APOD: Ireson Hill on Mars (2017 Jul 19)

Post a reply


This question is a means of preventing automated form submissions by spambots.
Smilies
:D :) :ssmile: :( :o :shock: :? 8-) :lol2: :x :P :oops: :cry: :evil: :roll: :wink: :!: :?: :idea: :arrow: :| :mrgreen:
View more smilies

BBCode is ON
[img] is ON
[url] is ON
Smilies are ON

Topic review
   

Expand view Topic review: APOD: Ireson Hill on Mars (2017 Jul 19)

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by Chris Peterson » Thu Jul 20, 2017 1:21 pm

JohnD wrote:
Chris Peterson wrote:
JohnD wrote:Meteoric iron would be nice. But landing at the usual speed for a meteor, with almost no atmosphere to slow it down would crater the bedrock and spread the meteor across the Marscape as vapour, condensing to dust. Is there a mechanism for a slow speed landing?
Yeah. The atmosphere. The rovers have found many meteorites sitting on the surface. On Mars, meteoroids which survive burning up in the upper atmosphere fall with a terminal velocity on the order of five to ten times that on Earth, still below the speed of sound and too slow to cause cratering. (Recall that Martian landers typically use parachutes for part of their landing sequence.)
Chris,
But something the size of Ireson Hill?
No, very unlikely. Sorry if I wasn't clear. I didn't mean to suggest I think this hill is an ancient meteorite, only that the atmosphere of Mars behaves much the same as that of Earth when it comes to meteorites surviving to the surface.

The largest meteorites on the Earth are on the order of two to three meters across. The lower limit on initial speed for a Martian meteoroid is about 5 km/s (compared with about 11 on Earth), so I imagine we might have somewhat larger bodies reaching the ground intact. But not, I think, anything the size of Ireson.

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by neufer » Thu Jul 20, 2017 11:05 am

JohnD wrote:
But Ireson Hill is intact and there is no crater.
Therefore Ireson is not a meteorite.
IMO, Ireson and the rest of the more weathered dark dunes are all formed from iron rich meteorite material left over from the formation of Gale Crater.

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by JohnD » Thu Jul 20, 2017 8:06 am

Chris Peterson wrote:
JohnD wrote:Meteoric iron would be nice. But landing at the usual speed for a meteor, with almost no atmosphere to slow it down would crater the bedrock and spread the meteor across the Marscape as vapour, condensing to dust. Is there a mechanism for a slow speed landing?
Yeah. The atmosphere. The rovers have found many meteorites sitting on the surface. On Mars, meteoroids which survive burning up in the upper atmosphere fall with a terminal velocity on the order of five to ten times that on Earth, still below the speed of sound and too slow to cause cratering. (Recall that Martian landers typically use parachutes for part of their landing sequence.)
Chris,
But something the size of Ireson Hill?
I went away to calculate, and meanwhile you and neufer talk up a storm! But I think I still have a point to make.

Ireson is 5 x 15m, or about a 10m wide stone. If it is meteoric iron then it will have a mass of about 4,000 tonnes.
Most meteorites seen on Mars, or found on Earth, are much smaller. Why?
The American Meteor Society estimates that meteors encounter the Earth at 11-72 Kilometers/sec- assume that true for Mars, but that's almost irrelevant, due to atmopsherioc drag.
NASA calculates terminal velocity due to atmospheric drag by Vt = SQR[2W/Cd Rho A]
Where W = Mass = 4x10^6 kg
Cd = Coeff drag For a sphere, about 0.6
Rho = atmospheric density At surface, ~0.020 kg/m3. Obviously the higher the lower, but this figure will maximise drag.
A = Fontal area 10m sphere = 78m^2
So Vt = SQR(2 x 4x10^6/0.6 x 0.02 x 78)
= 3000msec = 3kilometers/sec

This is at the lower limit for a "hypervelocity" impact, that would vapourise the meteor and raise a significant crater.
But Ireson Hill is intact and there is no crater.
Therefore Ireson is not a meteorite.
JOhn

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by Chris Peterson » Thu Jul 20, 2017 3:46 am

neufer wrote:
Chris Peterson wrote: (BTW, the correct term for material which survives ablation and is in the process of cold fall is "meteorite". Even before it hits the ground.)
  • Meteoroid => Meteor => Meteorite
That's not quite accurate. A meteoroid becomes a meteorite (assuming some of it survives ablation). The ablation process produces a physical phenomenon of energy release we call a meteor.

The Wikipedia article is also not too accurate anymore. Might have to edit it.

In actual usage, for many years now, surviving meteoritic material has been called a "meteorite" (including "micrometeorite") even before hitting the ground. This is especially true considering that the old IAU definitions didn't say "ground", but "Earth". Pretty useless since we've started finding meteorites on other planets!

In any case, as noted, the actual usage is what it is, and doesn't strictly follow the old IAU definitions. There are now new definitions (I was part of the committee that created them). They are still provisional (although in wide use), but will almost certainly be approved unchanged by Commission 22 at an IAU meeting in the near future.

The relevant new definitions are:

Meteor is the light and associated phenomenon (heat, shock, ionization), which results from the entry of a solid object from space into a gaseous atmosphere.

Meteoroid is a solid object of a diameter between 30 µm and 1 meter moving in, or coming from, interplanetary space.

Meteorite is any solid object that survived the meteor phase in a gaseous atmosphere without being completely vaporized.

Re: I hate vertically stretched images.

by geoffrey.landis » Thu Jul 20, 2017 3:40 am

bystander wrote:It's not vertically stretched, it's horizontally compressed.
ROFL.

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by neufer » Thu Jul 20, 2017 2:12 am

Chris Peterson wrote:
(BTW, the correct term for material which survives ablation and is in the process of cold fall is "meteorite". Even before it hits the ground.)
  • Meteoroid => Meteor => Meteorite
https://en.wikipedia.org/wiki/Meteorite wrote:
<<A meteorite is a solid piece of debris from an object, such as a comet, asteroid, or meteoroid, that originates in outer space and survives its passage through the Earth's atmosphere and impact with the Earth's surface or that of another planet. When the object enters the atmosphere, various factors like friction, pressure, and chemical interactions with the atmospheric gases cause it to heat up and radiate that energy. It then becomes a meteor and forms a fireball, also known as a shooting star or falling star; astronomers call the brightest examples "bolides." Meteorites that survive atmospheric entry and impact vary greatly in size. For geologists, a bolide is a meteorite large enough to create a crater.>>
https://en.wikipedia.org/wiki/Meteoroid wrote:
<<A meteoroid is a small rocky or metallic body in outer space. Meteoroids are significantly smaller than asteroids, and range in size from small grains to 1 meter-wide objects. Objects smaller than this are classified as micrometeoroids or space dust. Most are fragments from comets or asteroids, whereas others are collision impact debris ejected from bodies such as the Moon or Mars.>>
https://en.wikipedia.org/wiki/Asteroid#Terminology wrote:
<<Traditionally, small bodies orbiting the Sun were classified as comets, asteroids, or meteoroids, with anything smaller than 10 meters across being called a meteoroid (such as in Beech and Steel's 1995 paper). The term "asteroid", from the Greek word for "star-like", never had a formal definition, with the broader term minor planet being preferred by the International Astronomical Union. However, following the discovery of asteroids below 10 meters in size, Rubin and Grossman in a 2010 paper revised the previous definition of meteoroid to objects between 10 µm and 1 meter in size in order to maintain the distinction between asteroids and meteoroids.>>

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by Stephen Dale » Thu Jul 20, 2017 1:54 am

MIght it be an ancient meteor shock cone that has been eroded?

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by Chris Peterson » Thu Jul 20, 2017 1:27 am

neufer wrote:
Chris Peterson wrote:Sure. But even under current conditions, the atmospheric density in Earth's atmosphere at the point where meteorites [sic] are typically in free fall (they have lost their initial velocity) corresponds to a height in the Martian atmosphere of about 10 km.
That sort of depends on the size of the meteor [sic].
Obviously. If the meteoroid is more than a few meters in diameter, it's possible for it to reach the ground before it loses all of its initial velocity, which means the collision could release much more energy- enough to melt some or all of the body and to produce a crater. But the important point here is that the production of meteorites on Mars is similar to that on Earth.

(BTW, the correct term for material which survives ablation and is in the process of cold fall is "meteorite". Even before it hits the ground.)

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by neufer » Thu Jul 20, 2017 12:03 am

Chris Peterson wrote:
neufer wrote:
Chris Peterson wrote:
Yeah. The atmosphere. The rovers have found many meteorites sitting on the surface. On Mars, meteoroids which survive burning up in the upper atmosphere fall with a terminal velocity on the order of five to ten times that on Earth, still below the speed of sound and too slow to cause cratering. (Recall that Martian landers typically use parachutes for part of their landing sequence.)
Meteoric iron in the past could also have been slowed by:
  • 1) a thicker atmosphere
    2) a crater lake and/or
    3) the sediment left by that lake.
Sure. But even under current conditions, the atmospheric density in Earth's atmosphere at the point where meteorites [sic] are typically in free fall (they have lost their initial velocity) corresponds to a height in the Martian atmosphere of about 10 km.
That sort of depends on the size of the meteor.

Re: I hate vertically stretched images.

by bystander » Wed Jul 19, 2017 10:55 pm

geoffrey.landis wrote:Really. This is not a feature on Mars.
It's not vertically stretched, it's horizontally compressed.

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by Chris Peterson » Wed Jul 19, 2017 10:41 pm

neufer wrote:
Chris Peterson wrote:
JohnD wrote:
Meteoric iron would be nice. But landing at the usual speed for a meteor, with almost no atmosphere to slow it down would crater the bedrock and spread the meteor across the Marscape as vapour, condensing to dust. Is there a mechanism for a slow speed landing?
Yeah. The atmosphere. The rovers have found many meteorites sitting on the surface. On Mars, meteoroids which survive burning up in the upper atmosphere fall with a terminal velocity on the order of five to ten times that on Earth, still below the speed of sound and too slow to cause cratering. (Recall that Martian landers typically use parachutes for part of their landing sequence.)
Meteoric iron in the past could also have been slowed by:
  • 1) a thicker atmosphere
    2) a crater lake and/or
    3) the sediment left by that lake.
Sure. But even under current conditions, the atmospheric density in Earth's atmosphere at the point where meteorites are typically in free fall (they have lost their initial velocity) corresponds to a height in the Martian atmosphere of about 10 km. The scale heights of the two atmospheres aren't radically different (11 km on Mars versus 8.5 km on Earth). Meteors and meteorites don't behave all that differently between the two.

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by neufer » Wed Jul 19, 2017 10:10 pm

Chris Peterson wrote:
JohnD wrote:
Meteoric iron would be nice. But landing at the usual speed for a meteor, with almost no atmosphere to slow it down would crater the bedrock and spread the meteor across the Marscape as vapour, condensing to dust. Is there a mechanism for a slow speed landing?
Yeah. The atmosphere. The rovers have found many meteorites sitting on the surface. On Mars, meteoroids which survive burning up in the upper atmosphere fall with a terminal velocity on the order of five to ten times that on Earth, still below the speed of sound and too slow to cause cratering. (Recall that Martian landers typically use parachutes for part of their landing sequence.)
Meteoric iron in the past could also have been slowed by:
  • 1) a thicker atmosphere
    2) a crater lake and/or
    3) the sediment left by that lake.
http://asterisk.apod.com/viewtopic.php? ... 91#p273085

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by Chris Peterson » Wed Jul 19, 2017 9:59 pm

JohnD wrote:Meteoric iron would be nice. But landing at the usual speed for a meteor, with almost no atmosphere to slow it down would crater the bedrock and spread the meteor across the Marscape as vapour, condensing to dust. Is there a mechanism for a slow speed landing?
Yeah. The atmosphere. The rovers have found many meteorites sitting on the surface. On Mars, meteoroids which survive burning up in the upper atmosphere fall with a terminal velocity on the order of five to ten times that on Earth, still below the speed of sound and too slow to cause cratering. (Recall that Martian landers typically use parachutes for part of their landing sequence.)

Re: I hate vertically stretched images.

by neufer » Wed Jul 19, 2017 9:50 pm

geoffrey.landis wrote:
Really. This is not a feature on Mars.
http://sheltontrails.blogspot.com/2014/08/bar-harbor-blueberry-barrens.html wrote:
<<One of our fondest memories of Bar Harbor Campground is the hillside covered in blueberries overlooking Frenchman's Bay to the north. "Blueberry Barrens" are described by the State of Maine on their website, and I think this hillside fits that description.

May I digress about the rock? It's always there, just under foot, and it clearly plays a major part in how things grow here. I've never known quite what it was, but it's very different from the rest of the island, nothing like the famous pink granite of Cadillac Mountain. The geology map says it's the Bar Harbor Formation, which is composed of sandstones and siltstones that often show obvious bedding layers. I now see the bedrock maps says this is "Ireson Hill": "The rocks found along the shore at The Ovens and in the road-cuts along Route 3 at Ireson Hill on the northern side of the island also belong to the Bar Harbor Formation, but here the rock is flint-like and bedding is difficult or impossible to see. Some of these rocks are believed to be accumulations of ash that settled out of the atmosphere after a volcanic eruption." >>

I hate vertically stretched images.

by geoffrey.landis » Wed Jul 19, 2017 9:12 pm

Really. This is not a feature on Mars.

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by neufer » Wed Jul 19, 2017 7:17 pm

One should note that:

The dark Ireson Hill is located on the dark Bagnold Dune field on the slope of Mount Sharp in Gale Crater on Mars.

More than likely Ireson Hill is made of the same dark material as the Bagnold Dune field.

More than likely they were all under water and/or under other material at one time.

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by JohnD » Wed Jul 19, 2017 6:57 pm

Meteoric iron would be nice. But landing at the usual speed for a meteor, with almost no atmosphere to slow it down would crater the bedrock and spread the meteor across the Marscape as vapour, condensing to dust. Is there a mechanism for a slow speed landing?l
John

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by De58te » Wed Jul 19, 2017 6:24 pm

Here's my layman's theory. At the base of the hill I see light brown colored rock, similar to the color of the horizon and atmosphere. These are more or less layered and even. I would think they are Mars bedrock. Then we see dark grey sand. Wind born of course. On top and scattered haphazardly are dark blue colored rock. They look like mining debris. Most likely they were violently thrown there in maybe a meteor impact. In the NASA panorama link they say that the darker rocks analyzed have more and more iron and alkali. Iron meteor? However the Ireson Hill is at the entrance to a mile long streak of dark blue Martian terrain. The dark rocks could be blasted from the darker terrain. https://mars.nasa.gov/multimedia/images ... h-sol-1598 .

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by BillBixby » Wed Jul 19, 2017 4:45 pm

First impression on viewing the image was to reach for my 3D red and blues. Looks like a great image which will take some study and still leave unresolved questions.

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by Zuben L. Genubi » Wed Jul 19, 2017 3:55 pm

Are these shiny black fragmented rocks found in other rover images? Interesting that they are not found around the base of this feature. The deformation of the pink rock might suggest that this an upthrusting of some sort.

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by neufer » Wed Jul 19, 2017 2:45 pm

http://tolkiengateway.net/wiki/Smials wrote:
Smials were the hobbit-holes tunelled into earth mounds and hills.
  • "Smials. A word peculiar to hobbits (not Common Speech), meaning 'burrow'; leave unchanged. It is a form that the Old English word smygel 'burrow' might have had, if it had survived. The same element appears in Gollum's real name, Sméagol."
    ― Tolkien

    "In a hole in the ground there lived a Hobbit. Not a nasty, dirty, wet hole, filled with the ends of worms and oozy smell, nor yet a dry, bare, sandy hole with nothing in it to sit down on or to eat: it was a hobbit-hole and that means comfort."
    ― The Hobbit, "An Unexpected Party"
For generations the Hobbits, made diggings in the earth to live. By the later Third Age the poorest Hobbits still went on living in burrows of the most primitive kind with only one window or none. For the most well-to-do hobbits, smials were luxurious versions of those primitive diggings of old. Their tunnels had rounded walls and branched to other rooms. Smials included Bag End and the smials along Bagshot Row of Hobbiton, the Great Smials of Tuckborough and Brandy Hall. The latter two were large enough to have ample room for a hundred Hobbits.>>

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by JohnD » Wed Jul 19, 2017 1:45 pm

Curio has been inching up to Ireson since January!
See: http://redplanet.asu.edu/?s=ireson

Lots more views in B&W, but no theories of its formation/

John

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by Keyman » Wed Jul 19, 2017 1:41 pm

Yeahbut. If you do that it looks like a...hill. :(

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by Chris Peterson » Wed Jul 19, 2017 12:36 pm

bls0326 wrote:I like the "uncompressed" version of the today's picture better.
You should always like the click-thru image of APODs better. The images displayed on the main page are almost always reduced resolution, sometimes distorted, and frequently lack embedded color profiles. If you don't regularly follow the main page image to the actual submission, you're usually missing something important.

Re: APOD: Ireson Hill on Mars (2017 Jul 19)

by bls0326 » Wed Jul 19, 2017 12:31 pm

I like the "uncompressed" version of the today's picture better.

Top