🚀 🌎 Exploring the universe and our home planet. Verification: nasa.gov/socialmedia
28.9% of @nasa's followers are female and 71.1% are male. Average engagement rate on the posts is around 0.49%. The average number of likes per post is 477,654 and the average number of comments is 1,332.
@nasa loves posting aboutPolitics, Space, Government Organization, Government Agencies.
96,845,010
Followers
0.49%
Engagement Rate
478,986
Engagement per post
477,654
Average likes per post
1,332
Average comments per post
74
Global Rank
26
Country Rank
1
Category Rank
Follower and Post Growth Trends
Engagement Rate Growth Trends
Audience Gender
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Recent Posts
Oh Dinkinesh, you are marvelous. 💫⁣ ⁣ On Nov. 1, our #LucyMission flew by the first of 10 asteroids in its planned 12-year mission. And it turns out that asteroid Dinkinesh is actually a party of two. ⁣ ⁣ This is why we explore. These images were captured while zooming by Dinkinesh at 10,000 mph (4.5 km/s) from 270 miles away (430 km) and reveal that the main belt asteroid, originally estimated to be one half-mile-wide asteroid, is made up of two asteroids of different sizes. From a preliminary analysis of these first images, the team estimates that the larger body is about 0.5 miles (790 m) at its widest, while the smaller is about 0.15 miles (220 m) in size.⁣ ⁣ Dinkinesh, meaning “you are marvelous,” is the Amharic name for Lucy, the ancient hominid discovered in Ethiopia for which our spacecraft is named. Dinkinesh truly lived up to its name.⁣ ⁣ The flyby was a test of Lucy’s terminal tracking systems, which Lucy passed with flying colors. The team will use the data from this encounter to prepare for the next close-up look at an asteroid, the main belt asteroid Donaldjohanson, in 2025. ⁣ ⁣ Image descriptions:⁣ 1) Two asteroids against black space. The larger is a diamond-shaped gray dusty rock lit from the right. The smaller, mostly spherical rock is visible behind the larger’s lower right edge.⁣ ⁣ 2) An animation of several images taken 13 seconds apart depicting the smaller asteroid passing from left to right behind the larger, spinning asteroid. The apparent motion of the two asteroids is due to the motion of the spacecraft as it flew past at 10,000 mph (4.5 km/s).⁣ ⁣ Credit:NASA/Goddard/SwRI/Johns Hopkins APL/ASU⁣ ⁣ #NASA #Space #Asteroids #Asteroid #Discovery #Lucy #Spacecraft #SpaceRocks
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If you got it, haunt it ⁣ ⁣ A pulsar wind nebula resembles a ghostly hand in a composite image captured by @NASAChandraXray and the Imaging X-ray Polarimetry Explorer (IXPE). The pulsar, a fast spinning dense neutron star, can be seen as a bright white spot near the base of the palm. The new combination with IXPE reveals the magnetic field “bones” of this remarkable structure. IXPE observed this pulsar, MSH 15-52, for 17 days which is the longest it has looked at any single object since it launched in December 2021. ⁣ ⁣ The second image shows the magnetic field map in MSH 15-52. In this image, short straight lines represent IXPE polarization measurements, mapping the direction of the local magnetic field. Orange “bars” mark the most precise measurements, followed by cyan and blue bars with less precise measurements. The complex field lines follow the `wrist', 'palm' and 'fingers' of the hand, and probably help define the extended finger-like structures.⁣ ⁣ The amount of polarization — indicated by bar length — is remarkably high, reaching the maximum level expected from theoretical work. To achieve that strength, the magnetic field must be very straight and uniform, meaning there is little turbulence in those regions of the pulsar wind nebula.⁣ ⁣ Image description: ⁣ 1- A composite image of a pulsar wind nebula, which strongly resembles a ghostly purple hand with sparkling fingertips. The three longest fingertips of the hand-shape point toward our upper right, or 1:00 on a clock face. There, a small, mottled, orange and yellow cloud appears to sparkle or glow like embers. This orange cloud is part of the remains of the supernova explosion that created the pulsar. The backdrop of stars was captured in infrared light. ⁣ 2- The second image is the same as the first, this time with magnetic field vectors in orange, cyan and blue. Their placement follows the structure of the hand, indicating the precision of measurements.⁣ ⁣ Credit: X-ray: NASA/CXC/Stanford Univ./R. Romani et al. (Chandra); NASA/MSFC (IXPE); Infrared: NASA/JPL-Caltech/DECaPS; Image Processing: NASA/CXC/SAO/J. Schmidt⁣ ⁣ #NASA #Space #chandra #Xray #Telescope #Astronomy #Spooky #Halloween
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I wanna dance with somebody 💃⁣ ⁣ This dance between two galaxies captured by @NASAHubble. Interacting gravitationally toward one another, these galaxies lie about 500 million light-years from Earth in the constellation Tucana. ⁣ ⁣ The interacting galaxy pair is known as Arp-Madore, which is a collection of peculiar galaxies. What is peculiar about this group? There are actually three galaxies, not just two. If you look at the smaller galaxy’s upper arm on the lower right corner of the image, you can spot the knot-like structure. As seen from Earth’s perspective, astronomers have found it challenging to differentiate whether an object in space is one, or multiple objects, or lying in front of another. Astronomers discovered the third knot-like galaxy by analyzing the speed and direction which revealed that the redshift, the wavelength of light is seen “shifted” towards the red part of the spectrum making it its own entity. ⁣ ⁣ Image description: Two spiral galaxies. Each glows brightly in the center, where a bar stretches from side to side. The upper one is rounder, and its arms form two thin rings. The lower galaxy is flatter and its arms make one outer ring; a dusty knot atop its upper arm marks out a third object. Gravity is pulling gas and dust together where the galaxies come close. A number of small galaxies surround them on a black background.⁣ ⁣ Credit: ESA/Hubble and NASA, J. Dalcanton, Dark Energy Survey/ DOE/ FNAL/ NOIRLab/ NSF/ AURA; Acknowledgement: L. Shatz⁣ ⁣ #Galaxy #Dance #Space #NASA #Hubble #Telescope #Astronomy #Stars ⁣
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We find magnetic fields very attractive 🧲⁣ ⁣ This image shows supernova remnant SN 1006. It combines data from our Imaging X-ray Polarimetry Explorer (IXPE) and @nasachandraxray. The red, green, and blue elements reflect low, medium, and high energy X-rays. The IXPE data, which measure the polarization of the X-ray light, is show in purple in the upper left corner, with the addition of lines representing the outward movement of the remnant’s magnetic field.⁣ ⁣ Researchers say the results show a connection between the magnetic fields and the remnants high-energy particle outflow. Mapping these magnetic field structures of supernova remnants at higher energies with enhanced detail and accuracy enables us to better understand the processes driving the acceleration of these particles.⁣ ⁣ SN 1006 is about 6,500 light-years from Earth in the Lupus constellation. It is the remains of a massive explosion which occurred with when two white dwarfs merged or when a white dwarf pulled too much mass from a companion star – creating what is thought to be the brightest stellar event recorded in history.⁣ ⁣ Image description: The debris from an exploded star resembles a mottled red ball of churning fire against a softer backdrop of stars. The supernova remnant appears to be encircled by a gauzy blue and white ring that is most prominent at our lower right and upper left. This structure is markedly different from other rounded supernova remnants. At the upper lefthand corner, a labeled section of SN 1006 is highlighted in a blue-tinted circle. Within this circle, only the outer ring of the supernova remnant is shown, not the mottled red stellar material churning inside. This ring is part of the supernova's expanding blast wave, which has been observed in X-ray light by both Chandra and IXPE. Magnetic field lines are illustrated in the circle as spiky, white lines, pointing mostly upwards and toward the left. The backdrop of stars was captured in infrared light by the Spitzer Space Telescope.⁣ ⁣ Credit: X-ray: NASA/CXC/SAO (Chandra); NASA/MSFC/Nanjing Univ./P. Zhou et al. (IXPE); IR: NASA/JPL/Caltech/Spitzer; Image Processing: NASA/CXC/SAO/J.Schmidt⁣ #NASA #Space #Supernova
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