixel. Here's a Spitzer IR image of a dwarf planet:
Spitzer image of a dwarf planet
I suspect a space probe would be lost in the noise.

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"Current" positional data:

Voyager 1 Spacecraft, ephemeris for Fri 7 February 2014, 02:13 UTC Right Ascension: 17h 11m 54s Declination: +12° 01’ 12” (J2000) [HMS|00:00:00|Dec] Distance from Sun: 18,968.76 Million Km Distance from Earth: 19,024.36 Million Km Magnitude: N.A. Constellation: Oph

Voyager 2 Spacecraft, ephemeris for Fri 7 February 2014, 02:13 UTC Right Ascension: 20h 00m 03s Declination: -55° 56’ 58” (J2000) [HMS|00:00:00|Dec] Distance from Sun: 15,555.76 Million Km Distance from Earth: 15,662.57 Million Km Magnitude: N.A. Constellation: Tel

Pioneer 11 Spacecraft, ephemeris for Fri 7 February 2014, 02:13 UTC Right Ascension: 18h 49m 45s Declination: -08° 48’ 07” (J2000) [HMS|00:00:00|Dec] Distance from Sun: 13,202.88 Million Km Distance from Earth: 13,319.30 Million Km Magnitude: N.A. Constellation: Sct

Given that they are (1) powered by radio-thermal generators, (2) therefore above background temperature, and (3) on known trajectories, they are pretty easy to track. An orbital infrared telescope should be able to find them pretty easily. They are a small warm object on a known course.

References

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