<p>The hypothesis that the object has an extreme aspect ratio comes from both the max/min ratio of the light curve <em>and the shape</em> of the light curve, along with some assumptions of the uniformity of the albedo as you mentioned.</p>

<p>If you read the BBC article <a href="http://www.bbc.com/news/science-environment-42053634" rel="noreferrer">Bizarre shape of interstellar asteroid</a> and click from that page on the link that says <strong>which is published in Nature journal.</strong> it will take you to an open access draft of the Nature Letter. In it you can see the shape of the light curve. I've chopped up some sections to show below. </p>

<p>The "dip" is quite sharp. Remember magnitudes are a log scale, and so the dip would be even sharper on a linear scale. Since 5 magnitudes are a factor of ~100, a 2.5 magnitude dip is a factor of ~10.</p>

<p>This is what you would get when a high-aspect ratio objects so that is viewed end-on. A black spot would darken the curve much more gradually, being viewed for a longer fraction of the cycle.</p>

<p>This is not proof of the high-aspect ratio hypothesis, and the authors don't claim this. However, it's the best way to fit the curve with the fewest assumptions, as far as I can tell.</p>

<hr>

<p>Screen shot of the on-line Accelerated Preview of the Nature Letter <a href="https://www.nature.com/articles/nature25020" rel="noreferrer">A brief visit from a red and extremely elongated interstellar asteroid</a> K. Meech et al. doi:10.1038/nature25020</p>

<p><a href="https://i.sstatic.net/3pi00.png" rel="noreferrer"><img src="https://i.sstatic.net/3pi00.png" alt="enter image description here"></a></p>

<p><a href="https://i.sstatic.net/07FbZ.png" rel="noreferrer"><img src="https://i.sstatic.net/07FbZ.png" alt="enter image description here"></a></p>

<p><a href="https://i.sstatic.net/jKTpy.png" rel="noreferrer"><img src="https://i.sstatic.net/jKTpy.png" alt="enter image description here"></a></p>

<p><a href="https://i.sstatic.net/kPvAl.png" rel="noreferrer"><img src="https://i.sstatic.net/kPvAl.png" alt="enter image description here"></a></p>

CC BY-SA 3.0
2017-11-23T18:08:35.570Z
*... and the authors don't claim this* but they imply by the title of their Nature article. It's not even clear, whether this is the simplest explanation. Of course, a spherical body with albedo variation is ruled out, but small objects are typically never spherical. Btw. a 10:1:1 triaxial object is actually a 10:1 prolate object.
Walter
CC BY-SA 3.0
2017-11-21T12:26:11.533Z
2017-11-21T12:26:11.533Z
uhoh
<p>News articles have mentioned that the recently discovered asteroid <a href="https://www.nasa.gov/feature/solar-system-s-first-interstellar-visitor-dazzles-scientists" rel="noreferrer">'Oumuamua</a> is theorized to be greatly elongated based on observations of brightness variation. However, this hypothesis seems to be based on the assumption that the object's albedo distribution is reasonably uniform.
What if it isn't? Could large periodic brightness variations also be explained by 'Oomuamua having two highly contrasting hemispheres like <a href="https://en.wikipedia.org/wiki/Iapetus_(moon)" rel="noreferrer">Iapetus</a>? If the astronomers involved have already eliminated this competing explanation, how would they have done so and with what additional observational data?</p>

CC BY-SA 3.0
2017-11-21T07:32:27.683Z
We might soon be sure (2039), like explained here: https://space.stackexchange.com/a/23522/18615 , [project Lyra](https://arxiv.org/pdf/1711.03155.pdf) expecting to launch a light probe towards the thing.
J. Chomel
CC BY-SA 3.0
2017-11-21T12:27:00.167Z
@J.Chomel Yippie! I can't wait! :-)
uhoh
CC BY-SA 3.0
2017-11-22T09:53:11.757Z
As always [xkcd.com provides some guidance](https://xkcd.com/1919/).
StephenG - Help Ukraine
<asteroids>
Could asteroid 'Oumuamua actually be round?
user2127894
# Could asteroid 'Oumuamua actually be round?

(Asked by: username_0 on 2017-11-21)

News articles have mentioned that the recently discovered asteroid ['Oumuamua](https://www.nasa.gov/feature/solar-system-s-first-interstellar-visitor-dazzles-scientists) is theorized to be greatly elongated based on observations of brightness variation. However, this hypothesis seems to be based on the assumption that the object's albedo distribution is reasonably uniform.
What if it isn't? Could large periodic brightness variations also be explained by 'Oomuamua having two highly contrasting hemispheres like [Iapetus](https://en.wikipedia.org/wiki/Iapetus_(moon))? If the astronomers involved have already eliminated this competing explanation, how would they have done so and with what additional observational data?

**Tags:** asteroids

> **Comments:**
> **username_1**: We might soon be sure (2039), like explained here: https://space.stackexchange.com/a/23522/18615 , [project Lyra](https://arxiv.org/pdf/1711.03155.pdf) expecting to launch a light probe towards the thing.  
> **username_2**: @J.Chomel Yippie! I can't wait! :-)  
> **username_3**: As always [xkcd.com provides some guidance](https://xkcd.com/1919/).  

---

## 1 answers

### Answer by username_2 on 2017-11-21. Score: 10

The hypothesis that the object has an extreme aspect ratio comes from both the max/min ratio of the light curve *and the shape* of the light curve, along with some assumptions of the uniformity of the albedo as you mentioned.

If you read the BBC article [Bizarre shape of interstellar asteroid](http://www.bbc.com/news/science-environment-42053634) and click from that page on the link that says **which is published in Nature journal.** it will take you to an open access draft of the Nature Letter. In it you can see the shape of the light curve. I've chopped up some sections to show below.

The "dip" is quite sharp. Remember magnitudes are a log scale, and so the dip would be even sharper on a linear scale. Since 5 magnitudes are a factor of ~100, a 2.5 magnitude dip is a factor of ~10.

This is what you would get when a high-aspect ratio objects so that is viewed end-on. A black spot would darken the curve much more gradually, being viewed for a longer fraction of the cycle.

This is not proof of the high-aspect ratio hypothesis, and the authors don't claim this. However, it's the best way to fit the curve with the fewest assumptions, as far as I can tell.

---

Screen shot of the on-line Accelerated Preview of the Nature Letter [A brief visit from a red and extremely elongated interstellar asteroid](https://www.nature.com/articles/nature25020) K. Meech et al. doi:10.1038/nature25020

[![enter image description here](https://i.sstatic.net/3pi00.png)](https://i.sstatic.net/3pi00.png)

[![enter image description here](https://i.sstatic.net/07FbZ.png)](https://i.sstatic.net/07FbZ.png)

[![enter image description here](https://i.sstatic.net/jKTpy.png)](https://i.sstatic.net/jKTpy.png)

[![enter image description here](https://i.sstatic.net/kPvAl.png)](https://i.sstatic.net/kPvAl.png)

> **Comments:**
> **username_4**: *... and the authors don't claim this* but they imply by the title of their Nature article. It's not even clear, whether this is the simplest explanation. Of course, a spherical body with albedo variation is ruled out, but small objects are typically never spherical. Btw. a 10:1:1 triaxial object is actually a 10:1 prolate object.  

---

