we are made out of star dust [in greek]

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Ακαδημία Περιφερειακής Ενότητας Έβρου Είμαστε φτιαγμένοι από … αστερόσκονη Ελένη Καλδούδη Αν. Καθηγήτρια, Σχολή Επιστημών Υγείας, ΔΠΘ 30 Μαρτίου 2016 Η οργάνωση του μικρόκοσμου στη σύγχρονη φυσική

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  • . , ,

    30 2016

  • Hubble

    ( 1/10 )

    : https://en.wikipedia.org/wiki/Universe#/media/File:NASA-HS201427a-HubbleUltraDeepField2014-20140603.jpg

    : https://en.wikipedia.org/wiki/Full_moon

    https://en.wikipedia.org/wiki/Universe#/media/File:NASA-HS201427a-HubbleUltraDeepField2014-20140603.jpghttps://en.wikipedia.org/wiki/Full_moon

  • Hubble:

    , 1990 ( ~2030)

    134 m, 11tn

    Hubble: https://en.wikipedia.org/wiki/Hubble_Space_Telescope

    : https://en.wikipedia.org/wiki/Astronaut#/media/File:Astronaut-EVA.jpg

    https://en.wikipedia.org/wiki/Hubble_Space_Telescope

  • ~1026 m

    ~13.7

    ~200

    (

    )The Hubble Deep Field - NorthR. Williams (STScI), the Hubble Deep Field Team and NASAhttp://museumvictoria.com.au/discoverycentre/infosheets/planets/the-universe/

    1026 m = 100 000 000 000 000 000 000 000 000

    26 !!!

    1026

  • ~100.000

    ~100

    ( )

    =

    1 9,51015 m

    9,5

    Galaxy Messier 83.

    http://www.spitzer.caltech.edu/images/4832-sig11-

    016-A-Dusty-View-of-Milky-Ways-Smaller-Cousin

    COBE image of the Milky Way

    http://map.gsfc.nasa.gov/media/ContentMedia/dirbe123_2p6dec.jpg

    24.000

    1026 1016 m

    1016 m = 10 000 000 000 000 000

    16 !!!

  • 5.7 1012 m

    1,4 109 m

    8 (, , )

    http://www.planetaryvisions.com/Project.php?pid=2229

    5.71012 m

    1026 1016 1012 m

    = 106 = 1 000 000

  • 6.4 106 m

    1,7 m

    1026 1016 1012 106 m 10 m

    = 106 = 1 000 000

    = 106 = 1 000 000

    NASA, EPIC, Deep Space Climate Observatory (DSCOVR)

    http://www.space.com/31368-nasa-satellite-epic-earth-portraits-video.html

  • 10m 100 m

    https://en.wikipedia.org/wiki/Cell_(biology)#/media/File:DAPIMitoTr

    ackerRedAlexaFluor488BPAE.jpg

    1013 = = 10 000 000 000 000 = = 10 .

    1026 1016 1012 106 m 10 m 106 m

    = 106 = 1 000 000

  • -, nuclear magnetic resonance (NMR),, , (MS),surface plasmon resonance (SPR) atomic force microscopy (AFM)

    (HM),

    (confocal)

    -F ()

    (MRI, CT ultrasound)

    (PET, MRSI)

    ()

    (re

    solu

    tio

    n)

    : , . . , [email protected]

  • ,

    http://www.uniprot.org/

    ( 2015)

    549.000

    (

    )

    50.800.000

    http://www.uniprot.org/

  • 92

    500.000*

    24

    500.000

    ( . , , 2007 http://users.ntua.gr/nborbil/Article1.htm

    ~150.000 . , 2006

    1 nm 10 m

    ?

    http://users.ntua.gr/nborbil/Article1.htm

  • C24H8O6

    Iwata et al, Nature Communications, 2015

    http://www.nature.com/ncomms/2015/150716/ncomms8

    766/full/ncomms8766.html

    0.5nm

    1 = 109 =1

    1 000 000 000

    K. A. Cochrane et al , Nature Communications,

    2015http://www.nature.com/ncomms/2015/151006/nco

    mms9312/full/ncomms9312.html

    http://www.nature.com/ncomms/2015/151006/ncomms9312/full/ncomms9312.html

  • ?

    1900, ()

    =

    1900

    ~ 10-10m

    1010 =1

    1010=

    1

    10 000 000 000

  • ( )

    ( )

    ( )

  • 1909 1914

    Geiger & Marsden

    Rutherford

    ,

    (2p+2n)

    -

    -

    -

    - -

    --+++++++

    10-15 10-14 m

    10-10 m

    1026 1016 1012 106 10-10 10-15 m

  • (1)

    (2) (

    )

    (3)

  • (1)

    (

    )

    (2)

    (. )

    (3)

  • (3)

    (3)

    (1) ( )

    (2)

    (.

    )

    (2)

  • / ?

    Fermilab

    SLAC

    KEKCERN

    DESY

    BNL

    CESR

  • 17 1969

    Robert R. Wilson,

    ( Fermi Lab, http://www.fnal.gov/),

    , 250 $

    Fermi Lab

    ( Wilson :

    http://history.fnal.gov/testimony.html)

    http://www.fnal.gov/http://history.fnal.gov/testimony.html

  • http://w

    ww

    .dennish

    olm

    esd

    esigns.com

    /alber

    t_einste

    in.htm

    l

    htt

    p://

    ww

    w.s

    hut

    ters

    tock

    .co

    m/p

    ic-7

    36

    76

    83

    9/s

    tock

    -ve

    ctor

    -ang

    ry-c

    arto

    on-d

    rill-

    serg

    ean

    t-sc

    ream

    ing-

    in-

    ange

    r.htm

    l

    ?

    .

    ...

  • Fermilab (45 km Chicago)

    2

  • http://www.google.com/imgres?q=cern&hl=el&sa=X&rls=com.microsoft:en-us:IE-Address&biw=1228&bih=689&tbm=isch&prmd=imvnsz&tbnid=eYcOShzB7qCErM:&imgrefurl=http://www.pknews.gr/2011/06/cern-

    photos.html&docid=Kly3qKBI3MjgdM&imgurl=http://2.bp.blogspot.com/JnQ0PFXUY3E/Tgyb8tp2PpI/AAAAAAAALjM/EiliFMmmL0Q/s1600/cern1.jpg&w=1491&h=1020&ei=nRyJUL2wJcXXtAbZx4GIBQ&zoom=1&iact

    =rc&dur=284&sig=110011389120735540536&page=1&tbnh=181&tbnw=272&start=0&ndsp=12&ved=1t:429,r:7,s:0,i:104&tx=77&ty=60

    CERN

    8.5

  • CERN = Conseil Europeen pour la Recherche Nucleaire

    European Organization for Nuclear Research

    www.cern.org

    2.500

    10.000

    web!

    Large Hadron Collider

    ( & ) =

    http://el.wikipedia.org/wiki/%CE%9C%CE%B5%CE%B3%CE%AC%CE%BB%CE%BF%CF%82_%CE%95%CF%80%CE%B9%CF%84%CE%B1%CF%87%CF%85%CE%BD%CF%84%CE%AE%CF%82_%CE%91%CE%B4%CF%81%CE%BF%CE%BD%CE%AF%CF%89%CE%BD

    http://en.wikipedia.org/wiki/File:Cernfounders.pnghttp://en.wikipedia.org/wiki/File:Cernfounders.pnghttp://www.cern.org/

  • LHC (Large Hadron Collider)

    27 Km

    50 -175 m

    (

    )

    1994

    > 3 .

    : 3,5 eV 30 2010

    : 7 eV

    http://www.imerisia.gr/article.asp?catid=26514&subid=2&pubid=112153381

  • LHC (Large Hadron Collider)

    , 2 :

    7TeV

    ( )

    ,

    2808

    ~7 m (25ns)

    ~1011 ,

    ~0.5ng,

    16m ( 50 m)

    20J ,

    30m/s

    http://www.lhc-closer.es/php/index.php?i=1&s=1&p=1&e=0

  • ,

    2

    p (proton)

    n (neutron)

    = =

    =

    = = = +

    X(, ) XAZ

    p

    n

    u u

    d

    d d

    u

    +

  • 92

    92

    1

    2 e

    3 Li

    4 Be

    5

    6 C

    7 N

    8 O

    .

    15 P

    19 K

    20 Na

    92 U

  • http://ylikonet.gr/group/diktyo/forum/topics/3647795:Topic:299620

    (92+)

  • ,

    ,

    :

    :

    : 12C, 13C, 14C,

    12C 98,9% 13C1,1%

    A Z X X, X, X

  • ()

    ,

    .. :

    ( )

    15

    2 (C-12 & C-13)

    3 (C-12, C-13 & C-14)

    C-8C-9C-10C-11C-12C-13C-14C-15C-16C-17C-18C-19C-20C-21C-22

  • ?

    ( ,

    )

    ( )

  • ~ 270

    ~ 900 ()

    3.300

  • 0 20 40 60 80 100 120 140 160 220180 240200

    9

    8

    7

    6

    5

    4

    3

    2

    1

    ( )

    56-60

    24He

    816O

    1531P

    2656Fe

    92238U

  • 0 20 40 60 80 100 120 140 160 220180 240200

    9

    8

    7

    6

    5

    4

    3

    2

    1

    ( )

    24He

    816O

    1531P

    2656Fe

    92238U

  • 0 20 40 60 80 100 120 140 160 220180 240200

    9

    8

    7

    6

    5

    4

    3

    2

    1

    ( )

    24He

    816O1531P

    2656Fe

    92238U

    He

    H

    +

    ++ +

    ++

    +

    ++

    + +

  • NASA

    http://www.isciencetimes.com/articles/6486/20131207/nasa-scientist-maps-suns-plasma-flow-solar-flare.htm

  • BICEP2 2014, NASA

    http://bicepkeck.org/visuals.html

    t=0

    , , (= )

    10-43 1 s

    , ,

    1 1000 s:

    4 : 2p +2n He ()

    12 :

    1000s 300 000 :

    300 5 :

    8.5 9 :

    =7

    1=14

    2

    ~25%

    ~75%

    13.7

  • 75% 25% e

    : 100

    ,

    ( )

    ,

  • 24

    (4,2)

    12C

    12

    16

  • 0 20 40 60 80 100 120 140 160 220180 240200

    9

    8

    7

    6

    5

    4

    3

    2

    1

    ( )

    24He

    816O

    1531P

    2656Fe

    92238U

    56-60

  • NASAs Solar Dynamics Observatory Atmospheric Imaging Assembly (AIA)https://frontierscientists.com/2012/02/space-weather-and-your-technology/

  • ,

    (Fe-56)

    https://en.wikipedia.org/wiki/Stellar_evolution#/media/Fi

    le:Evolved_star_fusion_shells.svg

  • (Fe-56)

    ,

    ,

    (supernova)

    ,

    Cas A

    300

    http://spacefellowship.com/news/art15247/neutron-star-at-core-of-

    cassiopeia-a-has-carbon-atmosphere.html

  • https://en.wikipedia.org/wiki/Nucleosynthesis

  • ;

  • scanning tunneling microscopy http://phys.org/news/2010-04-molecule.html

    d

    d

    1010 =1

    1010 =

    1

    10 000 000 000

    : 60%

    2 :

  • ~10.000 , ,

    ,

    4

    http://www.anesthesia2000.com/physi

    cs/Chemistry_Physics/physics21.htm

    C2952 H4664 O832 N812 S8 Fe4

    5.5 = 5.5 109 =1

    1010 =

    5.5

    1 000 000 000

    :

    http://www.anesthesia2000.com/physics/Chemistry_Physics/physics21.htm

  • 280 000 000

    , 2 400 000

    - 100

    https://en.wikipedia.org/wiki/Blood#/media/File:Humanrbc1000x.jpg

    https://en.wikipedia.org/wiki/Blood

    7 = 7 106 =7

    106 =

    7

    1 000 000

    :

    https://en.wikipedia.org/wiki/Blood#/media/File:Humanrbc1000x.jpghttps://en.wikipedia.org/wiki/Blood

  • 5 107 = 50 000 000

    3 1013 = 30 000 000 000 000

    E. Bianconi et al, An estimation of the number of cells in the human body, Annals of Human Biology, vol.4(6), 463-472, 2013

    7.4 109 = 7 400 000 000

    http://solarviews.com/eng/earth.htm

  • W49B

    1000

    http://www.nasa.gov/sites/default/fi

    les/snr_fingerprint_large_0.jpg

  • , 68100

    Tel: 2551030329 & 6937124358

    Email: [email protected]

    :

    ,

    ,

    , 30 2016

    http://www.peevrou.eu/index.php/menu-

    acadimia-peevrou/menu-genikes-plirofories#

    mailto:[email protected]://www.peevrou.eu/index.php/menu-acadimia-peevrou/menu-genikes-plirofories