Jean-Baptiste Vincent updated 08 Oct. 2014

Slides:



Advertisements
Similar presentations
Open your binder to the notes section. Prepare to take notes
Advertisements

Can we use total field magnetics to find buried pit houses beneath layers of volcanic ash? Visible pit houses at Bridge River, B.C. (Prentiss et al., 2009)
Objective Our primary objective was to research craters in close proximity to the Mare Orientale basin. We scoured this section of the moon looking for.
Measuring the height of Lunar Mountains using data from the Liverpool Telescope.
The Moon.
Topographic Maps specialized maps which show the highs and lows (relief) of the Earth’s surface.
CONTOUR LINES.
Deep Impact Projectsmfa - 1 Deep Impact Projects (2) Mike A’Hearn.
Mapping Earth's Surface Review and Assessment Answers
Lesson 2 The Earth-Sun-Moon System
Summary Of the Structure of the Milky Way The following graphical data is meant to help you understand WHY astronomers believe they know the structure.
Levels of organization: Stellar Systems Stellar Clusters Galaxies Galaxy Clusters Galaxy Superclusters The Universe Everyone should know where they live:
The Moon, Our Constant Companion
Galaxies.
The Solar System. Overview of the Solar System Basics Source: Nine Planets - A Multimedia Tour of the Solar System * By Bill Arnett.
CCDs in space: the effects of radiation on Hubble’s Advanced Camera for Surveys (ACS) Max Mutchler, David Golimowski (Space Telescope Science Institute),
SHINE SEP Campaign Events: Long-term development of solar corona in build-up to the SEP events of 21 April 2002 and 24 August 2002 A. J. Coyner, D. Alexander,
Phases of Venus. Share Question How much more solar energy does Venus receive than the Earth, due to the fact that Venus is 0.72 times as far from the.
The Innermost Planet MERCURY.
Moon Impact Studies. What do We Know About the Moon?
Latitudinal Trend of Roughness and Circumpolar Mantles on Mars M. A. Kreslavsky J. W. Head III Brown University.
Sponge – What is a synchronous orbit?. Surface Features - Maria - oceans or seas. (Galileo thought they were oceans when he saw them through his.
Mars Student Imaging Program The Three Principles Impact Craters Features you must know and understand. Ejecta – Material, from the crater, that was thrown.
Planetary image interpretation and mapping Phil Stooke USGS map I-515.
Bradley Central High School
 If you were gone Friday  I need to check bellwork  I need to check your moon stations work  You must come in before or after school to make up a.
The Moon Origins And Features. Lunar Formation Models The moon is a sister world that formed in orbit around Earth as the Earth formed. The moon formed.
American Unmanned Mission: Surveyor ( )
Peculiar texture of high-latitude ground-ice-rich terrains M. A. Kreslavsky and J. W. Head Brown University Kharkov Astronomical Institute.
BACKGROUND MARS Research Presentation By Bradley Central Chemistry 3 rd Period Dr. Buckner.
Gale Crater Stratigraphic Measurements and Preliminary Interpretations Ryan Anderson April, 2009.
Unit 11 Mars. Physical Properties Radius: 3400 km Moons: Deimos, Phobos Mass: 6.4 × kg Density: 3900 kg/m 3 Length of Day: 24.6 hours.
Geological Features of the Earth How do natural processes affect geologic features? How do natural processes affect geologic features?
Galaxies. The Hubble Tuning-Fork Diagram This is the traditional scheme for classifying galaxies:
The Phases of the Moon Section ain.html#part2.
Impact craters are geologic structures formed when a large meteoroid, asteroid or comet smashes into a planet or a satellite.Impact craters are geologic.
Rock Slide—Palisades Cliffs May 12, 2012 Images and “Why it Happened”
EART 160: Planetary Science 11 February Last Time Paper Discussion: Stevenson (2001) –Mars Magnetic Field Planetary Interiors –Pressure inside Planets.
On the Larger Picture in Cometary Science
The Asteroid Belt and Beyond!
Craters on Comets J.-B. Vincent, N. Oklay, S. Marchi, S. Höfner, H. Sierks 33 (6 outlines) -> 27.
Volcanoes.
C-G: Conundrums and Antagonisms
Analysis and characterisation of the Aswan *possible* cliff collapse
60 1. What is the mass M in the system as given in the
© 2017 Pearson Education, Inc.
TERRAINS Terrain, or land relief, is the vertical and horizontal dimension of land surface. Terrain is used as a general term in physical geography, referring.
Rosetta/OSIRIS Morphology.
Landscape Development
Jets and sources of activity on 67P observed by OSIRIS
33 (6 outlines) -> 27.
“Venus Unveiled” The movie you are about to watch today is a little long for most of my students, but the material you will see here is some incredible.
W.-H. Ip Zhongyi Lin, Ian Lai, Vickie Lee. Yuan Li NCU/MUST
Changes on the smooth region of Imhotep
The ability for the ocean to absorb and store energy from the sun is due to… The transparency of the water that allows the sun’s ray to penetrate deep.
Ocean Floor.
Key Vocabulary Eclipse Vocabulary Annular eclipse Annulus Penumbra
Earth’s History.
Empirical Criteria for Rainfall-Induced Landslides
GG 450 February 19, 2008 Magnetic Anomalies.
Cratering on Small Bodies: Lessons from Eros
R.A. Yingst, F.C. Chuang, D.C. Berman, S.C. Mest
But…there is no book! Oh…rats…
When Mount St. Helens erupted, trapped gases caused the north side of the mountain to explode. Volcanic ash was ejected high into the atmosphere.
Sponge – What is a synchronous orbit?
Earth Science Chapter 8 Section 3
Terrestrial Planetary Geology: Basic Processes & Earth
Topographic Features L.O: STUDENTS WILL DESCRIBE HOW GRADIENT (SLOPES), HOLES & RIVERS ARE SHOWN ON TOPOGRAPHIC MAPS .
Ricocheting Black Hole Jet Discovered By Chandra
But…there is no book! Oh…rats…
Presentation transcript:

Jean-Baptiste Vincent updated 08 Oct. 2014 Activity and pits on 67P Jean-Baptiste Vincent updated 08 Oct. 2014

Is there such a thing as an active area Is there such a thing as an active area ? Are there features directly linked to activity, either as source or consequence ? The beginning of an answer to the activity question is the deep cylindrical hole seen close to the North pole of the comet.

Many jets can be linked to this hole, apparently starting from the bright walls on both sides. Note that the illuminated side of the hole in the image below is the opposite of the one seen in the image above and on previous slide. There is almost continuous activity during a comet day as each side gets illuminated. The hole has a very peculiar morphology, with horizontal layers, but also vertical striations and maybe small spherical features yet to be explained.

Is this pit a typical "active area" Is this pit a typical "active area" ? If yes, there should be others, with similar morphology and activity. We have two more in the same image, and they show some faint structures which are NOT compression artifacts (we have some in this image but nowhere near the jets). Jets ?

SHAP5 images. Some shadows show signal (blue), some not (red), are we seeing dust from active spots or just faint signal from the surface itself ?

Looking at it from a different angle, it’s as if the 3 depressions are slowly evolving into one common pit. Their floors have different elevation, though, which could be a signature of their relative age: the deepest = the oldest, or an intrinsic feature predating the activity.

Pit forms and expands radially Since all walls of the pits seem to be active, it's natural to think that they will expand radially. If a pit is initially formed on a sloped/terraced terrain, the circular shape will disappear after a while and only a fraction of the circle will remain. The downward expansion is more difficult to explain, as we need to be sure that any excavated material will escape the pit and not fall back on the floor. The depth of the pit could be indicative of the strength of the activity/gas pressure below the floor/volatile content. Poor artistic skills ! Pit forms and expands radially Pit edge cuts through existing cliff/slope, circular shape is lost

Physics ! 200 m Can erosion alone creates such a pit ? We take Seth_00 as an example. V = π r2 h = 6.28e6 m3 ρ = 400 kg/m3 => M = 2.5e9 kg 200 m Assuming Qdust = Qgas in mass, and Qgas from TN-5556 Qdust_perihelion = 255 kg/s => Terosion = 9.8e6 s = 3.7 months* Qdust_3.5AU = 9.3 kg/s => Terosion = 269e6 s = 8.5 years* (*) … of constant activity These numbers are an optimistic lower limit. If we take into account the latitude, we see that a pit like Seth_00 can only be active for a few months per orbit. Erosion is taking place but cannot be the only process forming the pit Need for a short-time, catastrophic event.

Source of outburst ? If erosion is not sufficient, we need to trigger an explosion somewhere below the surface. (I'm ruling out pits as primordial features) which mechanism ? how deep is the explosion taking place ? how deep are we excavating ? is d/D = 1 primordial ? Source ? super volatiles building up pressure below the surface ? cannot be too far deep, thermal gradient very steep exogenic phase transition ? see Dennis' talk

Explosive events. Methane sink holes in Siberia Explosive events ? Methane sink holes in Siberia. 30m diameter/ >70m depth K. Moskvitch, Nature, 31st July 2014

What about other pits/holes ? I started to prepare a catalog of all the pits seen in SHAP4S/SHAP5 images. I named the first one "Seth_00". I use it as a reference and every other depression is compared to this one. Selection criteria: circular or quasi-circular shape layers and/or vertical striations rough "cliffs", with possible debris field at their feet smooth floor (activity)

Seth Regio

Seth_00 to Seth_04 4 2 1 3 mean d/D = 0.9 3 Pit # Diameter Depth Depth/Diameter Seth_00 213 176 0.83 Seth_01 114 91 0.79 Seth_02 118 99 0.84 Seth_03 126 138 1.10 Seth_04 221 198 0.90 mean d/D = 0.9 Note: depth estimated from shadows and visible cliffs on flat images. Needs to be measured again on a proper DTM.

There are many "half-pit" structures in the same region. I'd like to think they use to be similar to Seth_00 but they could be formed by a completely different process. Former pits ?

Seth_05 Next to landing site C. Circular hole, vertical striations along the cliffs, smooth floor with some debris, no activity visible in this image

Ash Regio

Ash_01 & Ash_02 2 1 Tail side. Pits which resemble the other ones, but are partly embedded in dust mantle. Not clear to me if they are active spots or not. The floor of pit Ash_01 is brighter than the surroundings, fresh material ? Note that this is potentially the secondary source of activity predicted by Björn Davidsson and myself from inversion of jets and coma water density in the approach phase.

Ash_03-06 03 04 05 06 Right wing. Again many depressions and half-pits are seen there. Ash_03 & Ash_04 are much shallower than the reference pit, with a bowl shape instead of a cylindrical morphology. Probably not active pits, maybe these are signatures of inner voids, as Simone suggested. Ash_05 & Ash_06 are more like the reference, but the high curvature of the surface in this region complicates the interpretation.

Imhotep Regio

Imhotep regio A few depressions which could be related to activity (blue lines) Many circular features, described as consolidated terrain around impact craters by myself, or alternatively mud volcanoes by Anne-Thèrèse. Probably not active.

Ma'at Regio

Ma'at_01 & Ma'at_02 Two pits on the left side of the head, same morphology, jets detected 2 1 Many small depressions and granular flows can be seen in between the two pits, possible activity ongoing !

Ma'at_01 & Ma'at_02 2 1 More flows visible in high resolution (SHAP5 images)

Possible jets coming out of these pits. Single image inversion gives sources in the vicinity of Ma'at_01 and Ma'at_02 but we are not yet able to link this unambiguously to these two pits. Jet-like features coming out of the neck could look similar due to projection effects. Very close to the nominal landing site (J).

Ma'at_03 Several examples on the right side of the head. Morphology somewhat different from the reference pit: less deep, and with a rougher floor. It seems to me that if these were active pits, they have not been releasing gas/dust for a long while. They look older and the debris field is in my view more characteristic of rim failure and mass wasting than fresh dust.

Bastet Regio

Bastet_01 Right side of the head. Possibly a very old pit. Impressive set of striations on the surface, and significant mass wasting.

Map of pits Pits positions close to the neck are not well projected but this view gives you an idea of where they are. Exact positions given in separated XLS file.

Statistics

Summary Many pits on the comet, very specific morphology. Several of them show evidence for activity. Active pits appear to have a d/D close to 1 (depth = diameter), while inactive ones are much shallower Current activity/erosion alone is not sufficient to form these pits. They are more likely to start from an outburst/sink by surface collapse, and expand later with the sublimation of the inner walls. Pits can continue to evolve even without volatiles, but on much longer time scale like traditional craters (mass wasting, rim failure, deposit of ejecta from nearby active sources, …). Dust which cannot escape the pits accumulates at the bottom and forms a smooth layer, which can be moved or lifted later by complex gas flows. The walls (or ice layers within them) seem to be the main source of activity. Pit erosion by activity is an ongoing process. We are monitoring these areas since August, and might have already detected changes. Careful comparison between all images will tell us…