Henrietta Leavitt Discovered That RR Lyrae Stars Pulsate... (2024)

Physics High School

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Answer 1

Henrietta Leavitt was an astronomer who discovered that RR Lyrae stars pulsate at a regular rate that is directly related to their intrinsic brightness. This relationship, known as the period-luminosity relation, allowed Leavitt to measure the distances to many stars in our Milky Way galaxy and beyond. Her work revolutionized our understanding of the size and structure of the universe and paved the way for future astronomical discoveries.

Why do RR Lyrae stars pulsate?

RR Lyrae stars pulse like Cepheid variables, but the nature and histories of these stars is thought to be rather different. Like all variables on the Cepheid fluctuation strip, pulsations are caused by the κ-mechanism, when the ambiguity of ionized helium varies with its temperature.

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a disk, a hoop, and a solid sphere are released at the same time at the top of an inclined plane. they are all uniform and roll without slipping. in what order do they reach the bottom? group of answer choices sphere, disk, hoop hoop, sphere, disk hoop, disk, sphere disk, hoop, sphere

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When a disk, a hoop, and a solid sphere are released at the same time at the top of an inclined plane, and they all roll without slipping, they will reach the bottom in the following order: solid sphere, disk, hoop.

An inclined plane is a simple machine that consists of a sloping surface that allows an object to be moved from a lower point to a higher point with less force than would be required to lift the object directly. The inclined plane reduces the amount of work required by increasing the distance over which the force is applied.

The mechanical advantage of an inclined plane is determined by the ratio of the length of the incline to its height. The longer the incline, the less force is required to move the object, but the longer the distance over which the force must be applied. The height of the incline also affects the mechanical advantage, with a steeper incline requiring less distance to cover but more force to move the object.

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What color wire do you always plug into the COM port?a. Blueb. Black c. Red

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The correct option is B. The color of the wire you should always plug into the COM port is Black.

This is a bit of a tricky question because the answer depends on what type of cable you are using and what you are connecting to the COM port. Generally speaking, the COM port (or serial port) uses a 9-pin connector and is used for serial communication. In terms of the color of the wire, there is no one specific color that is always plugged into the COM port. The wires in a serial cable can be different colors and the color coding may vary depending on the manufacturer. However, what is important is that the wire that is connected to pin 1 on the COM port (usually the top-left pin) is the one that is used for transmitting data. This wire is typically color-coded as either blue or black, but again, it can vary.

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Which illustrates tertiary prevention for child maltreatment?

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That counseling services for families affected by child maltreatment would be an example of tertiary prevention.

Tertiary prevention focuses on reducing the negative consequences of an already existing problem.

Counseling services can help address the emotional and psychological impact of child maltreatment on the child and the family, and can provide resources and support for healing and recovery.
The third level of prevention, following primary and secondary prevention. Primary prevention focuses on preventing child maltreatment from occurring in the first place, while secondary prevention focuses on early intervention and addressing risk factors before maltreatment occurs. Tertiary prevention is aimed at reducing the negative consequences of an already existing problem.

Hence, counseling services for families affected by child maltreatment illustrate tertiary prevention. This level of prevention focuses on reducing the negative consequences of an already existing problem and can provide resources and support for healing and recovery.

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As an object moves around, on which quantities does the change in its gravitational potential energy depend? a. Its mass b. Its change in speed c. The path of the motion d. Its change in height

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The change in an object's gravitational potential energy depends only on its change in height above a reference level and its mass. So the correct options are (a) and (d).

The gravitational potential energy is the energy that an object possesses due to its position in a gravitational field. It is directly proportional to the object's mass and the height of the object above the reference level.

As an object moves around, its gravitational potential energy changes based on its change in height above the reference level.

The object's change in speed and path of motion do not affect the gravitational potential energy, as these quantities do not directly relate to the object's position in the gravitational field.

Therefore, the change in gravitational potential energy of an object can be calculated as the product of its mass, the acceleration due to gravity, and its change in height above a reference level, and is independent of the object's path or speed.

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A proton of mass 1.67

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1.67 * 10−27 kg I think this is the mass

at equilibrium on a bathroom weighting scale, the downward pull of gravity on you is balanced by

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At equilibrium on a bathroom weighing scale, the downward pull of gravity on you is balanced by the upward force called the normal force.

When you stand on a weighing scale, your weight (downward force due to gravity) pushes down on the scale. The scale, in response, exerts an equal and opposite force, known as the normal force, which acts upward to balance the gravitational force.

This is in accordance with Newton's Third Law of Motion, which states that for every action, there is an equal and opposite reaction. At equilibrium, these forces are equal, and the scale measures your weight based on this normal force.

Bathroom scales for home use show your weight on a dial or a digital screen. These scales weigh you in one of two ways: mechanically, with springs, or electronically, with circuits that bend under weight, changing the current flowing through them.

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A 5. 0-cm-diameter coil has 20 turns and a resistance of 0. 50ω. A magnetic field perpendicular to the coil is B=0. 020t + 0. 010t2, where B is in tesla and t is in seconds.

- Find an expression for the induced current I(t) as a function of time.

- Express your answer in terms of the variable t.

- Evaluate I at t=10s.

- Express your answer using two significant figures

Answers

At t = 10 seconds, the coil's induced current is roughly -0.39 A.

We have a coil with 20 turns and a diameter of 5.0 cm. A magnetic field B with a resistance of 0.50 is perpendicular to the coil and is where the coil is located.

B = 0.020t + 0.010 t2, where t is measured in seconds and B is measured in tesla, is the formula for the magnetic field. We may calculate the induced current I(t) in the coil using Faraday's Law of Electromagnetic Induction.

To get the rate of change of the magnetic flux through the coil, multiply the magnetic field by the coil area. The induced emf can then be used to calculate the induced current I(t) in the coil. We can assess I(10). At t = 10 seconds, the coil's induced current is roughly -0.39 A.

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A soccer player who has the ball is being chased by 4 other players from the opposing team. the player with the ball is running east at 20 m/s. select the opposing player who has the same velocity as the player with the ball.
a. number 17 who is running at 17 m/s in the westward direction.
b. number 03 who is running at 20 m/s in the eastward direction.
c. number 13 who is running at 12 m/s in the eastward direction.
d. number 28 who is running at 20 m/s in the northward direction.

Answers

Option B, number 03 who is running at 20 m/s in the eastern direction. Among the given options, number 03 has the same velocity as the soccer player with the ball.


Since the player with the ball is running east at 20 m/s, the opposing player who has the same velocity must also be running at 20 m/s in the eastward direction.

Option B is the only choice that meets these criteria.
The opposing player who has the same velocity as the player with the ball is number 03 who is running at 20 m/s in the eastward direction.

Hence, Among the given options, number 03 has the same velocity as the soccer player with the ball.

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Predict how network modifiers affect the structure of a ceramic glass.

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Network modifiers affect the structure of a ceramic glass is that they can alter the glass's properties such as its melting point, density, and viscosity. Network modifiers are elements that are added to a glass to break up the network of bonds that hold it together.

In a ceramic glass, the atoms are held together by strong covalent bonds that form a network structure. This network structure gives the glass its strength and hardness. However, the network structure can also make the glass brittle and difficult to process. By adding network modifiers, the bonds between atoms are weakened, and the glass becomes more malleable and easier to process.
The addition of network modifiers to a ceramic glass can significantly alter its properties, making it easier to process and improving its overall performance. The specific effects of network modifiers will depend on the type and amount of modifier added to the glass.

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A solenoid has a net length of 2 m, a radius of 10 cm, and a current of 4 A running through it. The solenoid is comprised of 500 turns. What is the magnitude of the magnetic field in the solenoid?A) 0.2 T B) 0.4 T C) 0.6 T D) 1.0 T E)Â1.26ÂT

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The magnitude of the magnetic field in the solenoid is 0.0126 T is not among the given options, there might be a typo in the problem or the answer choices.

Please double-check the given data and choices.

To find the magnitude of the magnetic field in the solenoid, we'll use the formula for the magnetic field inside a solenoid:
B = μ₀ * n * I
Where B is the magnetic field, μ₀ is the permeability of free space (4π x 10⁻⁷ Tm/A),

n is the number of turns per unit length, and I is the current.
First, let's calculate the number of turns per unit length (n):
n = total turns / length = 500 turns / 2 m = 250 turns/m
Now, plug the values into the formula:
B = (4π x 10⁻⁷ Tm/A) * (250 turns/m) * (4 A)
B ≈ 0.004π T ≈ 0.012566 T ≈ 0.0126 T.

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Question: A solenoid has a net length of 2 m, a radius of 10 cm, and a current of 4 A running through it. The solenoid is comprised of 500 turns. What is the magnitude of the magnetic field in the solenoid?A) 0.2 T B) 0.4 T C) 0.6 T D) 1.0 T E)Â 1.26Â T

A solid aluminum cylinder with density equal to 2700 kg/m3 has the weight equal to 0.66 N in air and the apparent weight of 0.354 N when immersed in an unknown liquid. What is the density of the liquid?

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The density of the unknown liquid is 997 kg/m³.

To Calculate the volume of the solid aluminum cylinder using the weight and density provided.
Formula: Volume = Weight / (Density * gravity), where gravity is approximately 9.81 m/s².
Volume = 0.66 N / (2700 kg/m³ * 9.81 m/s²) ≈ 2.45 x 10⁻⁵ m³
Calculate the buoyant force acting on the cylinder when immersed in the liquid.
Buoyant force = Weight in air - Apparent weight in liquid
Buoyant force = 0.66 N - 0.354 N = 0.306 N
Use the buoyant force to find the density of the unknown liquid.
Formula: Buoyant force = Liquid density * Volume * gravity
Liquid density = Buoyant force / (Volume * gravity)
Liquid density = 0.306 N / (2.45 x 10⁻⁵ m³ * 9.81 m/s²) ≈ 997 kg/m³

Hence, Using this buoyant force, we determined the density of the unknown liquid to be 997 kg/m³.

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If human starts making it s own food in the body then what will happen

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Answer:

We will no longer have a need for other food sources, and driving to stores and fridges will be obsolete, we will need to work less, and carbon dioxide levels will fall.

Explanation:

a 4kg ball started rolling from rest on top of a 4m high ramp. what is the velocity of the ball at the bottom of the ramp?

Answers

The velocity of the ball at the bottom of the ramp is approximately 8.86 m/s.

To find the velocity of the 4kg ball at the bottom of the 4m high ramp, we can use the conservation of mechanical energy principle. Since the ball starts from rest, its initial potential energy (PE) is converted into kinetic energy (KE) at the bottom of the ramp.

Initial PE = m * g * h
where m = 4kg (mass), g = 9.81 m/s² (acceleration due to gravity), and h = 4m (height)

Initial PE = 4 * 9.81 * 4 = 156.96 J (joules)

At the bottom, the potential energy is converted into kinetic energy:
KE = 0.5 * m * v²
where v is the velocity we want to find.

Since the initial PE = KE at the bottom, we can write:
156.96 J = 0.5 * 4 * v²

Solve for v:
v² = (156.96 / (0.5 * 4))
v² = 78.48
v = √78.48
v ≈ 8.86 m/s

The velocity will be approximately 8.86 m/s.

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a nearsighted person has a far point that is 4.2 m from his eyes. what power contact lenses will allow him to focus on distant objects?

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A nearsighted person with a far point of 4.2m from his eyes would need contact lenses with a power of 4.2D to focus on distant objects.

To determine the power of contact lenses needed for a nearsighted person to focus on distant objects, we need to use the formula: power = 1/focal length. The near point of a nearsighted person is closer than infinity, so we need to use the reciprocal of the far point distance to calculate the focal length.
Focal length = 1/far point distance = 1/4.2m = 0.238m
Now we can calculate the power needed:
Power = 1/focal length = 1/0.238m = 4.2 diopters (D)
Therefore, a nearsighted person with a far point of 4.2m from his eyes would need contact lenses with a power of 4.2D to focus on distant objects.

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what is the explanation for the poor definition of the reflecting surfaces in the center of the cross section

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The poor definition of the reflecting surfaces in the center of the cross section can be attributed to a number of factors. One possible explanation is the quality of the materials used in the reflective surfaces themselves. If the mirrors or other reflective surfaces are not of high quality, they may not be able to reflect light as effectively, leading to a loss of definition in the reflection.

Another possible factor is the angle at which the light is hitting the reflective surfaces. If the angle is not optimal, the reflection may be distorted or fuzzy, reducing its clarity. Additionally, the surrounding environment may also play a role in the quality of the reflection. If there are other sources of light or reflective surfaces nearby, this can create unwanted reflections or glare, further reducing the clarity of the central reflection.

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Three objects, a solid sphere, a hollow ring, and a solid disk, have the same radius R. A string is wrapped around each object and the same tangential force is applied to each object at R and time t = 0 s. Which one of the following statements concerning the angular momentum of these objects after a short time t has elapsed, assuming the tangential force was continually applied? A. The angular momentum of the solid disk is larger than that of the other two objects. B. The angular momentum of the solid sphere is larger than that of the other two objects. C. The angular momentum of the hollow ring is larger than that of the other two objects D. The angular velocity of all of the objects has the same value. E. The angular velocity of the solid disk and hollow ring are equal, but that of the solid sphere is smaller.

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Option E: The angular velocity of the solid disk and hollow ring are equal, but that of the solid sphere is smaller.

This is because angular momentum depends not only on the radius but also on the mass distribution of the object. The solid sphere has more mass concentrated at the center, while the solid disk and hollow ring have more distributed mass.

Therefore, the solid sphere will have a smaller angular velocity than the other two objects when the same tangential force is applied.

In summary, the angular momentum of the solid sphere, solid disk, and hollow ring will be different due to their mass distribution, and the solid sphere will have a smaller angular velocity than the other two objects.

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drag the items on the left to the appropriate blanks on the right to complete the sentences. (not all items will be used.) resethelp collisions could result in gas being stimulated blank stars. it could also blank gas blank galaxies, through tidal interactions, ram pressure events, or (indirectly) by inciting more stellar winds and supernova.target 1 of 6target 2 of 6target 3 of 6 we expect collisions between galaxies to be relatively blank (while star-star collisions are blank) because the typical distance between galaxies is blank in scale to the size of the galaxies themselves.target 4 of 6target 5 of 6target 6 of 6

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Collisions could result in gas being stimulated to form new stars. It could also strip gas from galaxies, through tidal interactions, ram pressure events, or (indirectly) by inciting more stellar winds and supernova.

We expect collisions between galaxies to be relatively rare (while star-star collisions are common) because the typical distance between galaxies is much larger in scale to the size of the galaxies themselves. 1. Collisions could result in gas being stimulated to form stars. 2. It could also remove gas from galaxies, through tidal interactions, ram pressure events, or (indirectly) by inciting more stellar winds and supernova. 3. We expect collisions between galaxies to be relatively rare (while star-star collisions are even rarer) because the typical distance between galaxies is large in scale to the size of the galaxies themselves.

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A puck slides along a frictionless surface in the northward direction. An eastward impulse is applied to the puck. The change in momentum of the puck is in the ____ direction

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A puck slides along a frictionless surface in the northward direction. An eastward impulse is applied to the puck. The change in momentum of the puck is in the eastward direction.

This is because impulse, which is equal to the change in momentum, is applied in the eastward direction. Since there is no friction to oppose the motion, the puck will continue to move in the direction of the impulse with the same speed and in the new direction.

Impulse in Physics is a term that is used to describe or quantify the effect of force acting over time to change the momentum of an object. It is represented by the symbol J and usually expressed in Newton-seconds or kg m/s.

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when an object is allowed to fall freely near the surface of the earth, the gravitational pull is such that the object falls 16 ft in the first second, 48 ft in the next second, 80 ft in the next second, and so on. a. find the total distance a ball falls in 6 s.
b. find a formula for the total distance a ball falls in n seconds.

Answers

a) The total distance a ball falls in 6 seconds is 576 feet.

b) The formula for the total distance a ball falls in n seconds is:
S_n = 16n * (n + 1) / 2

a. To find the total distance a ball falls in 6 seconds, we need to sum up the distances it falls during each second. Based on the given information, the distances are:
1st second: 16 ft
2nd second: 48 ft
3rd second: 80 ft
We can observe a pattern here: the distance increases by 32 ft each second (16, 48, 80, 112, 144, 176). So, the distances for the remaining seconds are:
4th second: 112 ft
5th second: 144 ft
6th second: 176 ft

Now, we can sum up these distances: 16 + 48 + 80 + 112 + 144 + 176 = 576 ft. Therefore, the total distance a ball falls in 6 seconds is 576 feet.

b. To find a formula for the total distance a ball falls in n seconds, we can notice that the sequence of distances forms an arithmetic progression with the first term a = 16 and the common difference d = 32. The formula for the sum of the first n terms of an arithmetic progression is:

S_n = n * (2a + (n - 1)d) / 2

In our case, S_n represents the total distance a ball falls in n seconds. Plugging in the values for a and d, we get:

S_n = n * (2 * 16 + (n - 1) * 32) / 2

Simplifying, the formula for the total distance a ball falls in n seconds is:

S_n = 16n * (n + 1) / 2

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which answer gives the correct order of how sound waves are sensed and perceived? group of answer choices pinna, auditory canal, eardrum, ossicles, cochlea, auditory nerve, temporal lobe auditory canal, pinna, ossicles, eardrum, cochlea, auditory nerve, temporal lobe temporal lobe, auditory nerve, cochlea, eardrum, ossicles, pinna, auditory canal eardrum, auditory canal, cochlea, ossicles, auditory nerve, temporal lobe

Answers

The correct order of how sound waves are sensed and perceived is: pinna, auditory canal, eardrum, ossicles, cochlea, auditory nerve, temporal lobe.

The process begins with the pinna, which collects and funnels sound waves into the auditory canal. The sound waves then travel through the auditory canal and reach the eardrum, causing it to vibrate.

These vibrations are then transmitted to the ossicles, a group of three small bones in the middle ear. The ossicles amplify and transfer the vibrations to the cochlea, a fluid-filled, snail-shaped structure in the inner ear. The cochlea contains tiny hair cells that convert the vibrations into electrical signals, which are then transmitted to the auditory nerve.

Finally, the auditory nerve carries these electrical signals to the temporal lobe of the brain, where they are interpreted as sound. This entire process allows us to sense and perceive the various sounds we encounter in our daily lives, enabling us to communicate and navigate the world around us.

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Scallops eject water from their shells to provide a orce. The graph shows a smoothed graph of actual data for the initial motion of a 25 g scallop speeding up to escape a predator. What is the magnitude of the net force needed to achieve this motion? How does this force compare to the 0.25 N weight of the scallop? v (m/s) 0.3 0.2 0.1 0.0 - 1 (s) 0.0 0.1 0.2 0.3 FIGURE P4.20

Answers

The net force required to achieve this motion is approximately 0.1675 N, which is much smaller than the weight of the scallop (0.25 N). This makes sense because the scallop is not moving against gravity, but rather against the resistance of the water as it ejects it from its shell.

We can use the formula F=ma, where F is the net force, m is the mass of the scallop, and a is the acceleration of the scallop. From the graph, we can estimate that the scallop reaches a speed of approximately 0.3 m/s after 0.25 seconds. The initial velocity is zero, so the change in velocity is 0.3 m/s.

Using the kinematic equation v = at, where t is the time it takes to reach a speed of 0.3 m/s, we get:

0.3 m/s = a(t)

t = 0.3/a

Substituting this value of t into the kinematic equation x = 0.5at², where x is the distance the scallop travels during the time t, we get:

0.1 m = 0.5a(0.3/a)²

a = 6.7 m/s²

Now we can calculate the net force:

F = ma = (0.025 kg)(6.7 m/s²)

= 0.1675 N

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rifle is fired in a valley with parallel vertical walls. the echo from one wall is heard in 2.0 sec and the echo from the other wall is heard 2 sec later (4s after the rifle is fired). what is the width of the valley?

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If the echo from one wall is heard in 2.0 sec and the echo from the other wall is heard 2 sec later then the width of the valley is 3d/s

Let's call the distance from the rifle to one of the walls "d". Since the sound wave travels twice the distance to the wall and back, the total distance the sound travels before reaching the listener is 2d. Similarly, the distance from the rifle to the other wall is also "d", so the total distance the sound travels before reaching the listener from that wall is 2d as well.

Let's call the width of the valley "w". When the sound bounces off the walls, it has to travel an additional distance of "w" to reach the listener. Since sound travels at a constant speed (assuming no temperature variation), we can use the following formula to find the speed of sound:

v = d / t

where v is the speed of sound, d is the distance traveled by the sound, and t is the time it takes for the sound to travel that distance.

Using this formula, we can find the speed of sound for both echoes:

v1 = 2d / 2s = d / s

v2 = 2d / 2s = d / s

Since the time delay between the two echoes is 2 seconds, the total distance the sound traveled to reach the listener is twice the width of the valley:

2w = v2 (4s) - v1 (2s)

Simplifying the equation, we get:

2w = 2d / s (4s) - d / s (2s)

2w = 6d / s

w = 3d / s

Therefore, the width of the valley is 3d/s. We can't solve for "d" or "s" without additional information, but we can say that the width of the valley is proportional to the distance from the rifle to the wall and inversely proportional to the speed of sound.

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2. Noah places four books with the same mass on four shelves of a bookcase. Each book has gravitational potential
energy because of its height above the ground.
If each book falls from its position, which statement correctly compares the kinetic energy of the books just before
they hit the ground?
A. They will all have zero kinetic energy.
B. They will all have the same kinetic energy.
C. The book on the top shelf will have the greatest kinetic energy.
D. The book on the bottom shelf will have the greatest kinetic energy.

Answers

The book on the top shelf will have the greatest kinetic energy. Option C

Why would the book on the top shelf will have the greatest kinetic energy?

When Noah's books books fall from their locations, they turn gravitational potential energy into kinetic energy.

The more gravitational potential energy a book has, the higher it is above the earth. As a result, the book on the highest shelf has the most gravitational potential energy. As the book falls, it has the more kinetic energy immediately before it strikes the ground.

Kinetic energy can be described as a type of energy an object has, given to movement or motion.

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Can someone help me with this? It's on the Kepler's Second Law experiment. These two questions are the same for all the planets.
(You can prob look up the photo for them, but I don't fully get it)

Mercury:
1. What do you notice about each area?
2. Record any observation regarding the perihelion distance (Rp) and the aphelion distance (Ra).

Earth:
1. What do you notice about each area?
2. Record any observation regarding the perihelion distance (Rp) and the aphelion distance (Ra).

Mars:
1. What do you notice about each area?
2. Record any observation regarding the perihelion distance (Rp) and the aphelion distance (Ra).

Saturn:
1. What do you notice about each area?
2. Record any observation regarding the perihelion distance (Rp) and the aphelion distance (Ra).

Neptune:
1. What do you notice about each area?
2. Record any observation regarding the perihelion distance (Rp) and the aphelion distance (Ra).

Comet:
1. What do you notice about each area?
2. Record any observation regarding the perihelion distance (Rp) and the aphelion distance (Ra).

can anyone fully help me with Neptune?

1. What is the orbit of the Neptune?
2. Is the Sun at the center of the Nepturn’s orbit?
3. Describe the motion of Neptune throughout its orbit? Does it move at constant speed?
4. What do you notice about each area?
5. Record any observation regarding the perihelion distance (Rp) and the aphelion distance (Ra).

Answers

According to Kepler's Second Law, as a planet orbits the Sun, an imaginary line connecting them sweeps across the same amount of area at the same rate.

Mercury's orbit is shaped like an egg, and the Mercury, orbits the Sun within Earth's orbit as an inferior planet; from Earth, Mercury's apparent distance from the Sun never exceeds 28°.

Due to its close proximity to the Sun, the planet may only be seen around the horizons of the western and eastern hemispheres, typically in the twilight hours.

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7. What is the relationship between transistors and gates?

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Transistors and gates are closely related in digital electronics. Gates are the basic building blocks of digital circuits and perform logical operations on input signals to produce an output.

They can be implemented using transistors, which are semiconductor devices that can act as switches or amplifiers. Transistors can be used to control the flow of current in a circuit, which is necessary for implementing logic gates. In fact, most digital circuits today are built using integrated circuits (ICs) that contain millions of transistors that are interconnected to form logic gates and more complex digital circuits. Therefore, without transistors, it would be impossible to build digital circuits and gates.

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The procedure that we use today to to find the distances to other variable stars in nearby galaxies out to roughly 25 Mpc is?

Answers

find the distances to other variable stars in nearby galaxies out to roughly 25 Mpc is called the Cepheid variable method.

Step 1: Identify Cepheid variable stars in nearby galaxies. These stars have a distinct relationship between their luminosity and pulsation period.

Step 2: Measure the pulsation period of the Cepheid variable star, which helps determine its intrinsic luminosity.

Step 3: Observe the apparent brightness of the Cepheid variable star from Earth.

Step 4: Apply the distance modulus formula, which relates the difference between the intrinsic luminosity and the apparent brightness to the distance.

Step 5: Calculate the distance to the Cepheid variable star, and thus to the nearby galaxy it resides in, using the distance modulus formula and the obtained values from Steps 2 and 3.

By following this procedure, astronomers can accurately determine distances to other variable stars in nearby galaxies out to roughly 25 Mpc.

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consider the following statements, all of which are actually true, and select the one that best explains why the moment of inertia of the earth is actually smaller than the moment of inertia you calculated. consider the following statements, all of which are actually true, and select the one that best explains why the moment of inertia of the earth is actually smaller than the moment of inertia you calculated.

Answers

The moment of inertia of the Earth is actually smaller than the moment of inertia you calculated because the Earth does not have uniform density.

As the planet formed, the densest materials sank to the center of the Earth. This created a dense iron core. Meanwhile, the lighter elements floated to the surface. The crust of the Earth is considerably less dense than the core. Thus, the Earth is not a perfect hom*ogeneous sphere, but has a non-uniform density distribution due to the presence of a dense core and lighter mantle and crust. This means that the mass is not distributed evenly throughout the Earth, leading to a smaller moment of inertia. Additionally, the Earth's rotation causes a bulging at the equator, further reducing the moment of inertia.

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what will be the potential energy utot of the system of charges when charge 2q is at a very large distance from the other charges? express your answer in terms of q , d , and appropriate constants.

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The potential energy utot of the system of charges when charge 2q is at a very large distance from the other charges can be calculated using the formula:

utot = k * (q * Q1 / r1 + q * Q2 / r2 + Q1 * Q2 / d)

where k is the Coulomb constant, Q1 and Q2 are the charges at distances r1 and r2 respectively, d is the distance between Q1 and Q2, and q is the charge that is being moved to infinity.

In this case, when charge 2q is at a very large distance from the other charges, we can assume that it is moved to infinity, so q = 2q. Thus, the formula becomes:

utot = k * (2q * Q1 / r1 + 2q * Q2 / r2 + Q1 * Q2 / d)

Simplifying the formula further, we get:

utot = 2kq (Q1 / r1 + Q2 / r2) + kQ1Q2 / d

Therefore, the potential energy utot of the system of charges when charge 2q is at a very large distance from the other charges is expressed in terms of q, d, and appropriate constants as:

utot = 2kq (Q1 / r1 + Q2 / r2) + kQ1Q2 / d
Hi! The potential energy (U_tot) of a system of charges when charge 2q is at a very large distance from the other charges can be calculated using the formula:

U_tot = k * (q1 * q2) / r

In this case, q1 and q2 are the charges, r is the distance between them, and k is the electrostatic constant (8.99 x 10^9 Nm^2/C^2). Since 2q is at a very large distance, its interaction with the other charges becomes negligible. Therefore, the potential energy of the system will only depend on the interactions between the remaining charges.

For example, if there are two charges q and -q separated by a distance d, the potential energy would be:

U_tot = k * (q * -q) / d

So, the potential energy of the system in terms of q, d, and the appropriate constant (k) is:

U_tot = -k * (q^2) / d

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why are 220-v circuits used for such devices as electric clothes dryers and stoves? what differences do you expect to find in the wire used for these circuits compared to 120-v lines?

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220-v circuits are used for electric clothes dryers and stoves because they require a larger amount of power to operate efficiently. These devices use heating elements to dry clothes or cook food, and these heating elements require a high voltage to generate enough heat. A 220-v circuit is capable of delivering twice as much power as a 120-v circuit, making it more suitable for high-power devices like clothes dryers and stoves.

The wire used for 220-v circuits is typically thicker and has a higher amperage rating compared to the wire used for 120-v lines. This is because a higher voltage requires more current to deliver the same amount of power. Thicker wire with a higher amperage rating can handle the higher current without overheating or causing a fire hazard. Additionally, 220-v circuits often require specialized outlets and connectors that can handle the higher voltage and current, further emphasizing the importance of proper wiring and installation.

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Use energy conservation to find the approximate final speed of a basketball dropped from a height of 2.12 m (roughly the height of a professional basketball player).

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The approximate final speed of the basketball dropped from a height of 2.12 m is 5.3 m/s.

The final speed of the basketball dropped from a height of 2.12 m can be found using the principle of energy conservation.

When the basketball is dropped, it gains potential energy due to its position at a height above the ground. As it falls, this potential energy is converted into kinetic energy, which is the energy of motion.
According to the principle of energy conservation, the total amount of energy in the system (the basketball and the Earth) remains constant. Therefore, the potential energy at the top of the drop must be equal to the kinetic energy at the bottom of the drop. The formula for potential energy is:
PE = mgh
Where m is the mass of the basketball, g is the acceleration due to gravity (9.8 m/s²), and h is the height of the drop (2.12 m). The formula for kinetic energy is:
KE = (1/2)mv²
Where m is the mass of the basketball and v is its velocity at the bottom of the drop.
Setting these two equations equal to each other, we can solve for v:
mgh = (1/2)mv²
Simplifying and solving for v, we get:
v = √(2gh)
Plugging in the values for g and h, we get:
v = √(2 × 9.8 m/s² × 2.12 m) ≈ 5.3 m/s


Hence , the approximate final speed of the basketball dropped from a height of 2.12 m is 5.3 m/s.

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Henrietta Leavitt Discovered That RR Lyrae Stars Pulsate... (2024)

FAQs

Why do RR Lyrae stars pulsate? ›

RR Lyrae stars pulse in a manner similar to Cepheid variables, but the nature and histories of these stars is thought to be rather different. Like all variables on the Cepheid instability strip, pulsations are caused by the κ-mechanism, when the opacity of ionised helium varies with its temperature.

What did Leavitt discover about stars? ›

In 1908, Leavitt published her discovery of the period-luminosity relationship—that is, the correlation between how bright a star is and the time it takes for the star to go from bright to dim. Cepheid variable stars change how bright they appear from day to day or week to week as a result of their instability.

Who discovered pulsating stars? ›

Henrietta Swan Leavitt (born July 4, 1868, Lancaster, Massachusetts, U.S.—died December 12, 1921, Cambridge, Massachusetts) was an American astronomer known for her discovery of the relationship between period and luminosity in Cepheid variables, pulsating stars that vary regularly in brightness in periods ranging from ...

Why do Cepheid stars pulsate? ›

The pulsations are due to the periodic expansion and contraction of the surface layers of the stars. The change in size is observed as a change in apparent magnitude.

What is the meaning of the pulsating star? ›

: a star that alternately increases and decreases in size usually with corresponding changes in brightness.

Why are RR Lyrae stars important? ›

RR Lyrae stars are one of the primary distance indicators for old stellar populations such as globular clusters, dwarf galaxies and galaxies.

What did Henrietta Swan Leavitt discover quizlet? ›

Henrietta Swan Leavitt discovered the period-luminosity relationship. This relationship is critical because it tells us the longer the pulsation period, the more luminous the star.

What did Henrietta Swan Leavitt discover for kids? ›

(1868–1921). American astronomer Henrietta Swan Leavitt was known for her discovery of the relationship between period and luminosity in Cepheid variables (pulsating stars that vary regularly in brightness in periods ranging from a few days to several months).

How did Henrietta Leavitt lose her hearing? ›

In 1898, she became a member of the Harvard staff. Leavitt left the observatory to make two trips to Europe and completed a stint as an art assistant at Beloit College in Wisconsin. At this time, she contracted an illness that led to progressive hearing loss.

Who discovered RR Lyrae stars? ›

Harvard College Observatory astronomer Williamina Fleming discovered RR Lyrae itself while examining a photographic plate taken on July 13, 1899. Further investigation showed the star varying in brightness every 13.6 hours from magnitude 7 to 8.

What was the first pulsating star? ›

The first pulsating star, o Ceti , was discovered in 1596 by David Fabricius. Fabricius' observations showed that over a period of 11 months, the bright second magnitude star faded, disappeared, and then finally returned to its former brightness.

Who discovered pulsation theory? ›

The vital force theory about the ascent of sap was advanced by J.C. Bose (1923). It is known as the pulsation theory. The theory states that the innermost cortical cells of the root absorb water from the external side and pump the same into xylem channels.

What is the difference between Cepheids and RR Lyrae? ›

RR Lyrae stars are like Cepheids but are far dimmer. They are often part of globular clusters. These stars also have a period-luminosity relationship which we can use to work out the distance to the cluster. The periods of RR Lyrae stars are much shorter (a few hours to a day or 2).

What is the theory of pulsating stars? ›

Pulsating variable stars are intrinsic variables as their variation in brightness is due to a physical change within the star. In the case of pulsating variables this is due to the periodic expansion and contraction of the surface layers of the stars.

Which stars pulsate? ›

Many intrinsic variable stars that pulsate with large amplitudes, such as the classical Cepheids, RR Lyrae stars and large-amplitude Delta Scuti stars show regular light curves.

Why do stars look like they are pulsing? ›

These so-called variable stars seem to pulsate — either because a star is in a binary system and its companion often eclipses it, or because the star itself periodically swells and shrinks, pulsating in brightness.

What do pulsating variable stars like Cepheids and RR Lyrae use to determine distances? ›

Type I and II Cepheids and RR Lyraes are all examples. All Cepheids with a certain period are assumed to have the same absolute magnitude. Measuring the apparent magnitude of a Cepheid then allows us to determine its distance using the period-luminosity relationship.

Why do stars have pulses? ›

Pulsars are rotating neutron stars observed to have pulses of radiation at very regular intervals that typically range from milliseconds to seconds. Pulsars have very strong magnetic fields which funnel jets of particles out along the two magnetic poles. These accelerated particles produce very powerful beams of light.

Why do Mira variables pulsate? ›

They are pulsating due to the entire star expanding and contracting. This produces a change in temperature along with radius, both of which factors cause the variation in luminosity.

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