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The slew rate for tracking comets is something that I have not had to mess with before, but I adjust my little EQ mount when I'm tracking the moon vs deep sky objects. How accurate is Hubble now? How many of its reaction wheels does it have left? I seem to remember it being down to just one at one point. Does that add difficulty in tracking this object with its very high velocity?


I'm no Hubble expert, but a bit of research turned up the "HST Primer" [1] which is apparently up-to-date for the current observing cycle, and which says:

> HST is capable of tracking moving targets with the same precision achieved for fixed targets. This is accomplished by maintaining FGS Fine Lock on guide stars and driving the FGS star sensors in the appropriate path, thus moving the telescope to track the target. Tracking under FGS control is technically possible for apparent target motions up to 5 arcsec/s.

According to JPL Horizons, the current angular motion of 3I/ATLAS across the sky is <0.03 arcsec/s, so it's well within Hubble's capabilities.

My understanding is that the Hubble's one-gyro mode mainly complicates the process of quickly moving from one target to another. Once the telescope is pointed at a target, the stabilization and tracking is done using guide stars without relying on gyros.

Anyway, in absolute terms, 3I/ATLAS isn't moving that fast. Its orbital speed is about 3x that of Mars, but it's farther away, and (for now) much of that motion is directed inward towards the sun.

[1]: https://hst-docs.stsci.edu/hsp/the-hubble-space-telescope-pr...


You're on the money. Hubble isn't too perturbed when it can lock on to guide stars, but some observations are no longer possible in one-gyro mode.


Hubble's slew rate (the rate at which it can change the broad direction its camera points) is about 6 degrees per minute [1], or about 1/10 of a degree per second (I refuse to use the incredibly cursed unit "minutes per second"). It tracks a fine object slower than that, but that gives a reasonable order-of-magnitude estimate.

At even 1 AU of distance, an angular velocity of 1/10 of a degree per second requires a linear speed of about 0.87c. Needless to say, 3I/ATLAS is not moving that fast - if it were, it would be outputting about 100 TW, mostly as heat, just from slamming into the interplanetary medium at relativistic speeds [2].

[1] https://www.pbs.org/deepspace/hubble/diagram.html#:~:text=Th...

[2] https://www.wolframalpha.com/input?i=%2840+*+mass+of+hydroge...


> I refuse to use the incredibly cursed unit "minutes per second"

Man, that is a horrible unit. I've never heard of that, but I can only imagine each semester professors every where have to endure an enterprising student using this to be "clever" in some way


“Arcminutes per second” would be the standard way to express it in astronomy.


FWIW, isn't it only "minutes" if you want to be confusingly short? I'd have said "minutes of arc" or "arcminutes".


I suspect, at ~4.5AU distance, even though 3I/ATLAS is moving at a relative speed of ~60 kms, its angular velocity across the sky is manageable for Hubble's current one-gyro pointing system, given non‑sidereal tracking and short (~100s) exposures.




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