[HN Gopher] First Hubble telescope images of interstellar comet ...
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       First Hubble telescope images of interstellar comet 3I/ATLAS
        
       Author : jandrewrogers
       Score  : 76 points
       Date   : 2025-07-22 16:41 UTC (6 hours ago)
        
 (HTM) web link (bsky.app)
 (TXT) w3m dump (bsky.app)
        
       | hooo wrote:
       | While it would be cool if it were alien technology[1], it looks
       | like an ancient comet?
       | 
       | [1]: https://avi-loeb.medium.com/is-the-interstellar-
       | object-3i-at...
        
         | csours wrote:
         | Oh dear, he's already at it with this one too
        
           | meepmorp wrote:
           | It'd be more surprising if he wasn't, tbh.
        
         | mcswell wrote:
         | Agreed, it would be cool, but. From that article, with my
         | commentary (disclaimer: IANAA, I Am Not An Astronomer):
         | 
         | 1) "The retrograde orbital plane... of 3I/ATLAS around the Sun
         | lies within 5 degrees of that of Earth... The likelihood for
         | that coincidence out of all random orientations is 0.2%." Not
         | sure where he comes up with 0.2%. 5/180 = 2.8%. (I use 180
         | degrees, rather than 360, because I suspect that if it were not
         | retrograde, he'd use the same argument.)
         | 
         | 2) "the brightness of 3I/ATLAS implies an object that is ~20
         | kilometers in diameter (for a typical albedo of ~5%), too large
         | for an interstellar asteroid. We should have detected a million
         | objects below the ~100-meters scale of the first reported
         | interstellar object 1I/`Oumuamua for each ~20-kilometer
         | object." Huh? We barely detected this object because it's so
         | dim. Why should we be detecting interstellar objects two or
         | three orders of magnitude smaller?
         | 
         | 3) "No spectral features of cometary gas are found in
         | spectroscopic observations of 3I/ATLAS." An article today (22
         | July, https://astrobiology.com/2025/07/spectroscopic-
         | characterizat...) says "Spectral modeling with an areal mixture
         | of 70% Tagish Lake meteorite and 30% 10-micron-sized water ice
         | successfully reproduces both the overall continuum and the
         | broad absorption feature... 3I/ATLAS is an active interstellar
         | comet containing abundant water ice, with a dust composition
         | more similar to D-type asteroids..."
         | 
         | 4. "For its orbital parameters, 3I/ATLAS is synchronized to
         | approach unusually close to Venus (0.65au where 1au is the
         | Earth-Sun separation), Mars (0.19au) and Jupiter (0.36au), with
         | a cumulative probability of 0.005% relative to orbits with the
         | same orbital parameters but a random arrival time." This
         | probability is harder to compute (although 0.65au from Venus is
         | nearly the radius of Venus' orbit, 0.72au, i.e. not close). In
         | any case, so what? Why would an interstellar probe travel close
         | to Mars or Jupiter, if they're interested in Earth? (see next
         | point) Later (his point 8), he says the probe comes close
         | enough to these planets to launch ICBMs at them. Ok...
         | 
         | 5. "3I/ATLAS achieves perihelion on the opposite side of the
         | Sun relative to Earth. This could be intentional..." Sure, if
         | they're interested in Earth, stay away from it.
         | 
         | And similarly for the rest of his points.
        
           | teraflop wrote:
           | > "The retrograde orbital plane... of 3I/ATLAS around the Sun
           | lies within 5 degrees of that of Earth... The likelihood for
           | that coincidence out of all random orientations is 0.2%." Not
           | sure where he comes up with 0.2%.
           | 
           | This part of the calculation, at least, is basically correct.
           | The orientation of a plane in space is defined by its normal
           | vector, so the right way to look at probabilities is in terms
           | of solid angle. The normal of 3I/ATLAS's orbit falls within a
           | cone around Earth's normal vector, having a half-angle of 5
           | degrees, and that cone's solid angle occupies about 0.2% of
           | the full sphere.
           | 
           | Of course, this is only the chance of a retrograde alignment.
           | Presumably, if the comet's orbit was _prograde_ aligned with
           | the Earth 's to within 5 degrees, Loeb would be making
           | exactly the same claim. So really, the relevant probability
           | is 0.4%.
           | 
           | Nevertheless, I agree that the article is basically just a
           | bunch of cherry-picked probabilities and insinuations that
           | don't add up to much.
           | 
           | Also:
           | 
           | > "the brightness of 3I/ATLAS implies an object that is ~20
           | kilometers in diameter (for a typical albedo of ~5%), too
           | large for an interstellar asteroid."
           | 
           | But to justify this, Loeb cites his own work showing that the
           | object is _either_ a large asteroid, _or_ a comet with a
           | small nucleus. And then he seems to have looked at some
           | earlier spectra and jumped to the conclusion that 3I /ATLAS
           | couldn't be a comet, so it must be a large asteroid. But of
           | course, follow-up observations have debunked this point and
           | clearly shown it to be a comet.
        
         | imafish wrote:
         | Why would it be cool, though? More like frightening, if the
         | thing was sent on purpose by another civilization.
        
       | dylan604 wrote:
       | 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?
        
         | pinko wrote:
         | 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.
        
         | teraflop wrote:
         | 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...
        
       | rkagerer wrote:
       | Dumb question: Is it the smaller one (that moves, along the same
       | axis as the background stars) or the bigger one (that's fairly
       | static). What's the other one?
        
         | exitb wrote:
         | The static lines are motion blurred stars (even the bright
         | one), the small dots are radiation noise, the one that moves,
         | with a coma is the comet.
        
         | mcswell wrote:
         | About the bigger one that doesn't seem to move: I think it does
         | move, it's just that it's so bright (for Hubble) that its
         | brightness overwhelms the slight elongation of its image. In
         | other words, it's (apparently) moving just like the other
         | stars, it's just hard to tell.
        
       | throw0101b wrote:
       | A lot of motion blur: have they tried adjusting the shutter
       | speed...
        
         | pinko wrote:
         | At ~100s, it's already at about the minimum for Hubble; often
         | it's 1-2 orders of magnitude longer.
        
         | mcswell wrote:
         | If I know what you're referring to, the motion blur is the
         | stars, not the comet. That's because Hubble is tracking
         | (pointing at) the comet, not the stars. The comet is therefore
         | not blurred in its direction of travel, while the stars appear
         | to be moving in the direction opposite of the comet's travel.
         | To the extent that the comet appears blurred, that's presumably
         | its coma.
        
       | amrrs wrote:
       | Noob Q: How do they know it's an interstellar comet? With the
       | speed of movement between two frames?
        
         | baggy_trough wrote:
         | This object was already discovered and known to have an
         | hyperbolic (uncaptured) orbit.
        
         | vikingerik wrote:
         | Short answer, yes. But it's many frames, and over a time span
         | of many nights and now weeks.
        
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       (page generated 2025-07-22 23:00 UTC)