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- California
- Southern California
- Apple Valley
- Sun City Apple Valley
Explore Our Home Collections
$173,990+
1511+ sqft
Living Well Collection ()
Living Well Collection
$173,990
Starting Price
1,511
sqft
2
bd
2
ba
2
TEST 2
Living Well Collection ()
Living Well Collection
$192,990
Starting Price
1,633
sqft
2
bd
2
ba
2
TEST 2
Living Well Collection ()
Living Well Collection
$215,990
Starting Price
1,958
sqft
2
bd
2
ba
2
TEST 2
Living Well Collection ()
Living Well Collection
$221,990
Starting Price
2,023
sqft
3
bd
2
ba
2
TEST 2
Living Well Collection ()
Living Well Collection
$241,990
Starting Price
2,340
sqft
3
bd
3
ba
2
TEST 2
Living Well Collection ()
$173,990
Starting Price
The Encore, a two bedroom, two bathroom home is one to make your own. Enjoy evening gatherings with close neighbors on your available front courtyard or sip your morning coffee in your sunny breakfast nook. The Owner’s suite encourages even more relaxation with available access directly into your backyard and a spacious bathroom with walk-in closet. Wind your day down in your available sun room complete with or without a cozy fireplace.
Living Well Collection ()
$192,990
Starting Price
Find contentment in this wonderful home; The Serenity, with 2 bedrooms, 2 bathrooms and an included den. The open great room is complete with adjacent dining area and kitchen with a sit-around island. Enjoy the large Owner’s Suite with private bath, walk-in closet and available retreat or snore room in place of the den. If the outdoors is your palace, enjoy your available sun or hearth room, front courtyard and garage extension.
Living Well Collection ()
$215,990
Starting Price
At just under 2,000 feet of gracious single-story living, The Celebration is a warm and inviting home. Enjoy 2 bedrooms, 2 bathrooms and included den or opt for a 3rd bath in place of the den. Complete with large storage area in the garage, this space can be easily converted into a convenient hobby room or snore room that connects to the spacious Owner’s Suite. Want a unique space? Check out our Super Laundry room complete with plenty of cabinets and a variety of available options to make this space work for you. Topping off the available features of the Celebration, you can enjoy a Dual Owner’s Suite sun or hearth room.
Living Well Collection ()
$221,990
Starting Price
The Haven is an impressive three bedroom, 2 bath home with a variety of options that will help you create your own personalized sanctuary. Entertain with your available built-in wet bar, wine storage or guest-friendly powder bath, extended covered patio and find relaxation in your available sun room – with or without a cozy fireplace. This home offers an optional dual owner’s suite complete with a separate sitting area, walk-in closet and en suite bath.
Living Well Collection ()
$241,990
Starting Price
This beautiful and spacious home provides a formal feel with the long, elegant entry foyer. This home at Sun City Apple Valley provides a separate formal dining room with a private covered patio or available for additional entertaining. Enjoy the convenience of three bedrooms and three full baths or convert one bedroom into a sunny den. An open great room with available fireplace and large covered patio in the back make this home a true candidate for free-flowing conversation. The Owner’s Suite showcases an optional bay window and is complete with large walk-in closet and rejuvenating bathroom.
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Hours:
Monday 9:00AM - 5:00PM
Tuesday 9:00AM - 5:00PM
Wednesday 9:00AM - 5:00PM
Thursday 9:00AM - 5:00PM
Friday 9:00AM - 5:00PM
Saturday 9:00AM - 5:00PM
Sunday 9:00AM - 5:00PM
Hours:
Monday 9:00AM - 5:00PM
Tuesday 9:00AM - 5:00PM
Wednesday 9:00AM - 5:00PM
Thursday 9:00AM - 5:00PM
Friday 9:00AM - 5:00PM
Saturday 9:00AM - 5:00PM
Sunday 9:00AM - 5:00PM
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The formation and evolution of the Solar System began 4.6 billion years ago
This model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.
The formation and evolution of the Solar System began 4.6 billion years ago
This model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.
The formation and evolution of the Solar System began 4.6 billion years ago
This model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.
The formation and evolution of the Solar System began 4.6 billion years ago
This model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.
Perturbation theory was first devised to solve otherwise intractable problems in the calculation of the motions of planets in the solar system
The Solar System has evolved considerably since its initial formation. Many moons have formed from circling discs of gas and dust around their parent planets, while other moons are thought to have formed independently and later been captured by their planets. Still others, such as Earth's Moon, may be the result of giant collisions. Collisions between bodies have occurred continually up to the present day and have been central to the evolution of the Solar System. The positions of the planets often shifted due to gravitational interactions.[2] This planetary migration is now thought to have been responsible for much of the Solar System's early evolution
The formation and evolution of the Solar System began 4.6 billion years ago
This model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.
The formation and evolution of the Solar System began 4.6 billion years ago
This model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.
The formation and evolution of the Solar System began 4.6 billion years ago
This model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.
The formation and evolution of the Solar System began 4.6 billion years ago
This model, known as the nebular hypothesis, was first developed in the 18th century by Emanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace. Its subsequent development has interwoven a variety of scientific disciplines including astronomy, physics, geology, and planetary science. Since the dawn of the space age in the 1950s and the discovery of extrasolar planets in the 1990s, the model has been both challenged and refined to account for new observations.
Perturbation theory was first devised to solve otherwise intractable problems in the calculation of the motions of planets in the solar system
The Solar System has evolved considerably since its initial formation. Many moons have formed from circling discs of gas and dust around their parent planets, while other moons are thought to have formed independently and later been captured by their planets. Still others, such as Earth's Moon, may be the result of giant collisions. Collisions between bodies have occurred continually up to the present day and have been central to the evolution of the Solar System. The positions of the planets often shifted due to gravitational interactions.[2] This planetary migration is now thought to have been responsible for much of the Solar System's early evolution
Perturbation theory was first devised to solve otherwise intractable problems in the calculation of the motions of planets in the solar system
For instance, Newton's law of universal gravitation explained the gravitation between two heavenly bodies, but when a third body is added, the problem was, "How does each body pull on each?" Newton's equation only allowed the mass of two bodies to be analyzed. The gradually increasing accuracy of astronomical observations led to incremental demands in the accuracy of solutions to Newton's gravitational equations, which led several notable 18th and 19th century mathematicians, such as Lagrange and Laplace, to extend and generalize the methods of perturbation theory. These well-developed perturbation methods were adopted and adapted to solve new problems arising during the development of quantum mechanics in 20th century atomic and subatomic physics. Paul Dirac developed perturbation theory in 1927 to evaluate when a particle would be emitted in radioactive elements. It was later named Fermi's golden rule.[7][8]