This document provides an overview of physics concepts related to motion. It discusses key topics including:
- The definition of physics as the study of objects and their interactions through observation, prediction, and experimentation.
- Isaac Newton's three laws of motion and law of universal gravitation, which describe how forces cause motion or changes in motion.
- Other motion concepts like position, velocity, acceleration, mass, and examples of how these principles apply to everyday situations like driving a car.
- How forces balance in static situations according to Newton's third law, and examples of centripetal force allowing circular motion.
First Law of Motion: The Law of Inertia
An object at rest tends to stay at rest, and an object in motion tends to stay in motion with the same speed and in the same direction, unless acted upon by an external net force (unbalanced force)
First Law of Motion: The Law of Inertia
An object at rest tends to stay at rest, and an object in motion tends to stay in motion with the same speed and in the same direction, unless acted upon by an external net force (unbalanced force)
Cleaning the place of work is cheaper than the long run psychological effects of the unclean place of work. The psychological impact associated with untidy environment might seem a little task, but it may have very dangerous effects if it's not addressed promptly. Visit to get more info http://www.homebuildingandloan.net/
Cleaning the place of work is cheaper than the long run psychological effects of the unclean place of work. The psychological impact associated with untidy environment might seem a little task, but it may have very dangerous effects if it's not addressed promptly. Visit to get more info http://www.homebuildingandloan.net/
Mirror - Physics by: Rey San Andrew RimandoRey Rimando
In this PowerPoint Presentation, you will find related topics with explanation like the Three Types of Mirror; it's characteristics and functions. Attached also is the video presentation used under the hyperlink(UNDERLINED WORDS). I'm hoping this will help a lot of students. Thanks! -Rey
The combination of Bayesian statistics and neural networks has proven to excel in predictive analytics. Blue Yonders solution NeuroBayes was developed and applied first in the field of particle physics but it can be successfully applied to a broad range of everyday problems for example demand prediction in retail. In this talk we introduce the basic concepts and explain the structure, components, and operations that build up an application for prediction.
Force and Mass;
Types of Forces;
Contact forces;
Field forces;
Newtons laws of motion;
Explanation;
It’s not Newton’s Laws;
Its Rishi Kanad laws;
Proof of stolen three laws of motion; how newton theft the laws ?
newton a modern thief?
laws of motion by Rishi Kanad
Vaisheshika - laws of motion
Comparision - Kanad rishi vs Newton
References for theft
Newton's First Law of Motion: I. Every object in a state of uniform motion tends to remain in that state of motion unless an external force is applied to it. This we recognize as essentially Galileo's concept of inertia, and this is often termed simply the "Law of Inertia".
Nutraceutical market, scope and growth: Herbal drug technologyLokesh Patil
As consumer awareness of health and wellness rises, the nutraceutical market—which includes goods like functional meals, drinks, and dietary supplements that provide health advantages beyond basic nutrition—is growing significantly. As healthcare expenses rise, the population ages, and people want natural and preventative health solutions more and more, this industry is increasing quickly. Further driving market expansion are product formulation innovations and the use of cutting-edge technology for customized nutrition. With its worldwide reach, the nutraceutical industry is expected to keep growing and provide significant chances for research and investment in a number of categories, including vitamins, minerals, probiotics, and herbal supplements.
DERIVATION OF MODIFIED BERNOULLI EQUATION WITH VISCOUS EFFECTS AND TERMINAL V...Wasswaderrick3
In this book, we use conservation of energy techniques on a fluid element to derive the Modified Bernoulli equation of flow with viscous or friction effects. We derive the general equation of flow/ velocity and then from this we derive the Pouiselle flow equation, the transition flow equation and the turbulent flow equation. In the situations where there are no viscous effects , the equation reduces to the Bernoulli equation. From experimental results, we are able to include other terms in the Bernoulli equation. We also look at cases where pressure gradients exist. We use the Modified Bernoulli equation to derive equations of flow rate for pipes of different cross sectional areas connected together. We also extend our techniques of energy conservation to a sphere falling in a viscous medium under the effect of gravity. We demonstrate Stokes equation of terminal velocity and turbulent flow equation. We look at a way of calculating the time taken for a body to fall in a viscous medium. We also look at the general equation of terminal velocity.
Slide 1: Title Slide
Extrachromosomal Inheritance
Slide 2: Introduction to Extrachromosomal Inheritance
Definition: Extrachromosomal inheritance refers to the transmission of genetic material that is not found within the nucleus.
Key Components: Involves genes located in mitochondria, chloroplasts, and plasmids.
Slide 3: Mitochondrial Inheritance
Mitochondria: Organelles responsible for energy production.
Mitochondrial DNA (mtDNA): Circular DNA molecule found in mitochondria.
Inheritance Pattern: Maternally inherited, meaning it is passed from mothers to all their offspring.
Diseases: Examples include Leber’s hereditary optic neuropathy (LHON) and mitochondrial myopathy.
Slide 4: Chloroplast Inheritance
Chloroplasts: Organelles responsible for photosynthesis in plants.
Chloroplast DNA (cpDNA): Circular DNA molecule found in chloroplasts.
Inheritance Pattern: Often maternally inherited in most plants, but can vary in some species.
Examples: Variegation in plants, where leaf color patterns are determined by chloroplast DNA.
Slide 5: Plasmid Inheritance
Plasmids: Small, circular DNA molecules found in bacteria and some eukaryotes.
Features: Can carry antibiotic resistance genes and can be transferred between cells through processes like conjugation.
Significance: Important in biotechnology for gene cloning and genetic engineering.
Slide 6: Mechanisms of Extrachromosomal Inheritance
Non-Mendelian Patterns: Do not follow Mendel’s laws of inheritance.
Cytoplasmic Segregation: During cell division, organelles like mitochondria and chloroplasts are randomly distributed to daughter cells.
Heteroplasmy: Presence of more than one type of organellar genome within a cell, leading to variation in expression.
Slide 7: Examples of Extrachromosomal Inheritance
Four O’clock Plant (Mirabilis jalapa): Shows variegated leaves due to different cpDNA in leaf cells.
Petite Mutants in Yeast: Result from mutations in mitochondrial DNA affecting respiration.
Slide 8: Importance of Extrachromosomal Inheritance
Evolution: Provides insight into the evolution of eukaryotic cells.
Medicine: Understanding mitochondrial inheritance helps in diagnosing and treating mitochondrial diseases.
Agriculture: Chloroplast inheritance can be used in plant breeding and genetic modification.
Slide 9: Recent Research and Advances
Gene Editing: Techniques like CRISPR-Cas9 are being used to edit mitochondrial and chloroplast DNA.
Therapies: Development of mitochondrial replacement therapy (MRT) for preventing mitochondrial diseases.
Slide 10: Conclusion
Summary: Extrachromosomal inheritance involves the transmission of genetic material outside the nucleus and plays a crucial role in genetics, medicine, and biotechnology.
Future Directions: Continued research and technological advancements hold promise for new treatments and applications.
Slide 11: Questions and Discussion
Invite Audience: Open the floor for any questions or further discussion on the topic.
Observation of Io’s Resurfacing via Plume Deposition Using Ground-based Adapt...Sérgio Sacani
Since volcanic activity was first discovered on Io from Voyager images in 1979, changes
on Io’s surface have been monitored from both spacecraft and ground-based telescopes.
Here, we present the highest spatial resolution images of Io ever obtained from a groundbased telescope. These images, acquired by the SHARK-VIS instrument on the Large
Binocular Telescope, show evidence of a major resurfacing event on Io’s trailing hemisphere. When compared to the most recent spacecraft images, the SHARK-VIS images
show that a plume deposit from a powerful eruption at Pillan Patera has covered part
of the long-lived Pele plume deposit. Although this type of resurfacing event may be common on Io, few have been detected due to the rarity of spacecraft visits and the previously low spatial resolution available from Earth-based telescopes. The SHARK-VIS instrument ushers in a new era of high resolution imaging of Io’s surface using adaptive
optics at visible wavelengths.
Seminar of U.V. Spectroscopy by SAMIR PANDASAMIR PANDA
Spectroscopy is a branch of science dealing the study of interaction of electromagnetic radiation with matter.
Ultraviolet-visible spectroscopy refers to absorption spectroscopy or reflect spectroscopy in the UV-VIS spectral region.
Ultraviolet-visible spectroscopy is an analytical method that can measure the amount of light received by the analyte.
What is greenhouse gasses and how many gasses are there to affect the Earth.moosaasad1975
What are greenhouse gasses how they affect the earth and its environment what is the future of the environment and earth how the weather and the climate effects.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
The ability to recreate computational results with minimal effort and actionable metrics provides a solid foundation for scientific research and software development. When people can replicate an analysis at the touch of a button using open-source software, open data, and methods to assess and compare proposals, it significantly eases verification of results, engagement with a diverse range of contributors, and progress. However, we have yet to fully achieve this; there are still many sociotechnical frictions.
Inspired by David Donoho's vision, this talk aims to revisit the three crucial pillars of frictionless reproducibility (data sharing, code sharing, and competitive challenges) with the perspective of deep software variability.
Our observation is that multiple layers — hardware, operating systems, third-party libraries, software versions, input data, compile-time options, and parameters — are subject to variability that exacerbates frictions but is also essential for achieving robust, generalizable results and fostering innovation. I will first review the literature, providing evidence of how the complex variability interactions across these layers affect qualitative and quantitative software properties, thereby complicating the reproduction and replication of scientific studies in various fields.
I will then present some software engineering and AI techniques that can support the strategic exploration of variability spaces. These include the use of abstractions and models (e.g., feature models), sampling strategies (e.g., uniform, random), cost-effective measurements (e.g., incremental build of software configurations), and dimensionality reduction methods (e.g., transfer learning, feature selection, software debloating).
I will finally argue that deep variability is both the problem and solution of frictionless reproducibility, calling the software science community to develop new methods and tools to manage variability and foster reproducibility in software systems.
Exposé invité Journées Nationales du GDR GPL 2024
Comparing Evolved Extractive Text Summary Scores of Bidirectional Encoder Rep...University of Maribor
Slides from:
11th International Conference on Electrical, Electronics and Computer Engineering (IcETRAN), Niš, 3-6 June 2024
Track: Artificial Intelligence
https://www.etran.rs/2024/en/home-english/
Professional air quality monitoring systems provide immediate, on-site data for analysis, compliance, and decision-making.
Monitor common gases, weather parameters, particulates.
1. 16/09/2013
1
Physics in Everyday Life
The Physics of Motion
Andrew Robinson
What is Physics?
• The study of objects and their interactions
• Observational science – why do things work
they way they do
• Predictive science – mathematical models are
developed to predict behaviour
• Experimental science – mathematical models
are tested to see if they reflect reality
• If they do and are accepted as a generally
robust model, then they become a Theory
Physics is Everywhere
• By looking around our
surroundings, we can see lots
of physics happening
• There is also lots of physics
happening which our own
senses cannot detect
Course Objectives
• To show you physics at work around us
• To explain why some things we observe
happen the way they do
• To show you that physics does not need
complicated mathematics to be
understandable
• To make you think
Describing
Motion
Position
Displacement
Velocity
(and Speed)
Acceleration
Position
• Where are we?
• To describe position, we need a Reference
Point, sometimes called the Origin
Equator
Greenwich Meridian
2. 16/09/2013
2
• René Descartes
• The Cartesian Coordinate System
Describing
Motion
Position
Displacement
Velocity
(and Speed)
Acceleration
Velocity and Speed
• These are similar concepts, the rate of change
of distance with respect to time
• In Physics there is a distinction between
velocity and speed
• Velocity is the speed, but also has a
designated direction
– This is an example of a vector quantity
• I drove at 80 km/hour describes a speed
• I drove due North at 80 km/hour describes a
velocity
Acceleration
• The rate of change of velocity
• How much faster are we getting?
– Accelerating
• How much slower are we getting?
– Decelerating The concept of
separate velocity and
acceleration is a
difficult one to
visualise
• A vehicle with a higher acceleration travels
further in any given time
• At the end of that time it has a higher speed
than the vehicle with the lower acceleration
3. 16/09/2013
3
The Aristotelians
• The Greek Scholar Aristotle considered what
made objects move
• He stated that an object required a Force to
keep it moving
• This definition of a “Force being an agent
causing motion” lasted until the Renaissance
period in western Europe.
Observe
Form
Hypothesis
Perform
Experiment
Compare
Observation
with
Experiments
Reject or
Accept
Hypothesis
The Great Greek
thinkers failed to
develop the
Scientific Method
• Aristotle did not test his theory of motion with
experiments.
• Nevertheless, his ideas on force and motion
dominated Western science for thousands of
years.
Vincenzo Galilei
and the Scientific Method
• Vincenzo Galilei (1520-1591)
was an accomplished Lutenist
and composer.
• He produced the first
description of how the tension
in a lute string changed the
pitch of the note.
• He did experiments, analysed
the results and produced a
mathematical formula to
describe the relationship
Galileo Galelei
• Vincenzo’s son Galileo applied the scientific
method to the study of motion
• His experiments, some rolling marbles down
slopes and others, clearly distinguished
between velocity (speed) and acceleration
• Some of his results contradicted Aristotle and
were very controversial
• Aristotle had hypothesized
that the heavier an object,
the faster it would fall
• Galileo dropped
cannonballs of different
weight from the top of the
leaning tower of Pisa.
• They hit the ground at the
same time!
4. 16/09/2013
4
Isaac Newton and the Laws of Motion
• In 1686, the English scientist
Isaac Newton, took work on
motion by Galileo and
Descartes, added his own
observations and
formulated three laws of
motion and a law of gravity
which describe most
observable motion.
The First Law of Motion
• An object continues at constant speed in a
straight line (i.e. at constant velocity) unless
acted on by an external force.
The natural state of
nature is either no
motion or motion in a
straight line with
constant speed
Aristotle was
wrong! Aristotle
assumed that
objects were
stationary when
no force was
exerted
The Second Law of Motion
• The force required to change the velocity of
an object is proportional to the mass of the
body and the acceleration
• 𝐹𝑜𝑟𝑐𝑒 = 𝑚𝑎𝑠𝑠 × 𝑎𝑐𝑐𝑒𝑙𝑒𝑟𝑎𝑡𝑖𝑜𝑛
𝐹𝑜𝑟𝑐𝑒 = 𝑚𝑎𝑠𝑠 × 𝑎𝑐𝑐𝑒𝑙𝑒𝑟𝑎𝑡𝑖𝑜𝑛
• If you apply more force to an object, it
accelerates more
So What is Mass?
• Sometimes called Inertia or Inertial Mass
• The resistance of a body to a force – a large
mass will resist a force more than a small
mass, and produce a smaller change in motion
(the acceleration)
Dictionary Definition:
inertness, especially with regard to effort, motion, a
ction, and the like; inactivity; sluggishness.
Mass and Weight
• Don’t confuse them!
• In physics, a weight is a force due to gravity
acting on a mass
• The mass is constant
• The weight depends where you are in the
universe
5. 16/09/2013
5
Walking On The Moon
• On the Moon, the gravitational force is a sixth
that on Earth
• The astronauts from Apollo 17 (Gene Cernan
and Harrison Schmitt) weigh less than they do
on Earth
• Their inertia (mass) is still the same
http://www.youtube.com/watch?v=wo3-fuYKWB4
Video: NASA
The Third Law of Motion
• When a force is exerted on an object, the
object exerts an equal and opposite force
back.
• Known as the Reaction Force
• This law is sometimes quoted as
• “Action and reaction are equal and opposite”
How Do We See It In Action?
• The Third Law was Newton’s major
contribution to development of the laws of
motion.
• If you push on an object, the object pushes
back on you with an equal force which is in
the opposite direction
“Child pushing Grandmother on tricycle”
Boy pushes
grandmother
Grandmother’s back
pushes on boy’s hands
Gravity pulls
down on
grandmother,
pushing her
towards the floor
Floor pushes back
on grandmother,
stopping her from
sinking into the
ground
Forces Can Cancel Out
• Force is a vector quantity (with magnitude and
direction).
• Vector quantities can be added together, so
that they cancel each other out, and the net
effect is zero
6. 16/09/2013
6
Vase with Irises (Van Gogh, 1890)
We know gravity is
pulling the vase down:
things fall towards the
Earth
Why doesn’t the vase
fall through the table?
The table pushes back on the vase, with a force equal to
the force of gravity. There is no force, no acceleration,
and a stationary object remains stationary
• In a tug of war contest, the teams are pulling
on the rope in opposite directions
• If both teams are evenly matched, then the
two forces exerted on the rope are equal and
opposite. They cancel out.
• There is no net force on the rope, so the rope
does not change its motion
• If the rope was stationary, it remains
stationary
• If one team is slightly stronger than the other, the
forces do not cancel out, and there is a small
force acting on the rope in the direction that the
stronger team are pulling
• Newton’s Second Law says that if there is a force,
then there must be acceleration.
• The stationary rope must start to move in the
direction of the acceleration
• Adding force vectors and cancelling them out
works with any number of vectors
If each of these
three force vectors
are equal, the net
force is zero
Engine Thrust
Air
resistance
(drag)
Lift
Aircraft Climbing
Gravity
• This is a free body diagram, it shows the
main forces acting on the aircraft
7. 16/09/2013
7
Gravity
• In the Principia Newton also
formulated a Law Of Gravity
to describe the easily
observable fact that things
fall down towards the
surface of the Earth
Apple tree at
Woolsthorpe Manor,
Grantham, where
Newton formulated the
Law of Gravitation
Newton’s Law of Gravity
• The gravitational force is exerted between any
two masses and depends on the value of each
of the masses.
• It also gets weaker with distance
With distance
squared to be exact
Kepler’s Laws
• Newton’s Law of Gravitation was able to
explain the earlier observations of planetary
motion made by Johannes Kepler (1571-1630)
Earth Blue
Mars Red
• Earth and Moon
seen from the
Galileo Probe
• Earth attracts the
Moon
• Moon attracts the
Earth
• The forces are
equal and opposite
Lunar Tides
• The gravitational pull of the moon is one of
the two contributing factors to explaining
tides in the seas and oceans
• The gravitational
pull of the sun is
the other
influencing factor
8. 16/09/2013
8
Circular Motion
• If the Earth and
Moon are pulling
on each other,
why don’t they
collide?
Direction of Velocity for a Rotating
Object
• The velocity vector is always at a tangent to
the spinning object
• The velocity vector is always at a tangent to
the spinning object
• So the vector points in a different direction
• This counts as a change in velocity over time
This is a
definition of
acceleration
• A rotating object is always subjected to a
force, because its velocity is always changing
• The force always acts to push the object into a
circular path – it is always towards the centre
Centripetal Force
• From Latin centrum
"centre" and petere
"to seek“
• The Centripetal force
is any force which
always acts to make
an object move in a
circular path
Where Does the Centripetal Force
Come From?
• It is not a new force of
nature, it has to come from
a force which is already
acting on the object
Bolas: South American Lasso
9. 16/09/2013
9
• For a ball on a string, it’s the tension force in
the taut string that pulls the ball around in a
circle
Tension Force
• For the moon going
round the sun, it’s gravity
that provides the
centripetal force
Gravitational Force
Turning a Corner in Your Car
Canadian Grand
Prix 2006,
Montreal
You turn in a
circular path, so
where does the
centripetal force
come from?
• Sideways friction forces from the tires (tyres)
provides the centripetal force
• If the friction force is not sufficient to hold you
in the circle, then you slide off the road
Ice
Slide off, if
there is not
enough
centripetal
force
• Whether friction can generate sufficient force
to hold you on the road depends on
1. The speed you are going – there is a
maximum safe speed
2. The radius of the turn (tighter turns – must
go slower)
3. How good your tires are (tread and rubber
compound)
4. The nature of the road surface – slippery
surfaces generate much less friction force
(ice, puddles of water)
10. 16/09/2013
10
Banked Turns
• In many cases of
turning, the object
turns more easily if
it is banked
• Why?
– If the turn is banked, then part of another force
can provide an extra contribution to the
centripetal force
– More force: easier to turn more quickly and in a
tighter turn
Friction
Weight
Force of road
pushing on car
• Centripetal force has contributions from
friction and normal force
• It is larger than it would be for a flat turn
• The car can take the banked turn faster than it
can take a flat turn
Centripetal
force
• There is a similar effect for aircraft, where
banking uses part of the lifting force
generated by the wings to provide centripetal
force
• The part of the lift force which is parallel to
the ground provides the centripetal force.
• The vertical part of the list force has to
counterbalance gravity, otherwise the plane
loses height!
gravity
11. 16/09/2013
11
Modes of Transport
• Moving ourselves around is mostly about
providing a force to push against something in
order to change our state of motion
The exception to this statement is the
rocket motor, which depends upon a
different physical principle, the
Conservation of Momentum. We will
discuss this principle in another class.
Sail Power
• We use the wind to provide a force
• The sails change the direction of the wind
velocity (which means the wind is accelerating
around the sail)
• The wind exerts a force on the sail
• The Sail exerts a force on the air. This force is
the one which moves the boat
http://www.phys.unsw.edu.au/~jw/sailing.html
• Wind changes direction
Force of sail on
air. The sail
pushes on the
air and this is
the force which
can move the
boat
Force on
air
making it
change
direction
• The force of the sail on the wind is applied to
the hull of the boat through the mast.
• The hull has a force on it, which changes its
motion
Propulsive
force, moves
the boat
forward
through the
water
Unwanted sideways force
• The sideways force (which is not wanted) is
counteracted by a drag force from the keel
under the hull
Sideways force
Propulsive forceDrag force
from keel
Drag force from water
Flettner Rotor Ship
• In the 1920’s the German engineer Anton
Flettner, used the Magnus effect to power
ships, by using wind power coupled to rotating
cylinders to generate a propulsive force more
efficiently than sails
Flettner Rotors
12. 16/09/2013
12
• The Flettner rotors were powered by low power
electric motors
Wind velocity
Force generated on rotor
Oar Power
• Use the oar to push on the water
• Newton’s Third Law, means that the water
pushes back on the oar.
• The oar is held by the crew, who sit in the
boat. The push of the water on the oar
propels the boat
Gondolas in Venice
• The oar pushes on the water
• The water pushes back on the oar
• This force is transmitted through the oar and
gondolier to the gondola
It actually depends on
the grip of the
gondolier’s shoes to the
deck!
Propellers or Paddlewheels
• The paddlewheel or propeller in a ship turns
and exerts a force on the water
• The water pushes back on the propulsion
system, moving the boat
Walking, Jogging or Running
• Our muscles move our skeletal
system so that we exert a force
on the road.
• The road pushes back on our
feet
• We move along
• Force is efficiently transferred to the ground if
there is plenty of grip
– A large friction force is applied between the
ground and the foot
– We wear shoes which are optimized to give good
grip in various conditions
13. 16/09/2013
13
• Wheelchair basketball (Canada vs Australia,
Sept 2012, Paralympics)
• Athlete pushes on the wheel
Wheel pushes on the floor
Floor pushes on the
wheel, wheelchair
moves forward
• To propel a car forward is similar, except that
the force to turn the wheel comes from the
engine
• Forward progress depends on there being
efficient transmission of force from wheel to
ground.
• This requires a large friction force.
– In slippery conditions, the wheel turns, but slips
on the road, and so no forward progress is made
Conclusions
• By studying motion, we can deduce many
things about the physical universe.
• We can see Newton’s Laws of Motion
operating all around us, even on objects which
do not appear to be moving.