Sentences with phrase «kilometers per hour]»

They are rated at 16.0 kilometers per liter (km / l) according to Japan's 10 - 15 mode test cycle (versions with power sliding doors are rated at 15.0 km / l).
At speeds over 60 kilometers per hour, the Rear Vehicle Monitoring (RVM) system detects vehicles approaching from behind and alerts the driver.
The special edition Demio 13C - V HID EDITION is based on the Demio 13C - V model grade that features a continuously variable transmission (CVT) and achieves eco-friendly fuel economy of 23.0 kilometers per liter * 2.
As a friendly reminder, the Jeep Grand Cherokee Trackhawk not only comes loaded with a 707 - hp engine, but is also able to sprint to 60 miles per hour (96 kilometers per hour) in just 3.5 seconds, continuing on to a quarter mile of 11.6 seconds, and a top speed of 180 mph (289 kmh).
The twin turbo V6 engine puts out 362 horsepower, plenty to push the speedometer needle to 150 kilometers per hour, then 160, and quickly to 170 before we settled in with the flow of traffic at 180.
The SUV requires 6.7 seconds to reach 62 miles per hour (100 kilometers per hour).
The Mazda Demio SKYACTIV - G will achieve fuel economy of 30 kilometers per liter (70.6 mpg US, 3.3 L / 100 km) on the 10 - 15 cycle without any assistance from an electric motor.
It accelerates from 0 - 60 mph in 4.6 seconds with an electronically regulated top speed of 186 mph (300 kilometers per hour).
This Lamborghini Urus hit 0 to 62 mph in 3.6 seconds and the top speed is 186 mph or 300 kilometers per hour.
The main Mickey face has a digital speedometer (in kilometers per hour) at its center surrounded by a wildly swinging power needle that ranges from Charge (during regenerative braking) on the left to Power (full acceleration) at the right.
That's incredible - they drove at about 65 kilometers per hour and that's not a traffic jam where hybrid cars show themselves well, so «hybrid» alone doesn't explain how it was possible.
However the phrase for fuel economy in metric countries is either kilometers per liter or liters per 100 Km.
What we noticed was the really elite athletes were able to reach 25 kilometers per hour.
My job is mainly at a computer, but I work out 5 days a week made up of the following, 1) 30 minutes run at 9.5 Kilometers per hour then, 2) 3 sets of 2 minutes at 6.5 Km per hour followed by 1 minutes at 10 Km per hour.
In graphene, however, the electrons» effective mass is zero and they behave like elementary particles obeying a version of Einsteinian relativity, albeit in a realm where the ultimate speed limit is about 800 kilometers per second instead of the usual 300,000 kilometers per second.
Colliding at speeds up to 22,000 miles per hour (36,000 kilometers per hour), such a collision may have stripped most of the rocky mantle from the protoplanet that became Mercury with its iron - rich core, while a Mars - size protoplanet struck the early Earth off - center and created a spray of mostly mantle material that later accreted to form the Moon.
So far astronomers have only been able to account for about 450 to 500 kilometers per second of the Local Group's motion.
While originally classified as a comet, observations from ESO and elsewhere revealed no signs of cometary activity after it slingshotted past the Sun on Sept. 9 at a blistering speed of 196,000 miles per hour (87.3 kilometers per second).
The Greenland and Antarctic ice sheets began to shed ice at a rate, now several hundred cubic kilometers per year, which is continuing to accelerate [23]--[25].
Charged winds moving at speeds up to 1000 kilometers per second from the star, much like those in our Sun's solar wind but millions of times denser, are able to follow the twisted field lines on their way out into space.
As of Nov. 20, «Oumuamua is travelling about 85,700 miles per hour (38.3 kilometers per second) relative to the Sun.
2000 years is a long time, but we're still talking 650 kilometers per second, and just 20 years to the Oort Cloud!
Where winds are blowing east, that motion adds speed to the planet's already high rotational speed of about 43,000 kilometers per hour (27,000 miles per hour).
According to astrophysicist Paul Sutter, the universe expands at roughly 68 kilometers per second per megaparsec, where a megaparsec is 3.26 million light - years (more on that later).
Pixels scales of the composite images vary from 2 to 4 kilometers per pixel (1.2 to 2.5 miles per pixel).
(These disturbances travel at the speed of light, while the fastest seismic waves of an earthquake propagate at several kilometers per second, which means that monitoring the disturbances could potentially improve existing early - warning systems by seconds or even minutes.)
Light travels at 186,000 miles per second (300,000 kilometers per second).
The most current estimate of H is 70 kilometers per second per megaparsec.
Eventually, two of these stars either grazed each other or collided, triggering a powerful eruption that launched other nearby protostars and hundreds of giant streamers of dust and gas into interstellar space at speeds greater than 150 kilometers per second.
The spectra of a nova shows blue - shifted absorption lines showing that a hot dense gas is expanding towards us at a few thousands of kilometers per second.
Winds have been clocked at 1,800 kilometers per hour (1,118 miles per hour) near Saturn's equator.
What was it's average speed in kilometers per hour (or miles per hour)?
Doppler shifts of the disk material close to the center show that the gas is moving at speeds of hundreds of kilometers per second.
The coronal mass ejection, or CME, traveled at over 1450 kilometers per second.
The Earth orbits the sun at 15 kilometers per second (18.5 miles per second).
Putting the measurements together, the team determined the star is moving at about 1,200 kilometers per second — much higher than the velocities of previously known stars in the Milky Way galaxy.
MAUNA KEA, HI — Scientists using the W. M. Keck Observatory and Pan-STARRS1 telescopes on Hawaii have discovered a star that breaks the galactic speed record, traveling with a velocity of about 1,200 kilometers per second or 2.7 million miles per hour.
The sun moves in the plane of the galaxy on the outskirts of one of its spiral arms at a speed of 220 kilometers per second (136 miles per second).
There are strong winds of 350 kilometers per hour (218 miles per hour) at the cloud tops, but surface winds are weak — no more than a few kilometers (or miles) per hour.
When a large solar eruption occurs, the release of material can often be a billion tonnes or more spewing out from the sun's interior at over 2,500 kilometers per second (5,500 mph)(Credit: Airbus Defence and Space (UK)-RRB-
However, when a particularly large eruption occurs, the release of material can often be a billion tonnes or more spewing out from the sun's interior at over 2,500 kilometers per second (5,500 mph).
When a large solar eruption occurs, the release of material can often be a billion tonnes or more spewing out from the sun's interior at over 2,500 kilometers per second (5,500 mph)
Right now these two are on a collision course at 300 kilometers per second, and when they do collide, they will form a new super-giant, elliptical galaxy.
July 29, 2014 NGC 514, an intermediate spiral galaxy in Pisces Image Credit: Curt Harris / NOAO / AURA / NSF and Adam Block / Mount Lemmon SkyCenter / University of Arizona (http://skycenter.arizona.edu/gallery) NGC 514 is an intermediate spiral galaxy, located about 95.9 million light - years away from Earth in the constellation of Pisces (the Fishes), while it is receding from us at approximately 2,472 kilometers per [continue reading]
Starting from the Earth's orbital speed of 30 kilometers per second (km / s), the change in velocity (delta - v) the spacecraft must make to enter into a Hohmann transfer orbit that passes near Mercury is large compared to other planetary missions.
And its speed (about 100,000 kilometers per hour, or 62,000 miles per hour) rules out an origin within the solar system or the Oort cloud, where comets come from.
NGC 514 is an intermediate spiral galaxy, located about 95.9 million light - years away from Earth in the constellation of Pisces (the Fishes), while it is receding from us at approximately 2,472 kilometers per second.
Upon reaching this height, they can erupt for a few minutes to hours and send large amounts of material racing through the corona and outward into space at 600 miles per second (1,000 kilometers per second); these eruptions are called coronal mass ejections.
The star spins around its axis at the speed of 600 kilometers per second at the equator, a rotational velocity so high that the star is nearly tearing apart due to centrifugal forces.
And as of Nov. 5, they estimated it was racing toward the sun at nearly 45 kilometers per second (almost 28 miles per second).
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