<p>Five years have passed, and several papers have been published about this. The latest, <a href="https://doi.org/10.1016/j.icarus.2018.09.006" rel="nofollow noreferrer">Neesemann et al. (2019)</a>, compiles previous results and propose a new age estimate. Or rather estimates, because dating such object is tricky! It depends on which model you use (lunar-derived chronology model versus asteroid-derived chronology model, or ADM), and on which part of the crater you use the model on (ejecta blanket versus interior lobate deposits). Hence the large interval in the result: they found an age of <strong>1.6 to 63.7 Ma</strong> (ADM on ejecta blanket), which they translated to &quot;relatively young&quot;, geologically speaking.</p>

CC BY-SA 4.0
2020-11-19T10:01:07.877Z
Not sure why your answer wasn't selected as the answer, its reference is a lot more recent than the 2015 references in the other one, and it gives a synthesis of previous work.  Also, FWIW, the lunar cratering model is ridiculous to use within the asteroid belt itself, but I'm not going to fight that battle on StackExchange.
Stuart Robbins
CC BY-SA 4.0
2020-11-19T10:33:53.037Z
@StuartRobbins Well, the other answer was accepted five years ago, when it was the only answer—and it was an accurate answer at the time of writing! And SE does not allow to change once an answer is accepted.
Jean-Marie Prival
CC BY-SA 4.0
2020-11-19T16:19:50.397Z
Ha!  I was tired and didn't think to look at the date.  And apparently it does let you change things, since your answer is now accepted.
Stuart Robbins
CC BY-SA 4.0
2020-11-19T16:42:19.563Z
Yes, it looks like someone has changed the tick after all. Thanks!
Jean-Marie Prival
CC BY-SA 4.0
2020-11-19T09:53:06.263Z
2020-11-19T09:53:06.263Z
Jean-Marie Prival
<p><a href="https://gsa.confex.com/gsa/2015AM/webprogram/Paper260706.html" rel="nofollow">It seems</a> not yet.  <a href="https://gsa.confex.com/gsa/2015AM/webprogram/Paper260352.html" rel="nofollow">The non-uniform density of craters</a> seen on Ceres is still under investigation.  From the abstracts of those papers, they're still working on trying to date the ejecta material from that crater, and trying to understand the resurfacing that appears to be going on.</p>

CC BY-SA 3.0
2015-11-19T04:22:55.283Z
2015-11-19T04:22:55.283Z
Dave
<p>Has any official information been published regarding the estimated age of the Occator crater on Ceres?  I ran some quick searches but couldn't find anything putting a definitive (or even speculative) date on the moment of impact.</p>

<p>I ask because based upon my own very amateur analysis of the imagery:</p>

<p><a href="https://i.sstatic.net/Sd3Uu.jpg" rel="noreferrer"><img src="https://i.sstatic.net/Sd3Uu.jpg" alt="enter image description here"></a></p>

<p>...there seems to be a marked decrease in the amount of secondary cratering visible within a fairly uniform radius of the main crater.  </p>

<p>My assumption is that when the impact occurred, the surrounding area was likely blanketed by material kicked up from the impact site, obscuring most pre-existing craters (smaller ones, in particular).  Kind of like fresh snowfall, except made of rock.  </p>

<p>So for a (small) secondary crater to be visible near Occator, the impact would have to have occurred <em>after</em> the impact that created Occator crater.  Meaning that the relative lack of small craters near Occator would seem to imply a fairly recent impact ("recent" in terms of Ceres geological timescales), I believe?</p>

<p>Is there any official data that would confirm or refute this?</p>

<ceres><crater>
Age of Occator Crater
aroth
# Age of Occator Crater

(Asked by: username_0 on 2015-11-19)

Has any official information been published regarding the estimated age of the Occator crater on Ceres? I ran some quick searches but couldn't find anything putting a definitive (or even speculative) date on the moment of impact.

I ask because based upon my own very amateur analysis of the imagery:

[![enter image description here](https://i.sstatic.net/Sd3Uu.jpg)](https://i.sstatic.net/Sd3Uu.jpg)

...there seems to be a marked decrease in the amount of secondary cratering visible within a fairly uniform radius of the main crater.

My assumption is that when the impact occurred, the surrounding area was likely blanketed by material kicked up from the impact site, obscuring most pre-existing craters (smaller ones, in particular). Kind of like fresh snowfall, except made of rock.

So for a (small) secondary crater to be visible near Occator, the impact would have to have occurred *after* the impact that created Occator crater. Meaning that the relative lack of small craters near Occator would seem to imply a fairly recent impact ("recent" in terms of Ceres geological timescales), I believe?

Is there any official data that would confirm or refute this?

**Tags:** ceres, crater


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## 2 answers

### Answer by username_1 on 2020-11-19. Score: 4 | Accepted answer

Five years have passed, and several papers have been published about this. The latest, [Neesemann et al. (2019)](https://doi.org/10.1016/j.icarus.2018.09.006), compiles previous results and propose a new age estimate. Or rather estimates, because dating such object is tricky! It depends on which model you use (lunar-derived chronology model versus asteroid-derived chronology model, or ADM), and on which part of the crater you use the model on (ejecta blanket versus interior lobate deposits). Hence the large interval in the result: they found an age of **1.6 to 63.7 Ma** (ADM on ejecta blanket), which they translated to "relatively young", geologically speaking.

> **Comments:**
> **username_2**: Not sure why your answer wasn't selected as the answer, its reference is a lot more recent than the 2015 references in the other one, and it gives a synthesis of previous work.  Also, FWIW, the lunar cratering model is ridiculous to use within the asteroid belt itself, but I'm not going to fight that battle on StackExchange.  
> **username_1**: @StuartRobbins Well, the other answer was accepted five years ago, when it was the only answer—and it was an accurate answer at the time of writing! And SE does not allow to change once an answer is accepted.  
> **username_2**: Ha!  I was tired and didn't think to look at the date.  And apparently it does let you change things, since your answer is now accepted.  
> **username_1**: Yes, it looks like someone has changed the tick after all. Thanks!  

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### Answer by username_3 on 2015-11-19. Score: 2

[It seems](https://gsa.confex.com/gsa/2015AM/webprogram/Paper260706.html) not yet. [The non-uniform density of craters](https://gsa.confex.com/gsa/2015AM/webprogram/Paper260352.html) seen on Ceres is still under investigation. From the abstracts of those papers, they're still working on trying to date the ejecta material from that crater, and trying to understand the resurfacing that appears to be going on.


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