G R A V I T Y G R A V I T Y
G G UNDER THE INFLUENCE
UNDER THE INFLUENCE K R I S T E N YO U N G M A N
Published by Kompendium of K Press 69 Kissling Street San Francisco, CA 94103 Š 2011 Kompendium of K Press All rights reserved Printed and bound in the United States of America 11 1 First Edition No part of this book may be used or reproduced in any manner without written permission from the publisher, except in context of reviews. Every reasonable attempt has been made to identify owners of copyright. Errors or omissions will be corrected in subsequent editions. Library of Congress Cataloguing-In-Publication Data Gravity:Under the Influence/ edited by Kristen Youngman
p.cm. - (Design Briefs)
Includes bibliographic references and index.
ISBN 000-000-000 1. Handbooks, manuals, etc. 2. Book design, book reference.
Dedication This book is dedicated to Cindy Loffler and Jon Burg. Without their love and support, I’m not sure I would have been able to escape the gravity of my situation. You guys are the best.
Acknowledgments Special thanks to Julia Brown at the Academy of Art University and the GD 221 class. Really enjoyed all your inspiration, encouragement and talent you shared with me. I hope our paths cross often in the future.
Contents 4
1.0 Freeform Collage
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2.0 Letterforms
14
3.0 Photography
24
4.0 Pattern
34
5.0 Grid
36
6.0 Identity
40
7.0 Infographics
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8.0 Paper Composition
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9.0 Word Play
56
10.0 Environment
1.0 Freeform Collage
Gravitation, or gravity, is a natural phenomenon by which physical bodies attract with a force proportional to their mass. In everyday life, gravitation is most familiar as the agent that gives weight to objects with mass and causes them to fall to the ground when dropped. Gravitation causes dispersed matter to co-
in its orbit around the Earth; for the formation
alesce, and coalesced matter to remain intact,
of tides; for natural convection, by which fluid
thus accounting for the existence of the Earth,
flow occurs under the influence of a density
the Sun, and most of the macroscopic objects
gradient and gravity; for heating the interiors
in the universe. Gravitation is responsible for
of forming stars and planets to very high tem-
keeping the Earth and the other planets in their
peratures; and for various other phenomena
orbits around the Sun; for keeping the Moon
observed on Earth.
7
9
2.0 Letterforms
Einstein proposed that spacetime is curved General Relativity
by matter, and that free-falling objects are moving along locally straight paths in curved
In general relativity, the effects of gravitation are
spacetime. These straight paths are called
Einstein discovered the field equations of
ascribed to spacetime curvature instead of a
geodesics. Like Newton’s first law of motion,
general relativity, which relate the presence
force. The starting point for general relativity is
Einstein’s theory states that if a force is applied
of matter and the curvature of spacetime and
the equivalence principle, which equates free fall
on an object, it would deviate from a geodesic.
are named after him. The Einstein field equa-
with inertial motion, and describes free-falling
For instance, we are no longer following geo-
tions are a set of 10 simultaneous, non-linear,
inertial objects as being accelerated relative to
desics while standing because the mechanical
differential equations. The solutions of the field
non-inertial observers on the ground. In Newto-
resistance of the Earth exerts an upward force
equations are the components of the metric
nian physics, however, no such acceleration can
on us, and we are non-inertial on the ground
tensor of spacetime. A metric tensor describes a
occur unless at least one of the objects is being
as a result. This explains why moving along the
geometry of spacetime. The geodesic paths for a
operated on by a force.
geodesics in spacetime is considered inertial.
spacetime are calculated from the metric tensor.
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13
The Draw of You
If we removed all other masses around us, and only you and typography remained, this would be the result—a typeface based on the Law of Attraction to the reader.
3.0 Photography
Gravitational Attraction [physics] the force of attraction between all masses in the universe; especially the attraction of the earth’s mass for bodies near its surface; “the more remote the body the less the gravity”; “the gravitation between two bodies is proportional to the product of their masses and inversely proportional to the square of the distance between them”; “gravitation cannot be held responsible for people falling in love.” — Albert Einstein
17
Gravitational Interaction: A weak, fundamental interaction between two physical objects due to their mass and energy, especially an interaction occurring between elementary particles.
Gravitational Field: a kind of force that surround massive objects
Weightlessness: absence of a support force
Fundamental Interactions: Also called fundamental force, they are the way that simplest particle in the universe interact with one another.
Strong Interactions: Interactions that are responsible for forces between quarks and gluons and nuclear binding.
4.0 Pattern
Newton’s Theory
In 1687, English mathematician Sir Isaac Newton published Principia, which hypothesizes the inverse-square law of universal gravitation. In his own words, “I deduced that the forces which keep the planets in their orbs must [be] reciprocally as the squares of their distances
from the centers about which they revolve: and thereby compared the force requisite to keep the Moon in her Orb with the force of gravity at the surface of the Earth; and found them answer pretty nearly.”
A discrepancy in Mercury’s orbit pointed out flaws in Newton’s theory. By the end of
Newton’s theory enjoyed its greatest success
the 19th century, it was known that its orbit
when it was used to predict the existence of
showed slight perturbations that could not be
Neptune based on motions of Uranus that
accounted for entirely under Newton’s theory,
Although Newton’s theory has been supersed-
could not be accounted for by the actions of
but all searches for another perturbing body
ed, most modern non-relativistic gravitational
the other planets. Calculations by both John
(such as a planet orbiting the Sun even closer
calculations are still made using Newton’s the-
Couch Adams and Urbain Le Verrier predicted
than Mercury) had been fruitless. The issue
ory because it is a much simpler theory to work
the general position of the planet, and Le Verri-
was resolved in 1915 by Albert Einstein’s new
with than general relativity, and gives sufficiently
er’s calculations are what led Johann Gottfried
theory of general relativity, which accounted
accurate results for most applications involving suf-
Galle to the discovery of Neptune.
for the small discrepancy in Mercury’s orbit.
ficiently small masses, speeds and energies.
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5.0 Grid
When we look into the Universe today, we see that pretty much every large galaxy has a supermassive black hole in its heart. Even the Milky Wayhas a black hole at its core with a mass of four millions times that of the Sun.
might start sometime, if something falls into it.
Before you start running around in circles and
Though we don’t know of anything that can fall
screaming, remember this: 1) it’s a long way
into it soon. But we might miss cold gas. Hmmm.
off, 26,000 light years (260 quadrillion kilometers), 2) its mass is still very small compared
Anyway, remember this as well: even though
to the 200 billion solar masses of our galaxy,
black holes can cause death and destruction
and therefore 3) it can’t really harm us. Unless
on a major scale, they also help galaxies them-
it starts actively feeding. Which it isn’t. But it
selves form! So we owe our existence to them.
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6.0 Identity
Fructus Genesis by Jason Blasso Before that old tree Fell the fruit The mind of Science Stooped and ’stood And weighted
Hurtled down
The gravity of it all
The seed of heresy
Then he held on high
Earth bound
The heavy pome
In fiery flight
And with hot hand
Until the new tree
Hurled down
Sprang raging into life
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8
G
G
G R AV I T Y
3
40
7
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G 12
5
11
7.0 Infographics
Gravitational Interaction If you are standing on a scale in a moving
Every one knows that objects fall because of
elevator, you would find your weight reading
gravity, even before Newton. Newton did not discover gravity, but discovered that gravity
The sensation of apparent weight comes from
would change —not when you are at the steady
is universal. It is the same force that pulls an
the support that you feel from the floor, from
motion but during accelerated motion. The
apple off a tree, holds the moon in orbit, and
a chair, etc. Different sensations of apparent
scale would show an increase of your weight
that both Earth and the moon are similarly held
weight can occur on an elevator since it is
when the elevator accelerate upward, and de-
in orbit around the sun. He also discovered that
capable of zero or constant speed (zero ac-
crease as it accelerate downward. If the eleva-
all objects in the universe attract each other.
celeration) and can accelerate either upward
tor cable broke and the elevator fell freely, the
The phenomenon of “weightlessness” occurs
or downward. If the elevator cable breaks then
scale reading would register zero; at this point
when there is no force of support on your body.
both you and the elevator are in free fall. The
you will feel weightless, because your insides
When your body is effectively in “free fall”,
resultant experience of weightlessness might
would no longer be supported by your legs and
accelerating downward at the acceleration
be exhilarating if it weren’t for the anticipation
pelvic region. The picture on the right show the
of gravity, then you are not being supported.
of the quick stop at the bottom.
weight and weightlessness in an elevator.
43
eleva tor stopped
elevator up
elevator down
(a =0)
(a=g)
(a=-g)
mg
W=mg
mg
mg
W=2mg
mg
-mg
W= 0
Be Less Heavy-Handed G RAVITY BAS I C S Every particle of matter in the universe attracts every other particle with a force that is directly proportional to the product of the masses of the particles and inversely prop ortional to the s qua r e of the di s t a nce betw e e n t h e m . In other w ord s , two bodi es of ma s s es m1 a nd m2 , s e p a r ated b y a d is t ance r , a ttr a ct ea ch other w i th a f o rc e F t h a t is p rop ortional to ( m1 x m2 ) / r 2 . The cons t a nt o f p ro p o rt ionality is know n a s the gr a vi t a ti ona l cons t a nt ( N e w t o n ' s c ons t ant), and is a l w a ys denoted by the l etter G .
We c a n t h e n e x p re s s t h e l a w o f g ra vi ty as
F= Gm m 1
r2
Th e va l u e o f G ha s b e e n m e a s u r e d i n e x t r e m e l y d e l i c a t e l a b o ra t o r y e x p e r i m e nt s . I n S I u n i t s , i t s va l u e i s 6. 67 x 1 0 - 1 1 n e w t on m e t e r 2 / k i l og ra m 2 .
G RAVITATI O NAL F I E LD I N S I D E A B O O K t humb ma s s
2
So now tha t you h a v e t h e b a s i c s d o w n l e t ’ s h a v e s o m e fun. U s e the for ce o f y o u r i m a g i n a t i o n t o s u s p e n d t h e ea r th’ s gr a vi t a ti on a l p u l l o n h o l d a n d l e t ’ s o n l y l o o k a t the gr a vi ty for ces b e t w e e n y o u r h a n d s a n d t h i s b o o k . Wi th your ha nds h o l d i n g t h e b o o k t h e e n t i re m a s s o f t h e book i s a ttr a cti ng y o u r h a n d s . I f you move them t o t h e m i d d l e o f t h e p a g e y o u w i l l exper i ence ha l f th e w e i g h t b e c a u s e t h e o u t s i d e o f t h e pa ges a r e pul l i ng i n a n e q u a l a n d o p p o s i t e d i re c t i o n a s the i ns i de pa r t of t h e p a g e .
G RAVI TAT I O NAL F I E LD I N S I D E A P L A N ET I f y o u co u l d f al l f rom th e N orth pol e strai gh t to t he S o ut h p o l e th i s i s wh at wou l d h ap p e n : A t th e beginning o f t he fa l l , th e gravi t ati on al f i e l d stre n gth an d your a ccel er a t ion are g, bu t you ' d f i n d th e y ste adi ly decr ease a s y o u co n ti n u e toward th e c e n te r of Earth . You ar e b ei ng p ul le d " d own ward" toward Earth ' s c e n t er, you ar e a l s o b ei ng pu l l e d " u pward" b y th e part of Ear t h t hat is "a b o v e" y ou . In f ac t, wh e n you ge t to th e c e nt er of E a r t h, t he pu l l " down " i s bal an c e d by th e pu l l "up". Yo u a r e p ul l ed i n e ve ry di re c ti on e q u al l y so th e n et for ce on y o u i s z er o. Th e re i s n o ac c e l e rati on as you w hiz wit h ma xi mum s p e e d past th e c e n te r of Earth .
R = 7� d i s tan ce fro m h an d at ed g e to cen ter o f b o o k = fu l l wei g h t t hum b mass
R= 3 . 5 � mov e h a n d he re to ex p eri en ce ha l f t h e w e i gh t (@ h al f th e d i s tan ce)
at the e xa c t c en t e r p oi n t y our h a n d is w eig ht l e s s (bliss in t h e g u t t e r )
Black Tidal S pa ghetti
= g
S ome thi ngs to k now : 1 . G RAV I TY B AS I C S gr a vi ty depends on di s t a n c e s o . . . the fa r ther a w a y you a re = t h e w e a k e r t h e g ra v i t y 2 . B LAC K H O LE S bl a ck hol es a r e ver y c o m p a c t e d , d e n s e m a t t e r you ca n get ver y cl os e t o t h e m b e c a u s e o f t h i s 3 . TI DAL FO R C E [ di ffer e n t i a l ] the cha nge of gr a vi ty o v e r d i s t a n c e
l on g object
mass
(le ss g) (mo r e g)
d ist ance f rom mass
’s G
A
EVENT HOR I ZON escape Ve l o c i ty = s p
of li gh
t
No o ne can hear you. Sp eed o f so u n d is m u ch too slow to escap e. No eye- wit nesses eit her. Ever y th in g th at happ en s in side th e ho r izo n is fo r ever invisible.
h
e in G fo rce
= 1 00s of m illio
hhh h h h hhh h h hh hh h
ns o f X’s eart h
hh
eed
h
h h
h h
renc
h
h h
diffe
h
h
h
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W hat ’ s g o i n g o n h e r e ? ! ?
h h h
B l a ck h o l e s a re v e ry s m a l l . . .
h h
So y o u c a n g e t V E RY c l o s e t o t h e m
h h
Th a t m a k e s t h e t i d a l f o rc e C R A Z Y, l i k e d i s t re s s i n g l y b i g
h h h h h
t h e f o rc e i s s o s t ro n g t h a t y o u r f e e t g e t y a n k e d a way f ro m y o u r h e a d a t h u n d re d s o f m i l l i o n s o f t i m e s t h e f o rc e o f e a rt h ’ s g ra v i t y
h
y o u ’ d b e s t re t ch e d i n t o a l o n g , t h i n s t rand a n d t h e n s h re d d e d
B L AC K H O LE
a s t ro n o m e rs c a l l t h i s s p a g h e t t i fi cati on!
8.0 Paper Composition
The Principle of Superposition The fact that the total gravitational field is just given by adding the two vectors together is called the Principle of Superposition. This may sound really obvious, but in fact it isn’t true for every force found in physics: the strong forces
fields from all the individual masses. Newton
between elementary particles don’t obey this
used this to prove that the gravitational field
principle, neither do the strong gravitational
outside a solid sphere was the same as if all
fields near black holes. But just adding the
the mass were at the center by imagining the
forces as vectors works fine for gravity almost
solid sphere to be composed of many small
everywhere away from black holes, and, as you
masses—in effect, doing an integral, as we
will find later, for electric and magnetic fields
shall discuss in detail later. He also invoked su-
too. Finally, superposition works for any num-
perposition in calculating the orbit of the Moon
ber of masses, not just two: the total gravita-
precisely, taking into account gravity from both
tional field is the vector sum of the gravitational
the Earth and the Sun.
49
Newton’s laws explain the paths of objects moving
etary motions. But they do much more than that.
at any point in space near any gravitating body.
Newtonian gravitation governs not only the planets,
These laws provide a firm physical and mathematical
moons, and satellites in their elliptical orbits but also
foundation for Copernicus’s heliocentric model of
the stars and galaxies in their motion throughout our
the solar system and for Kepler’s laws of plan-
universe—as well as apples falling to the ground.
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53
We can all relate to feeling the weight of something on our shoulders or having a heavy heart. We all feel the effects of gravity, whether it’s physically, emotionally or psychologically.
9.0 Word Play
To his Coy Mistres s by Andrew Mar vell
Had we but world enough, and time, This coyness, lady, were no crime. We would sit down and think which way To walk , and pass our long love’s day; Thou by the Indian Ganges’ side Shouldst rubies find ; I by the tide O f Humber would complain. I would
Now therefore, while the youthful hue
Love you ten years before the Flood ;
Sits on thy skin like morning dew,
And you should, if you please, refuse
But at my back I always hear
And while thy willing soul transpires
Till the conversion of the Jews.
Time’s winged chariot hurr ying near;
At ever y pore with instant fires,
My vegetable love should grow
And yonder all before us lie
Now let us spor t us while we may;
Vaster than empires, and more slow.
Deser ts of vast eternit y.
And now, like am’rous birds of prey,
An hundred years should go to praise
Thy beaut y shall no more be found,
Rather at once our time devour,
Thine eyes, and on thy forehead ga ze;
Nor, in thy marble vault, shall sound
Than languish in his slow-chapp’d power.
Two hundred to adore each breast,
My echoing song ; then worms shall tr y
Let us roll all our strength, and all
But thir t y thousand to the rest ;
That long preser v’d virginit y,
Our sweetness, up into one ball ;
An age at least to ever y par t,
And your quaint honour turn to dust,
And tear our pleasures with rough strife
And the last age should show your hear t.
And into ashes all my lust.
Thorough the iron gates of life.
For, lady, you deser ve this state,
The grave’s a fine and private place,
Thus, though we cannot make our sun
Nor would I love at lower rate.
But none I think do there embrace.
Stand still, yet we will make him run.
he fruit — And with Fell t hot The tree ha m n old d H ind at ur of th le re s d und In fiery fo do cie arth bo E f l i Be ght w e— .T om h e yp m av in d he Bef o r et ha hen he held on hi t g h o T d—T he h ld too eav tr d ‘s he seed of heresy . y an wn T B e po f o ed do re m op led th e to urt a t ol eS H d ncn — t
weighted T d n A il fe. eighted The gr he w ife. And weig avi l ree Spra t d The tentailntgh rto flight. The min fiery d of sci en ce
t — And with ho t ha frui e h nd ll t v y a e p e h ethat old to F h e —Hur rem T e e e h r Fe Eal g o i re f he ll rt ooped an t h ony. B nce St d d ‘s e i c nodwHn Th hot hdad— ith meee held oun r high w h
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d In un bo
St
Hu rtl ed
do
g n a r r a p g S i n e e rt ging into life. g into ra ng raging intAnd praUntil wtheeignew o h ndll— U S p e din
it fru e th
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nd ‘stood — oped a Th Sto en ce h ien wn The seed o e he sc f d do l . The t h m i h t — of g tle e friu An ind o ere ur l th fl d fs s HFel iery —e nf
ee
all—Until f it tre the n y o e new e Spra ew l th e new tree ng l th f it all— S o y ife l ntoof it.aA wg.intnrge odse— e Tv ynu a heH ‘stTohe hned— port l nd e ow
ith hot hand Hurled dw d An y. Before that ow res e — Earth old n — tr hepom b it o y c e n S f u e v t o nd e o ru eao f sci pe da I e hd o Th n do tled wn — u rle nderH am t hpo n highdTd h ho eld o
ll Fe
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weighted Th And f it a e gra vity o ll—U vit gra y of it all—U nti n e h g t T t r a i d hte raging vit ng ravniety i g le rAifea
ooped and ‘stood — The nh ce St n e eh i eld f sc o on d in hi m gh e Th Th o r f e e t B h . a y t s o e r l d e tree fh do Fe ll t see e he h T f n d — Then he held o o t w on d ‘s n h da fierty t. T igh lefdlidgohw pe n hTe d—InHur o n hm o e si w oun ee o b A d n — d d t wit i d u r e h f he e h h a e he vy — T Tehn h od to eeddown — H s e d u le
ith hot hand Hurled do wn nd w A — —
55
e fruit — And
h w Fell t tree ghted ith hot hThe T i a e h n old e w at gd Hmuind d th r r ledof s a re vd cie fo An arth bound In fiery e o n f h l t e i i Be g w —E l hw i t e t t . Th tr y om em e yp Un av in e S d Spra he n — g e p l l r ree a t g ith hot hand Hurled in r dw e t e d o w An y. Before thatS olw p ew resme — Eart — dn e o h p b it ou trr vf yh ence Stoo nd e an ru eao f sci pe ehn f o i o t d e d a a I y ll t Th n ed down vi erH—tln u g i d i r n l e am t hpoag n highdTd n h d o Th ho l e ed ll eaen
The gravity d e t of h g it ei t all—Until th a e i of it all—Until ne th f h e T o ed gra ht prang S ight r e f it otreh
B Until the ne efore th w hen he held on high ll— The d—T t at old r h stoo ‘a e d o e f h e a r e esi g nd wn The se in y.n at Be to l vy p etr g i f o ed i do f a re e r opf led th . ome S to rt a g A t Hu o eS o A . e n ld f n i n l ncn — d t w ra to d— e T g ionped anad ‘gstoion Sto hi i enn ce h ien g sc gtlerdedforiwughintt.—TThhteesimeeid of heteheol l of d ur l th fl nAndl nt h of res HFel iery U es —e nf — i l f e o t r a. e—geU w odse— e Tv ynu a heH ‘stTohe hned— port l nd e ow
hanidn Hut hotg rlo hn g ed do iti lwifn e— . w a d n r A — g HuA it n ru rtl n f T d h e ed d e t hrea t . h T g i h l t e f h g m y ind do w ier g ll r f i e n o a I f sc F p d v ne e i u en e bo e g ce it h r a th w T v r St y d i Ea d e t n d A w i — t h tuit ndhw y — ot h e fr an hh A t l g d .h Theethhaetaovlyd ptoremeee —iHgur el e eF f e Fe Eal g r ion h. Bi efocreeSw ll rt d ar toopet e t n h e d y n n d ‘s e i d c nownw A T d— h ndy t ho eediat Hounh i ldl t et hig ith v h r m h w nhe
ooped and ‘stood — The nh ce St n e eh sci eld f o on d in hi m gh e h Th T sy. Before that old e r e tree of h Fe eed ll t s e he h T f Then he he n — d o ld o w ‘sto n d an fdlight. high fuierrty ed e l downTh n I p H Tehm nd— oo n u e si w o ee o b d — And w d t i d u i t r e h f e h Then e heav d — Th he h y o to eed wn — H e s d do u le
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ou
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rm om en ti nt o S e t me fre e, leave m e be. I do n't He re I am an wan dI t to S . e o n m eth st go fal m i ' a n I n g la t ign. You hold m al d s not ew e n ou r r e w i o th he ly om Il
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10.0 Environment
Gravity depends on distance. The farther you are from an object, the weaker its gravity. So if you have a long object near a massive one, the long object will feel a stronger gravitational force on the near end versus a weaker force on the far end! This change in gravity over distance is called the tidal force (which is a bit of a misnomer, it’s not really a force, it’s a differential force, and yes, it’s related to why we have ocean tides on Earth from the Moon).
59
60
Gravity Lyrics by Sara Bareilles Something always brings me back to you. It never takes too long. No matter what I say or do, I still feel you here till the moment I’m gone. You hold me without touch. You keep me without chains. I never wanted anything so much than to drown in your love and not feel your rain. (chorus) Set me free, leave me be. I don’t want to fall another moment into your gravity. Here I am and I stand so tall, just the way I’m supposed to be. But you’re on to me and all over me.
65
This book was printed on Epson 4 Star Preminum Presentation Paper, Matte Double-sided in San Francisco, California. Fonts include Berthold Akzidenz Grotesk Regular, Italic and Medium