It should be clear from this diagram that you never even see half the earth-and that being close to the view port is essential to see enough. If the need is to see all of earth within a 135° view angle (2 θ in the diagram) then we can obtain h from.
Here are the amazing planet sights to look for this year! As an evening star, Mercury appears in the western sky setting about an hour after the sun. As a morning star, it appears in the eastern sky rising about an hour before the sun. There must be a clear, unobstructed horizon on these occasions.
In the daytime, you can clearly see major landforms. At night, from Earth orbit, you see the lights of Earth’s cities. Earth in daylight, from the International Space Station in 2012. The North American Great Lakes shine in the sun.
As an evening star, Mercury appears in the western sky setting about an hour after the sun. As a morning star, it appears in the eastern sky rising about an hour before the sun. There must be a clear, unobstructed horizon on these occasions. Mercury usually appears as a bright "star" with a yellowish or ochre hue.
(The north celestial pole is defined as the point in the celestial sphere directly above Earth's North Pole. So, if you are at the North Pole, the north celestial pole must be directly above your head). Where on Earth can you stand and, over the entire year, see the entire sky? the tilt of the Earth's axis.
At the Earth's equator, no star is circumpolar because all the stars rise and set daily in that part of the world. You can (theoretically) see every star in the night sky over the course of one year.
People near the North Pole can see the constellations that are to the north of Earth in space. People near the South Pole can see the constellations that are to the south. People who live in between can see some of both, depending on how close they are to the equator.
Why Do We See Different Constellations During the Year? If observed through the year, the constellations shift gradually to the west. This is caused by Earth's orbit around our Sun. In the summer, viewers are looking in a different direction in space at night than they are during the winter.
The Antarctic sky is quite different from the one we know in the Northern Hemisphere. The Big Dipper and the North Star are not visible from there.
To see the north celestial pole directly overhead, it would have to be your zenith. This can only happen at the Earth's north pole, which is located at the north celestial pole.
Sadly, no observer on Earth can see all 88 constellations at once. Which star patterns one can spot at any given night depends on the time, season, the stargazer's latitude and, obviously, the observational conditions.
Answer: There are no constellations visible all-year from the Earth's equator. By the same token, all constellations are visible at some point during a given year.
Polaris will thus be visible in 13000 years or so as a wintertime star to all of Africa, all of Australia, and most of South America, but none of Antarctica. After millions of years, proper motion may make Polaris visible over Antarctica.
No, the sky we see is not the same. At any point on earth at any given time, about 1/2 of the entire possible sky will be visible (basically, think of the sky above you as a giant "dome" which is equal to 1/2 of the entire sphere around the earth).
When the Big Dipper is seen above Polaris, the North Star, the Southern Cross is seen standing over the southern horizon in southern Florida and Texas. For the Southern Hemisphere, by the way, it works the same way – but in reverse.
You're absolutely right that stars twinkle — and sometimes appear to move around — due to our atmosphere “scrambling” their light as it travels from the top of Earth's atmosphere to the ground. This phenomenon, also called scintillation, tends to occur more obviously in bright stars.
This says that you would have to be 3678 km (2285 miles) away from the earth to see it as a full disk. Since the ISS is orbiting at an altitude of 347 km (216 miles) perigee and 360 km (224 miles) apogee (the mean is about 353 km (219 miles)), I believe that you will not be able to see the earth as a full disk from the space station.
So, if you started moving straight up from the North Pole, you would see a smaller and smaller earth-disk, including more and more of the earths surface. When you reached about 1000 km, the earth would look around 120 degrees across, and you would see the polar regions down to about 60 degrees North Latitude... Share.
Mars will appear rather close to a 16% waxing crescent moon as they descend the west-northwest sky on the evening of May 15. On the evening of July 13, Mars will stand very closely below a much brighter Venus. On the evening of July 30, Mars will pass closely above the 1st magnitude star Regulus in Leo.
Venus is always brilliant, and shining with a steady, silvery light. It is visible in the morning in the eastern sky at dawn from Jan. 1 to 23. It appears in the evening in the western sky at dusk from May 24 to Dec. 31. When the year opens, it will be visible very low near the east-southeast horizon about 90 minutes before sunrise.
A small telescope may reveal its tiny, greenish disk. Uranus spends all of 2021 in the constellation of Aries the Ram. Evenings from January 1 to April 12; mornings from May 16 to November 3; evenings again from November 4 to December 31.
Brightest in 2021: Aug. 8 to Sept. 2. Jupiter is at opposition to the Sun on August 20, shining at a dazzling magnitude of -2.9. On the morning of March 5, about a half hour before sunup, Jupiter will appear just to the right of Mercury. Both planets will hover low above the east-southeast horizon. Use binoculars.
On New Year's Day it resembles the brilliant star Arcturus, both in terms of color and brightness; thus, is at its brightest at the very start of the year. Positioned against the stars of Pisces, Mars is high in the south-southeast at nightfall and will not set until 1:30 a.m.
Coming off a spectacular autumn apparition in 2020, when Mars came within 38.6 million miles (62.1 million km) of Earth and briefly became the third brightest object in the night sky, this planet has since fallen behind Earth and is receding, growing smaller and dimmer each night.
Mercury. As an evening star, Mercury appears in the western sky setting about an hour after the sun. As a morning star, it appears in the eastern sky rising about an hour before the sun. There must be a clear, unobstructed horizon on these occasions.
Not only is it warm enough to stand around in short sleeves and look at the stars, but the Milky Way is also visible soon after sunset. The planets are visible at different times depending on the year, but views like this of the Milky Way can be enjoyed every summer and early autumn.
The Southern Hemisphere has a different perspective on the universe around us and so a different view of the night sky, including some sights that those in the Northern Hemisphere never see. In the above image, you can see a great example of that: the Milky Way’s bright core. You have to be in the Southern Hemisphere to see our own galaxy’s center at its brightest. It’s best viewed from a remote dark sky destination like Karijini National Park in Western Australia between April and November.
On the left is the summer Milky Way streaming towards the horizon, and on the right is a meteor – also known as a shooting star – from the Delta Aquariid meteor shower, which happens every year in July. Click here for EarthSky’s yearly meteor guide. Image via Noel Benadom. 4.
Why do stars twinkle? Technically they don’t, but the closer you are to sea-level, the more air you are stargazing through – which distorts everything and makes stars look like they’re twinkling.
Acadia National Park, Maine, U.S. September is probably the best month of the year at Acadia for stargazing and astrophotography (which is the photography of astronomical and celestial objects in the night sky).
The “king of the meteor showers,” the Geminids can produce up to 120 marvelous multicolored meteors per hour. Click here for EarthSky’s meteor shower guide. Arches National Park in the U.S. state of Utah.
For a totally different kind of photo, get yourself here for dusk on November 24, 2019, for a rare close conjunction of Venus and Jupiter, when the 2 brightest planets will be just 1.4 degrees apart for one night only.
The Sun always takes a path from east to west across the sky during the day. The only thing that varies is whether that path goes directly above you, or arcs across the Southern sky, or arcs across the Northern sky or even arcs below the horizon. The starting and ending points are the same.
At noon, it will be 23.4 degrees above the horizon - the same angle as the Earth's tilt. This is as high as the Sun ever gets at the North Pole.
At noon, it will be 23.4 degrees above the horizon - the same angle as the Earth's tilt. This is as high as the Sun ever gets at the South Pole. At the Equator. The Equator is at a latitude of 0 degrees. At the spring equinox, the Sun will start in the East, arc directly overhead and set in the West.
At the South Pole, it will be 0 degrees above the Northern horizon (right along it). And at the equator, it will be directly above (90 degrees above the horizon). Learning Outcomes. When you are finished, you should be able to: Explain the importance of latitude in determining the Sun's path across the sky.
The peak of summer is called the summer solstice and is on June 21st in the Northern hemisphere. This is when the days are longest, and the Sun at noon is as high as it will ever be. At 40 degrees north, the Sun rises in the East and arcs across the Southern sky to set in the West.
A latitude of 40 degrees north means that you are 40 degrees above the equator. New York City and Madrid are two cities at about this latitude. In its arc across the sky, the Sun reaches its highest point at noon. This high point is super high in winter and super low in summer.
The arc is right in the middle when the days and nights are 12 hours each on March 21st ( the spring equinox) and September 21st ( the autumn equinox ). At Noon on either of the equinoxes, when the Sun is at its highest, it will be exactly 40 degrees above the horizon - the same as the latitude.
One must travel an infinite distance before 50% of the planet is visible. Any closer and the distance between your eyes will mean that less than 50% is visible - as your eyes are not the diameter of the earth apart, at any real distance it is only possible to approach the 50% boundary. Highly active question.
Virgin Galactic will take passengers aboard SpaceShipTwo as high as 65 miles above the surface of the earth. But from this altitude, passengers will only be able to see a certain segment of the curvature of the earth through windows as large as 17 inches in diameter. How much further into space would SpaceShipTwo have to travel to give passengers ...
From the window of the ISS, the surface of the Earth looms large. In the daytime, you can clearly see major landforms. At night, from Earth orbit, you see the lights of Earth’s cities. Earth in daylight, from the International Space Station in 2012. The North American Great Lakes shine in the sun.
That’s in contrast to our sun’s distance from Earth of about 93 million miles (150 million km). In this image, the sun is located on the right, outside the image frame. Image via ESA/ NASA / NRL/ Solar Orbiter/ SolOHI. What does Earth look like from outer space?
Earth and moon seen by NEAR spacecraft in 1998. Speeding outward from the Earth and moon system, you pass the orbits of the planets Mars, Jupiter and Saturn. From all of these worlds, Earth looks like a star, which gets fainter as you get farther away.
It’s highly elliptical, stretching from just 2.7 billion miles (4.4 billion km) to over 4.5 billion miles (7.3 billion km) from the sun. Pluto is within the limiting distance at which – if we just consider brightness alone, no other factors – we should be able to see Earth with the eye alone.
Earth is the bluish-white speck approximately halfway down the brown band to the right.
The first images of the Earth from the moon came from the Apollo mission. Apollo 8 in 1968 was the first human spaceflight to leave Earth orbit. It was the first earthly spacecraft to be captured by and escape from the gravitational field of another celestial body, in this case the moon.
Launched by Japan, and officially named the Selenological and Engineering Explorer (SELENE), Kaguya studied the origin and evolution of the moon. The frame below is from Kaguya ’s onboard HDTV camera. Earth viewed from the moon by Kaguya in 2007. Image via SELENE Team JAXA/ NHK.