HR 8799 b is a Jovian planet, she is arrogant and vain, she loves fashion, and does not care about other people's opinions, but this causes conflict between her and her brothers, who do not like her arrogance, and ask her to stop, she becomes reflective , but does not show feelings that will change. The spectrum is consistent with field objects from early-L to T4 (3σ confidence level), with a best-fitting type of T2. It is 1.6 times more massive and 1.5 times bigger compared with our Sun. HR 8799 b; HR 8799 b is an exoplanet orbiting the star HR 8799, located about 131.7 light-years (40.4 pc) away from Solar System. HR 8799 hoặc V354 Pegasi là ngôi sao lớn hơn mặt trời khoảng 3 lần, có các hành tinh là HR 8799e,c,g,b. Cosponsors of H.R.8799 - 116th Congress (2019-2020): To prohibit transfers of individuals between ICE facilities and Federal, State, and local facilities, to ensure physical distancing inside ICE facilities, and for other purposes. hr 8799は、ペガスス座に属し、太陽系から129光年(39パーセク)の距離に存在する主系列星で、かじき座γ型 変光星である。 また、うしかい座λ型星にも分類される。 hr 8799という名称はハーバード改訂光度カタログにおける識別子である。 HR 8799 is ’n hoofreeksster van rofweg 30 miljoen jaar oud sowat 129 ligjare van die Aarde af in die sterrebeeld Vlieënde Perd.Sy massa is rofweg 1,5 keer dié van die Son en sy ligsterkte 4,9 keer die Son s'n. Dit is deel van ’n stelsel wat ook ’n rommelskyf en minstens vier gasreuse bevat. 어머니 항성은 겉보기 등급 6등성에 목동자리 람다형 항성이다. 질량은 목성의 5~11배, 반지름은 목성의 110~130퍼센트 정도일 것이다. Direct imaging of exoplanetary systems is a powerful technique that can reveal Jupiter-like planets in wide orbits, can enable detailed characterization of planetary atmospheres, and is a key step toward imaging Earth-like planets. hr 8799 b는 페가수스자리 방향으로 지구로부터 약 129 광년 떨어진 곳에 있는 항성 hr 8799 주위를 도는, 외계 행성이다. hr 8799 bは、先述の通り主星であるhr 8799よりかなり遠くに位置する。しかし、hr 8799が太陽の4.92倍明るい恒星であり、また惑星系の生成年代が2000万年から5000万年 と若いため 、表面温度は約600℃と高い 。 この温度により、直接撮影されるきっかけとなった赤外線を放出しており、その光度は … HR 8799 adalah bintang urutan utama berusia 30 juta tahun terletak 129 tahun cahaya (39,6 parsec) dari Bumi di konstelasi Pegasus.Bintang i ni memiliki sekitar 1,5 kali massa Matahari dan 4,9 kali luminositas matahari. Hành tinh có thể sống được là: HR 8799c và nó nặng hơn sao mộc khoảng 10 lần và lớn hơn 1,9 lần. Imaging detections are challenging because of the combined effect of small angular separation and large luminosity contrast between a planet and its host star. Bintang i ni adalah bagian dari sistem yang juga berisi disk puing dan setidaknya empat planet besar. . Too faint to have a proper or Greek letter name, or even a Flamsteed number, it is known best by its numbers in the Bright Star(HR) and the Henry Draper (HD) Catalogues.The temperature is measured at 7250 Kelvin. HR 8799 b on eksoplaneetta, joka löydettiin 13. marraskuuta 2008.Planeetta löydettiin kuvaamalla se suoraan. Se kiertää hieman Aurinkoa suurempaa A-tyypin pääsarjan tähteä HR 8799 noin 129 valovuoden päässä Maasta, Pegasuksen tähdistön suunnalla.. Planeetta kiertää emotähteään 68 AU:n etäisyydellä, ja sen kiertoaika on noin 450 vuotta. Its discovery was publicly announced on 2008. THE STAR HR 8799, also known as HD 218396, is a sixth magnitude (5.99) white, class A5 hydrogen fusing dwarf that lies just with the Great Square of Pegasus. The host star HR 8799 has apparent magnitude of 6.0, with absolute magnitude of 2.9. 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