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      These images captured by the Curiosity rover in 2014 reveals yet another unexplained aerial phenomenon in the Martian atmosphere, a cigar-shaped object with a consistent width and rounded ends. 

      What makes this anomaly particularly compelling is the sharp clarity of the image. According to Jean Ward the stars in the background appear crisp and unblurred, indicating that the object is not the result of motion blur or a long exposure. Notably, the object appears in five separate frames over an 8-minute span, suggesting it is moving relatively slowly through space, uncharacteristic of a meteorite entering the atmosphere. It also lacks the fiery tail typically associated with atmospheric entry. 

      Rather than a meteor, the object more closely resembles a solid, elongated craft of unknown origin. When oriented horizontally, it even appears to feature a front-facing structure, possibly a porthole or raised dome, hinting at a cockpit or command module. 

      Whether this object is orbiting beyond the visible horizon or connected to the surface far in the distance, its sheer size is unmistakable. Its presence raises compelling questions, could this be further evidence of intelligently controlled craft, whether of extraterrestrial or covert human origin, navigating through Martian airspace?View the full article
    • By NASA
      NASA/JPL-Caltech/ASU Arsia Mons, one of the Red Planet’s largest volcanoes, peeks through a blanket of water ice clouds in this image captured by NASA’s 2001 Mars Odyssey orbiter on May 2, 2025. Odyssey used a camera called the Thermal Emission Imaging System (THEMIS) to capture this view while studying the Martian atmosphere, which appears here as a greenish haze above the scene. A large crater known as a caldera, produced by massive volcanic explosions and collapse, is located at the summit. At 72 miles (120 kilometers) wide, the Arsia Mons summit caldera is larger than many volcanoes on Earth.
      Learn more about Arsia Mons and Mars Odyssey.
      Image Credit: NASA/JPL-Caltech/ASU
      View the full article
    • By NASA
      2 Min Read June’s Night Sky Notes: Seasons of the Solar System
      Two views of the planet Uranus appear side-by-side for comparison. At the top, left corner of the left image is a two-line label. The top line reads Uranus November 9, 2014. The bottoms line reads HST WFC3/UVIS. At the top, left corner of the right image is the label November 9, 2022. At the left, bottom corner of each image is a small, horizontal, white line. In both panels, over this line is the value 25,400 miles. Below the line is the value 40,800 kilometers. At the top, right corner of the right image are three, colored labels representing the color filters used to make these pictures. Located on three separate lines, these are F467M in blue, F547M in green, and F485M in red. On the bottom, right corner of the right image are compass arrows showing north toward the top and east toward the left. Credits:
      NASA by Kat Troche of the Astronomical Society of the Pacific
      Here on Earth, we undergo a changing of seasons every three months. But what about the rest of the Solar System? What does a sunny day on Mars look like? How long would a winter on Neptune be? Let’s take a tour of some other planets and ask ourselves what seasons might look like there.
      Martian Autumn
      Although Mars and Earth have nearly identical axial tilts, a year on Mars lasts 687 Earth days (nearly 2 Earth years) due to its average distance of 142 million miles from the Sun, making it late autumn on the red planet. This distance and a thin atmosphere make it less than perfect sweater weather. A recent weather report from Gale Crater boasted a high of -18 degrees Fahrenheit for the week of May 20, 2025.
      Credit: NASA/JPL-Caltech Seven Years of Summer
      Saturn has a 27-degree tilt, very similar to the 25-degree tilt of Mars and the 23-degree tilt of Earth. But that is where the similarities end. With a 29-year orbit, a single season on the ringed planet lasts seven years. While we can’t experience a Saturnian season, we can observe a ring plane crossing here on Earth instead. The most recent plane crossing took place in March 2025, allowing us to see Saturn’s rings ‘disappear’ from view.
      A Lifetime of Spring
      NASA Hubble Space Telescope observations in August 2002 show that Neptune’s brightness has increased significantly since 1996. The rise is due to an increase in the amount of clouds observed in the planet’s southern hemisphere. These increases may be due to seasonal changes caused by a variation in solar heating. Because Neptune’s rotation axis is inclined 29 degrees to its orbital plane, it is subject to seasonal solar heating during its 164.8-year orbit of the Sun. This seasonal variation is 900 times smaller than experienced by Earth because Neptune is much farther from the Sun. The rate of seasonal change also is much slower because Neptune takes 165 years to orbit the Sun. So, springtime in the southern hemisphere will last for several decades! Remarkably, this is evidence that Neptune is responding to the weak radiation from the Sun. These images were taken in visible and near-infrared light by Hubble’s Wide Field and Planetary Camera 2. Credit: NASA, L. Sromovsky, and P. Fry (University of Wisconsin-Madison) Even further away from the Sun, each season on Neptune lasts over 40 years. Although changes are slower and less dramatic than on Earth, scientists have observed seasonal activity in Neptune’s atmosphere. These images were taken between 1996 and 2002 with the Hubble Space Telescope, with brightness in the southern hemisphere indicating seasonal change.
      As we welcome summer here on Earth, you can build a Suntrack model that helps demonstrate the path the Sun takes through the sky during the seasons. You can find even more fun activities and resources like this model on NASA’s Wavelength and Energy activity. 
      View the full article
    • By NASA
      Curiosity Navigation Curiosity Home Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Images Videos Audio Mosaics More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions Mars Home 2 min read
      Sol 4546: Martian Jenga
      NASA’s Mars rover Curiosity acquired this image using its Left Navigation Camera on May 19, 2025 — Sol 4544, or Martian day 4,544 of the Mars Science Laboratory mission — at 02:23:29 UTC. NASA/JPL-Caltech Written by Michelle Minitti, Planetary Geologist at Framework
      Earth planning date: Monday, May 19, 2025
      Have you ever played the game Jenga, where you remove one wooden block from a stack, gently place it on another part of the stack, then repeat over and over as you try to keep the stack from toppling over? There are strategies to the game such as what blocks you can afford to remove, and where you can manage to place them without throwing the structure out of balance. That is very much how planning felt today — but instead of wooden blocks, the objects the science team was moving around were science observations in the plan.
      We had an unusual one-sol plan today so there were very restricted time windows in the plan in which to fit science observations and our next drive. We are driving through an area with criss-crossing fracture sets (which we call boxwork structures) large enough to be seen from orbit. Since they have only recently come within our view, there is no shortage of new observations to make of the fractures as we try to understand the processes that led to their formation. If the fractures were caused by extensive fluid flow through the Martian crust, understanding them would be an important contribution toward tracing the history of Martian water.
      To fit in all the desired observations — including APXS and MAHLI on a DRT-brushed target, multiple ChemCam RMI and Mastcam mosaics, and a ChemCam LIBS analysis — in addition to environmental monitoring activities and a long drive, the team used every trick in its book to achieve a delicate balancing act of science, time, and power. Some activities were trimmed to fit in smaller time windows, others were moved to less-constrained parts of the plan, and other activities were placed in parallel with each other to take advantage of Curiosity’s ability to multitask. 
      Once our planning Jenga game was over, the team had won — we had a complete and perfectly balanced plan! Who says you cannot teach an old dog (4,546-sols-old) new tricks?
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      Last Updated May 22, 2025 Related Terms
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