By Robert, Alexis, and Arleth

Slides:



Advertisements
Similar presentations
The Solar System Chapter 12 Section 1 Pgs
Advertisements

The Outer Planets Chap 16, Sec 4.
Neptune The Blue Planet.
THE OUTER PLANETS. The first four outer planets- Jupiter, Saturn, Uranus, and Neptune- are much larger and more massive than Earth, and they do not have.
4.5 The Outer Planets What Do the Outer Planets Have in Common?
THE OUTER PLANETS. The Gaseous Planets- Jupiter, Saturn, Uranus, Neptune.
Chapter 20 – The Solar System. Facts and Pictures From
NEPTUNE Chris Haney Artemio Huerta Raimar Ortiz. DATE OF DISCOVERY Neptune was discovered on September 23 rd 1846, by Urbain Le Varrier and Johann Galle.
Uranus and Neptune Astronomy 311 Professor Lee Carkner Lecture 19.
The Solar System An Interactive Learning Station.
Uranus and Neptune Astronomy 311 Professor Lee Carkner Lecture 19.
Neptune is the 8th planet from the sun in our solar system.
 Mercury Venus  Earth Mars Small in size Made of rock and metal. Few satellites. Slow rotation.
The Nine Planets (13.14).
Planets of the Solar system Section 4 Section 4: The Outer Planets Preview Key Ideas The Outer Planets Gas Giants Jupiter Saturn Uranus Neptune Objects.
This PowerPoint is all about space and different planets. It will all so talk about the different objects in space.
The Outer Planets Jupiter, Saturn, Uranus, Neptune Click here to move to the next slide!
Ch The Outer Planets.
Neptune: The Last Gas Giant
Name that Planet!. This planet has 2 moons, whose names are Phobos and Deimos.
The Inner Planets Mercury Closest planet to the sun Surface has many craters and looks like the moon Cliffs that may have formed from the iron rich.
The Outer Planets Jupiter It is the 5 th planet from the sun, and the largest planet in the solar system Contains more mass than all the other.
Our solar system Chapter 2 By Mrs. Shaw.
By: Mrs. Crisp The Outer Planets. S.P.I – Distinguish among the planets according to their known characteristics such as appearance, location,
Solar System Notes.
The Gas Giant Planets. Jupiter Origin of name: From the king of the gods, Zeus or Jupiter.
I.Uranus and Neptune: Discoveries, atmospheres, interiors, rotation, magnetic fields, moons, rings, Uranus’ axis tilt and seasons. II.Pluto and Charon:
Cole Nachman. Symbol Why the name Neptune? ❏ Urbain Le Verrier discovered planet. ❏ Claimed right to name discovery.
Uranus and Neptune Uranus: general information –Discovered in 1781 (Herschel) –Radius about 4x that of Earth –Mass about 14.5x that of Earth –Nearly featureless.
The Solar System Kayli White & Anne Riley. The inner planets vs. the outer planets The inner planets: Mercury, Venus, Earth, and Mars. They are relatively.
Hilari Hopson.  There are eight major planets in the solar system, all with their own unique features.  This power point will explain how each of these.
The Planet Neptune Julia Carnevale.
Neptune By Maxwell Salvadore. History Discovered by Urbain Le Verrier and Johann Galle Discovered by Urbain Le Verrier and Johann Galle Discovered on.
Physical Characteristics of the Planet Neptune by: Jonathon Carten.
NEPTUNE. FACTS Named after Roman god of the sea Named after Roman god of the sea Only planet that cannot be seen without a telescope Only planet that.
Greenhouse Effect Earth absorbs energy from the Sun and heats up Earth re-radiates the absorbed energy in the form of infrared radiation The infrared radiation.
The Outer Planets Know about Jupiter Know about Saturn
Neptune By Vicente And Leo. Explorations The Voyager 2 spacecraft was launched in 1977 and it reached Neptune on Aug 24, So, Voyager 2 took about.
The Jovian Planets, Part III Uranus and Neptune. URANUS The God of the Heavens.
Discovery of Uranus, Neptune, Pluto The last 3 planets were discovered with telescopes, in the last 150 years or so (too faint to see with eyes) Studied.
Planets of the Solar system Section 4 Key Ideas Identify the basic characteristics that make the outer planets different from terrestrial planets. Compare.
Section One: Our Planets, Our Solar System The Planets, From Closest To the Sun  Mercury  Venus  Earth  Mars  Jupiter  Saturn  Uranus  Neptune.
Exploring Our Solar System: A Journey By: Sarah Naeger.
The Outer Planets - Jupiter Jupiter, the largest of the planets, is 2.5 times more massive than all the other planets combined It is covered by clouds.
This picture of Neptune was taken by Voyager 2 on August 20, One of the great cloud features, dubbed.
By: Shua Kim. It was named after the Roman mythology, Neptune, he was the god of the sea.
Chapter 23 The Solar System Section 2 Outer Planets Notes 23-4.
The Solar System.
Neptune Shaniya Malcolm General Science.  Surface Of Neptune  The Space Shuttle/ Voyager 2  Composition  Winds  When Discovered  Facts  Symbols.
The Solar System Steele Smith. The Solar System.
I.Uranus and Neptune: Discoveries, atmospheres, interiors, rotation, magnetic fields, moons, rings, Uranus’ axis tilt and seasons. II.Pluto and Charon:
The Windy Planet. Neptune was the first planet located through mathematical predictions rather than through regular observations of the sky. (Neptune.
What does Neptune look like? The particles of icy methane in the clouds takes orange and red light waves and absorbs them, which leaves blue light waves.
Neptune By: Macy and Whitney.
Reviewing the Inner Planets
Section 3: The Outer Planets
Neptune The Windy Planet.
Neptune The Blue Planet.
URANUS.
The Outer Planets.
Neptune The Blue Planet.
Section 4 – pg 562 The Outer Planets
Section 3: The Outer Planets
Uranus.
JUPITER A Gaseous planet.
The Outer Planets of Our Solar System
The Gas Giants...and Pluto
Neptune The Blue Planet.
The Outer Planets of Our Solar System
The Solar System Steele Smith.
Presentation transcript:

By Robert, Alexis, and Arleth Neptune By Robert, Alexis, and Arleth

Discovery Neptune was discovered September 23rd, 1846. The time is takes for Neptune to circle around the sun once (orbital period) is 165 years. The length of their average day is 16 hours and 6 minutes.

Neptune Neptune is the eighth and farthest planet from the Sun in the Solar System. It is the fourth-largest planet by diameter and the third-largest by mass. Among the gaseous planets in the Solar System, Neptune is the most dense.

Location of Neptune The planet Neptune was mathematically predicted before it was directly observed. After it was discovered, it turned out it had been observed many times before but not recognized. There were others who made various calculations about its location, which did not lead to its observation.

Earlier observations Neptune is invisible to the naked eye as it is too dim. There is evidence that Neptune was seen and recorded by Galileo Galilei in 1613, Jérôme Lalande in 1795 and John Herschel in 1830, but none is known to have recognized it as a planet at the time.

Neptune’s moon discovery Neptune's largest moon, Triton, was discovered at the same time as the planet. Another satellite, Nereid, wasn't found until 1949. The other six were spotted by Voyager II during its flyby in 1989. A lot of research has been done on Triton, and there is evidence that life may have existed there at one time.

Neptune’s Atmosphere Neptune’s atmosphere is made up mostly of hydrogen, helium, and methane. The upper atmosphere of Neptune contains some white clouds of frozen methane. Neptune has an average cloud-top temperature of about -225 C. At a speed of 1,000 km/h, Neptune has the strongest winds in the Solar System.

Moons William Lassell spotted Triton on 10 October 1846 -- just 17 days after a Berlin observatory discovered Neptune. It is the largest moon Neptune has and the farthest. Dutch-American astronomer Gerard Kuiper (for whom the Kuiper Belt was named) found Neptune's third-largest moon, Nereid, in 1949. He missed Proteus, the second-largest, because it's too dark and too close to Neptune for telescopes of that era.

Moons Proteus and five other moons had to wait for Voyager 2 to make themselves known. All six are among the darker objects found in the solar system. Astronomers using improved ground-based telescopes found more satellites in 2002 and 2003, bringing the known total to 13.

Triton Voyager 2 revealed fascinating details about Triton. Part of its surface resembles the rind of a cantaloupe. Ice volcanoes spout what is probably a mixture of liquid nitrogen, methane and dust, which instantly freezes and then snows back down to the surface. Triton's icy surface reflects so much of what little sunlight reaches it that the moon is one of the coldest objects in the solar system, about -400 degrees Fahrenheit (-240 degrees Celsius).

Rings The rings of Neptune consist primarily of five principal rings and were first discovered (as "arcs") in 1984. At their densest, they are comparable to the less dense portions of Saturn's rings but much of Neptune's ring system is quite tenuous, faint and dusty, more closely resembling the rings of Jupiter.

Internal Observation The mantle is equal to 10 to 15 Earth masses and is rich in water, ammonia and methane. The core of Neptune is composed of iron, nickel and silicates, with an interior model giving a mass about 1.2 times that of Earth.

The Mysterious Dark Spot In 1989, the Great Dark Spot, an anti-cyclonic storm system was discovered by NASA's Voyager 2 spacecraft. The storm resembled the Great Red Spot of Jupiter. Some five years later, on 2 November 1994, the Hubble Space Telescope did not see the Great Dark Spot on the planet. Instead, a new storm similar to the Great Dark Spot was found in the planet's northern hemisphere.

Orbital Period Because Neptune is not a solid body, its atmosphere undergoes differential rotation. The wide equatorial zone rotates with a period of about 18 hours, which is slower than the 16.1-hour rotation of the planet's magnetic field. By contrast, the reverse is true for the polar regions where the rotation period is 12 hours.

http://www. cleanvideosearch. com/media/action/yt/watch http://www.cleanvideosearch.com/media/action/yt/watch?videoId=EmUvTH7sveg

As you can see, Earth is no comparison to Neptune’s mass and size.