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Don't Miss This Weekend's Sky Show As The Moon And Mars Shine Together

Don't Miss This Weekend's Sky Show As The Moon And Mars Shine Together

Forbes5 hours ago

In an alignment of celestial bodies, Mars was captured here rising out of a lunar occultation on 13 ... More January 2025 using the new Visitor Center 0.6-meter Shreve Telescope at the U.S. National Science Foundation Kitt Peak National Observatory (KPNO), a Program of NSF NOIRLab, near Tucson, Arizona.
Skywatchers will have two opportunities this weekend to see the moon form striking alignments in the post-sunset sky. On Saturday, June 28, a trio featuring the moon, Mars and the bright star Regulus will appear in a neat arc. Then, on Sunday, June 29, the moon and Mars will be in a very close conjunction — and in some parts of the world, Mars will be briefly occulted by the moon. Here's everything you need to know about what to see in the night sky this weekend.
Where And When to Look
Be outside looking to the western horizon about 45 minutes after sunset. You'll need a clear, unobstructed view since the moon and its companions will be low in the sky. The display will be short-lived, disappearing from view within about 45 minutes as twilight deepens — so good timing is imperative. Mars will appear dimmer than the moon, but it will be easy to find.
Saturday, June 28: Moon, Regulus And Mars
What You'll See
On Saturday, June 28, a 16%-lit crescent moon will be a spectacular sight. Slightly above and left of the moon will be Regulus, the brightest star in the constellation Leo, and farther away, the reddish dot of the planet Mars. The three objects will be spaced nearly evenly, forming a clear visual arc.
That arc will crumble after sunset on Sunday, June 29, when the now 24%-lit crescent moon will appear in conjunction with Mars — just 0.2 degrees apart as seen from North America. That's less than an outstretched little finger held against the night sky. From parts of the Pacific and northern South America, the moon will occult Mars for about an hour, according to In-The-Sky.org.
Sunday, June 29: Moon And Mars In Conjunction
Observing Tips
You just need naked eyes for this sky event, though a pair of binoculars will enhance the view, especially on Sunday, when the moon and Mars will be close enough to fit within the same field. However, a close-up of the moon on either night will reveal something beautiful on its night side — Earthshine, sunlight reflected from Earth's clouds, oceans and ice caps onto the lunar surface.
An open view to the west is essential both nights, especially during the first hour after sunset, when the celestial trio is visible.
Monday, June 30: Moon, Mars And Regulus
What's Next In The Night Sky
Although the arc of bright objects will be much looser, look west after sunset on Monday, June 30, and you'll see a 33%-lit crescent moon, this time on the other side of Mars and Regulus.
For exact timings, use a sunrise and sunset calculator for where you are, Stellarium Web for a sky chart and Night Sky Tonight: Visible Planets at Your Location for positions and rise/set times for planets.
Wishing you clear skies and wide eyes.

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A Simple Way to Close Racial Gaps in Cancer Trial Enrollment
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A Simple Way to Close Racial Gaps in Cancer Trial Enrollment

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Why Reliability Is The Hardest Problem In Physical AI
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Why Reliability Is The Hardest Problem In Physical AI

Dr. Jeff Mahler: Co-Founder, Chief Technology Officer, Ambi Robotics; PhD in AI and Robotics from UC Berkeley. getty Imagine your morning commute. You exit the highway and tap the brakes, but nothing happens. The car won't slow down. You frantically search for a safe place to coast, heart pounding, hoping to avoid a crash. Even after the brakes are repaired, would you trust that car again? Trust, once broken, is hard to regain. When it comes to physical products like cars, appliances or robots, reliability is everything. It's how we come to count on them for our jobs, well-being or lives. As with vehicles, reliability is critical to the success of AI-driven robots, from the supply chain to factories to our homes. While the stakes may not always be life-or-death, dependability still shapes how we trust robots, from delivering packages before the holidays to cleaning the house just in time for a dinner party. 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Space Elevators Could Totally Work—If Earth Days Were Much Shorter
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They're moving in a circular path as the Earth rotates. When an object moves in a circle, it has an acceleration toward the center. This centripetal acceleration has a magnitude that increases with the angular velocity (ω) as well as the radius of the circular path (r). The sum of the two forces (gravity and the scale) must equal the mass multiplied by the acceleration. This means that the force of the scale will be: Why is the north pole different? Yes, you are still rotating, but you are ON the axis of rotation, so the radius (your distance from the axis) is zero, and that gives you a zero acceleration. If you use an angular velocity for a 24-hour day, your effective weight at the equator is 99.7 percent of the value at the north pole. With a 12-hour day (which means the Earth is spinning twice as fast and your angular velocity is twice as high), the scale would read a value that's 98.6 percent of the actual gravitational force. The faster you spin, the lighter you are. Would you notice that in real life? I think that if you flew straight from the north pole to the equator, you might feel a change in effective weight of over 1 percent. With this lower weight, you could jump just a little bit higher and walk around with a lighter step. Space Elevators Let's think about orbits for a moment. If you put an object near the Earth, there will be a downward-pulling gravitational force. As you get farther away from the surface of the Earth, this gravitational force gets weaker. However, if you have an object in space that's initially at rest, the gravitational force will cause it to fall down and crash. But wait! If we use the same circular motion trick for the effective weight we can make the object move in a circle such that the mass multiplied by the centripetal acceleration is equal to the gravitational force. It would be the same as standing on a scale with an effective weight of zero. We call this a circular orbit. The rate that an object orbits depends on the distance from the center of the Earth (r). We can calculate that as: Here G is the universal gravitational constant and M is the mass of the Earth. If you put in a value of r that is 400 kilometers above the surface of the Earth, you get an angular velocity that would take the object 92 minutes to complete an orbit. Note: This is pretty much what the international space station (ISS) does. Wouldn't it be cool if the International Space System had a cable running down to the Earth? Unfortunately, the dangling cable would be whipping around the Earth so fast, you wouldn't be able to embark or disembark. Well, it's possible to fix this problem. Suppose you move the space station up to a distance of 36,000 kilometers instead of 400 kilometers? In that case, the angular velocity of the ISS would be the same as the rotation rate of the Earth. As seen from the surface of the Earth, the ISS would remain in the same spot in the sky because they would both take 24 hours to rotate. We call this a geostationary orbit—but it has to be directly over the equator so that the direction of the rotations are the same. With an object in geostationary orbit, you could run a cable down to the Earth. Boom —there's your space elevator. But wait! There are some problems. Can you imagine a cable that's 36,000 kilometers long? That's a LOT of cable. It's so much that you'd also have to counterbalance the weight of the cable with some big mass a little past the geostationary level. This system would require a tension in the material that exceeds the maximum value for the strongest steel cables. It could only work with something like a carbon nanotube cable—which we don't have (yet). OK, but what if we make the Earth spin twice as fast with a 12-hour day? In that case, a geostationary orbit would have a larger angular velocity (to match the faster Earth). If you crunch the numbers, the geostationary distance would be only 20,000 kilometers, or around 45 percent shorter. What if the Earth rotated so fast that the ISS was in a geostationary orbit just 400 kilometers above the surface? That might make the space elevator possible. Of course now we are going to have a MUCH shorter day of only 92 minutes. That's not worth it. Can you imagine having to get out bed every 92 minutes? I might even get dizzy. It's too bad because I really want a space elevator.

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